Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

Abstract

We present here the final results of the Hubble Space Telescope Key Project to measure the Hubble constant. We summarize our method, the results and the uncertainties, tabulate our revised distances, and give the implications of these results for cosmology. The analysis presented here benefits from a number of recent improvements and refinements, including (1) a larger LMC Cepheid sample to define the fiducial period-luminosity (PL) relations, (2) a more recent HST Wide Field and Planetary Camera 2 (WFPC2) photometric calibration, (3) a correction for Cepheid metallicity, and (4) a correction for incompleteness bias in the observed Cepheid PL samples. New, revised distances are given for the 18 spiral galaxies for which Cepheids have been discovered as part of the Key Project, as well as for 13 additional galaxies with published Cepheid data. The new calibration results in a Cepheid distance to NGC 4258 in better agreement with the maser distance to this galaxy. Based on these revised Cepheid distances, we find values (in km/sec/Mpc) of H0 = 71 +/- 2 (random) +/- 6 (systematic) (type Ia supernovae), 71 +/- 2 +/- 7 (Tully-Fisher relation), 70 +/- 5 +/- 6 (surface brightness fluctuations), 72 +/- 9 +/- 7 (type II supernovae), and 82 +/- 6 +/- 9 (fundamental plane). We combine these results for the different methods with 3 different weighting schemes, and find good agreement and consistency with H0 = 72 +/- 8. Finally, we compare these results with other, global methods for measuring the Hubble constant.

Accepted to the Astrophysical Journal, 10 figures

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• Keck HIRES Spectroscopy of Extragalactic HII Regions: C and O Abundances from Recombination Lines
• Astrophysical Tests of Modified Gravity: Constraints from Distance Indicators in the Nearby Universe
• The Murmur of the Sleeping Black Hole: Detection of Nuclear Ultraviolet Variability in LINER Galaxies
• Modified Friedmann Equations from Tsallis Entropy
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• Ejection of the massive Hydrogen-rich envelope timed with the collapse of the stripped SN2014C
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• Host Galaxies Catalog Used in LIGO Searches for Compact Binary Coalescence Events
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• Reconstructed Density and Velocity Fields from the 2MASS Redshift Survey
• Internal Dynamics, Structure and Formation of Dwarf Elliptical Galaxies: I. A Keck/HST Study of Six Virgo Cluster Dwarfs
• On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002
• Inflation model constraints from the Wilkinson Microwave Anisotropy Probe three-year data
• New Optical Reddening Maps of the Large and Small Magellanic Clouds
• Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared
• GW170817 Falsifies Dark Matter Emulators
• A new upper limit on the total neutrino mass from the 2dF Galaxy Redshift Survey
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
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• The shear power spectrum from the COMBO-17 survey
• A Study of the Type II-Plateau Supernova 1999gi, and the Distance to its Host Galaxy, NGC 3184
• Lemaitre-Tolman-Bondi model and accelerating expansion
• The Colors of Dwarf Elliptical Galaxy Globular Cluster Systems, Nuclei and Stellar Halos
• The internal structure of the lens PG1115+080: breaking degeneracies in the value of the Hubble Constant
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data
• The Orbital Histories of Magellanic Satellites Using Gaia DR2 Proper Motions
• Observables sensitive to absolute neutrino masses. II
• The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
• Cosmological and astrophysical parameters from the SDSS flux power spectrum and hydrodynamical simulations of the Lyman-alpha forest
• Cosmological Parameters from the 2003 flight of BOOMERANG
• Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el
• Effect of inhomogeneities on the expansion rate of the Universe
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• The EFIGI catalogue of 4458 nearby galaxies with detailed morphology
• The Time Delays of Gravitational Lens HE0435-1223: An Early-Type Galaxy With a Rising Rotation Curve
• HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
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• Classical Cepheid Pulsation Models. X. The Period-Age Relation
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• The REFLEX Galaxy Cluster Survey VII: Omega_m and sigma_8 from cluster abundance and large-scale clustering
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• The M33 Metallicity Project: Resolving the Abundance Gradient Discrepancies in M33
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• The ACS Fornax Cluster Survey. VIII. The Luminosity Function of Globular Clusters in Virgo and Fornax Early-Type Galaxies and its Use as a Distance Indicator
• SFI++ I: A New I-band Tully-Fisher Template, the Cluster Peculiar Velocity Dispersion and H0
• Gravitational Lens Time Delays: A Statistical Assessment of Lens Model Dependences and Implications for the Global Hubble Constant
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• Quantitative Spectroscopy of 24 A supergiants in the Sculptor galaxy NGC 300: Flux weighted gravity luminosity relationship, metallicity and metallicity gradient
• A high redshift detection of the integrated Sachs-Wolfe effect
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• Inflation and WMAP three year data: Features have a Future!
• A Determination of H_0 with the CLASS Gravitational Lens B1608+656: III. A Significant Improvement in the Precision of the Time Delay Measurements
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• Strong gravitational lensing of explosive transients
• Investigations of dust heating in M81, M83, and NGC 2403 with the Herschel Space Observatory
• Ultra-luminous X-ray Sources in nearby galaxies from ROSAT HRI observations I. data analysis
• The Nature of UCDs: Internal Dynamics from an Expanded Sample and Homogeneous Database
• Spectral Models for Low-luminosity Active Galactic Nuclei in LINERs: The Role of Advection-dominated Accretion and Jets
• Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound
• (An)isotropy of the Hubble diagram: comparing hemispheres
• A Test of the Copernican Principle
• Extended Mid-Infrared Aromatic Feature Emission in M 82
• Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder
• Effective number of neutrinos and baryon asymmetry from BBN and WMAP
• Testing dark energy beyond the cosmological constant barrier
• A VLT study of metal-rich extragalactic H II regions. I. Observations and empirical abundances
• Internal Properties of Ultra-Compact Dwarf Galaxies in the Virgo Cluster
• Interpreting Cosmological Vacuum Decay
• The Hubble Constant from the Gravitational Lens B1608+656
• Pseudo-Dirac Neutrinos, a Challenge for Neutrino Telescopes
• Self-Similar Models for the Mass Profiles of Early-type Lens Galaxies
• Insights into the Cepheid distance scale
• Measuring the matter density using baryon oscillations in the SDSS
• Progress in the physics of massive neutrinos
• A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
• The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days
• Supernovae in Early-Type Galaxies: Directly Connecting Age and Metallicity with Type Ia Luminosity
• Astrometry with Hubble Space Telescope: A Parallax of the Fundamental Distance Calibrator RR Lyrae
• Challenges to the DGP Model from Horizon-Scale Growth and Geometry
• Anomalous extinction behaviour towards the Type Ia SN 2003cg
• NGC 300: an extremely faint, outer stellar disk observed to 10 scale lengths
• Rock 'n' Roll Solutions to the Hubble Tension
• The Geometric Distance and Proper Motion of the Triangulum Galaxy (M33)
• The electromagnetic counterparts of compact binary mergers
• Observational constraints on the curvaton model of inflation
• 2XMM Ultraluminous X-Ray Source Candidates in Nearby Galaxies
• Cosmicflows-4
• Metamorphosis of SN 2014C: Delayed Interaction Between a Hydrogen Poor Core-collapse Supernova and a Nearby Circumstellar Shell
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• The Cepheid Distance to NGC 1637: A Direct Test of the EPM Distance to SN 1999em
• The WSRT wide-field HI survey: II. Local Group features
• Hubble Diagrams of Type Ia Supernovae in the Near Infrared
• Constraints on the shape of the Milky Way dark matter halo from the Sagittarius stream
• The type IIb SN 2008ax: spectral and light curve evolution
• The AMIGA project. I. Optical characterization of the CIG catalog
• Ram Pressure Stripping of the Large Magellanic Cloud's Disk as a Probe of the Milky Way's Circumgalactic Medium
• New cosmological mass limit on thermal relic axions
• Evolution in the properties of Lyman-alpha emitters from redshifts z ~ 3 to z ~ 2
• Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest
• Composite Bulges: The Coexistence of Classical Bulges and Disky Pseudobulges in S0 and Spiral Galaxies
• The Araucaria Project. Near-Infrared Photometry of Cepheid Variables in the Sculptor Galaxy NGC 300
• How supernova explosions power galactic winds
• The Cluster Mass Function from Early SDSS Data: Cosmological Implications
• I Zw 18 revisited with HST/ACS and Cepheids: New Distance and Age
• High-redshift objects and the generalized Chaplygin gas
• Mirror dark matter and large scale structure
• The oxygen abundance in the inner HII regions of M101. Implications for the calibration of strong-line metallicity indicators
• The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33
• Median statistics and the Hubble constant
• Response of the Milky Way's disc to the Large Magellanic Cloud in a first infall scenario
• Cosmic shear results from the deep lens survey - I: Joint constraints on omega_m and sigma_8 with a two-dimensional analysis
• The underluminous Type Ia Supernova 2005bl and the class of objects similar to SN 1991bg
• Deep Hubble Space Telescope Imaging of IC 1613 II. The Star Formation History
• SN 2005bf: A Possible Transition Event Between Type Ib/c Supernovae and Gamma Ray Bursts
• Optical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002bo
• Cosmology of Mass-Varying Neutrinos Driven by Quintessence: Theory and Observations
• Chandra Detection of the First X-ray Forest along the Line of Sight To Mkn 421
• Constraining cosmological parameters using Sunyaev-Zel'dovich cluster surveys
• Towards Cosmological Concordance on Galactic Scales
• Clustering of Local Group distances: publication bias or correlated measurements? III. The Small Magellanic Cloud
• The Magellanic Cloud Calibration of the Galactic Planetary Nebula Distance Scale
• Cepheid calibration of type Ia Supernovae and the Hubble constant
• Constraints on cosmic opacity and beyond the standard model physics from cosmological distance measurements
• A Review of the Distance and Structure of the Large Magellanic Cloud
• The Dipole Anisotropy of the 2 Micron All-Sky Redshift Survey
• Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB
• Large-Scale Tests of the DGP Model
• The Star Formation Epoch of the Most Massive Early-Type Galaxies
• A measurement of the Hubble constant from Type II supernovae
• The Correlation between Dispersion Measure and X-ray Column Density from Radio Pulsars
• First Determination of the Distance and Fundamental Properties of an Eclipsing Binary in The Andromeda Galaxy
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• Absolute Values of Neutrino Masses: Status and Prospects
• The effect of metallicity on the Cepheid Period-Luminosity relation from a Baade-Wesselink analysis of Cepheids in the Galaxy and in the Small Magellanic Cloud
• Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
• Consistent estimates of (56)Ni yields for type Ia supernovae
• THINGS about MOND
• An alternative to the cosmological 'concordance model'
• Stellar velocity profiles and line strengths out to four effective radii in the early-type galaxies NGC 3379 and NGC 821
• The He-rich core-collapse supernova 2007Y: Observations from X-ray to Radio Wavelengths
• The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
• The Space Motion of Leo I: Hubble Space Telescope Proper Motion and Implied Orbit
• Early-universe constraints on a time-varying fine structure constant
• Core-collapse supernovae missed by optical surveys
• The PHANGS-HST Survey: Physics at High Angular resolution in Nearby GalaxieS with the Hubble Space Telescope
• Neutrino Mass and Dark Energy from Weak Lensing
• Chandra Survey of Nearby Highly-Inclined Disk Galaxies I: X-ray Measurements of Galactic Coronae
• Constraints on modified Chaplygin gas from recent observations and a comparison of its status with other models
• Dealing with systematics in cosmic shear studies: new results from the VIRMOS-Descart Survey
• Determining the Hubble constant from Hubble parameter measurements
• The Megamaser Cosmology Project: I. VLBI observations of UGC 3789
• The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS
• High Resolution Molecular Gas Maps of M33
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• Power of Observational Hubble Parameter Data: a Figure of Merit Exploration
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• Estimates of Cosmological Parameters Using the CMB Angular Power Spectrum of ACBAR
• FeII/MgII Emission Line Ratio in High Redshift Quasars
• Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data
• A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND
• Constraining Dark Energy with X-ray Galaxy Clusters, Supernovae and the Cosmic Microwave Background
• Light propagation in statistically homogeneous and isotropic dust universes
• The neutrino mass bound from WMAP-3, the baryon acoustic peak, the SNLS supernovae and the Lyman-alpha forest
• Type Ia Supernova Light Curve Inference: Hierarchical Bayesian Analysis in the Near Infrared
• Absolute-Magnitude Distributions and Light Curves of Stripped-Envelope Supernovae
• Time-dependent matter instability and star singularity in $F(R)$ gravity
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Type IIn Supernova SN 2010jl: Optical Observations for Over 500 Days After Explosion
• The bottleneck of the CNO burning and the age of the Globular Clusters
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• Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
• Constraining f(R) theories with the energy conditions
• Analysis of First LIGO Science Data for Stochastic Gravitational Waves
• Observational constraints on the dark energy and dark matter mutual coupling
• The Inner Halo of M87: A First Direct View of the Red-Giant Population
• The dispersion of growth of matter perturbations in f(R) gravity
• A List of Galaxies for Gravitational Wave Searches
• Cosmology with a Variable Chaplygin Gas
• Direct Distances to Cepheids in the Large Magellanic Cloud: Evidence for a Universal Slope of the Period-Luminosity Relation up to Solar Abundance
• The Cosmic Lens All-Sky Survey: statistical strong lensing, cosmological parameters, and global properties of galaxy populations
• The relations among 8, 24, and 160 micron dust emission within nearby spiral galaxies
• Type IIP Supernovae as Cosmological Probes: A SEAM Distance to SN 1999em
• The Rise and Fall of Type Ia Supernova Light Curves in the SDSS-II Supernova Survey
• The generalized second law of thermodynamics in the accelerating universe
• A measurement of Hubble's Constant using Fast Radio Bursts
• On the metallicity gradient of the Galactic disk
• The Planetary Nebula System of M33
• The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z~0.7
• The Relationship Between Intergalactic HI/OVI and Nearby (z<0.017) Galaxies
• Cosmology with photometric redshift surveys
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• The First Hours of the GW170817 Kilonova and the Importance of Early Optical and Ultraviolet Observations for Constraining Emission Models
• Joint CMB and Weak Lensing Analysis; Physically Motivated Constraints on Cosmological Parameters
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• Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations
• Peanuts at an Angle: Detecting and Measuring the Three-Dimensional Structure of Bars in Moderately Inclined Galaxies
• The Chandra ACIS Survey of M33: X-ray, Optical and Radio Properties of the Supernova Remnants
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• The DECam Local Volume Exploration Survey: Overview and First Data Release
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• Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound
• The Dark Universe
• A Magellanic Origin for the Warp of the Galaxy
• Intracluster Planetary Nebulae in the Virgo Cluster III: Luminosity of the Intracluster Light and Tests of the Spatial Distribution
• Cepheid Calibration of the Peak Brightness of SNe Ia. XI. SN 1998aq in NGC 3982
• The stellar population histories of early-type galaxies. III. The Coma Cluster
• Cosmological Signatures of Interacting Neutrinos
• Dark matter in elliptical galaxies: I. Is the total mass density profile of the NFW form or even steeper?
• Connecting Far-Infrared and Radio Morphologies of Disk Galaxies: Cosmic-Ray Electron Diffusion After Star Formation Episodes
• Simulating the gamma-ray emission from galaxy clusters: a universal cosmic ray spectrum and spatial distribution
• Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
• Cepheid pulsation models at varying metallicity and DY/DZ
• The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for its Tidal Disruption
• Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance
• Current cosmological bounds on neutrino masses and relativistic relics
• Cepheid distances from infrared long-baseline interferometry - I. VINCI/VLTI observations of seven Galactic Cepheids
• Formation and evolution of dwarf elliptical galaxies I. Structural and kinematical properties
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Observational Constraints on General Relativistic Energy Conditions, Cosmic Matter Density and Dark Energy from X-Ray Clusters of Galaxies and Type-Ia Supernovae
• The Formation of the First Stars in the Universe
• An updated Gamma Ray Bursts Hubble diagram
• Isotropic Luminosity Indicators in a Complete AGN Sample
• The Globular Cluster Luminosity Function and Specific Frequency in Dwarf Elliptical Galaxies
• The Discovery of Cepheids and a Distance to NGC 5128
• Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results
• A Sudden Gravitational Transition
• New constraints on MOND from galaxy clusters
• COSMOGRAIL XVI: Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring
• Searches for Giant Pulses from Extragalactic Pulsars
• The Dynamical Status of the Cluster of Galaxies 1E0657-56
• The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
• A multi-wavelength study of z = 3.15 Lyman-alpha emitters in the GOODS South Field
• Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter
• Improved constraints on H0 from a combined analysis of gravitational-wave and electromagnetic emission from GW170817
• Constraining the quintessence equation of state with SnIa data and CMB peaks
• Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data
• Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
• The normal Type Ia SN 2003hv out to very late phases
• Supernova cosmology: legacy and future
• Structure, mass and distance of the Virgo cluster from a Tolman-Bondi model
• Constraining Inverse Curvature Gravity with Supernovae
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• A new extragalactic distance determination method using the flux-weighted gravity of late B and early A supergiants
• Dynamical masses of ultra-compact dwarf galaxies in Fornax
• Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant
• On the Progenitor of Binary Neutron Star Merger GW170817
• Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
• Age Problem in the Holographic Dark Energy Model
• Friedmann cosmology with decaying vacuum density
• The ACS Virgo Cluster Survey XI. The Nature of Diffuse Star Clusters in Early-Type Galaxies
• Chandra Acis Survey of X-Ray Point Sources in 383 Nearby Galaxies I. the Source Catalog
• The VMC Survey IV. The LMC star formation history and disk geometry from four VMC tiles
• An Accelerating Cosmology Without Dark Energy
• Constraining dark energy with Sunyaev-Zel'dovich cluster surveys
• The shape of the dark matter halo in the early-type galaxy NGC 2974
• On Absorption by Circumstellar Dust, With the Progenitor of SN2012aw as a Case Study
• Prospects for Determining the Equation of State of the Dark Energy: What can be Learned from Multiple Observables?
• Surface Brightness Fluctuations in the Hubble Space Telescope ACS/WFC F814W Bandpass and an Update on Galaxy Distances
• Constraint on Coupled Dark Energy Models from Observations
• Constraints on Dark Energy from Supernovae, Gamma Ray Bursts, Acoustic Oscillations, Nucleosynthesis and Large Scale Structure and the Hubble constant
• Cosmological parameters from strong gravitational lensing and stellar dynamics in elliptical galaxies
• Nonlinear Structure Formation and "Apparent" Acceleration: an Investigation
• Sample variance in the local measurements of the Hubble constant
• Constraints on Chaplygin quartessence from the CLASS gravitational lens statistics and supernova data
• Cosmic microwave background and large scale structure limits on the interaction between dark matter and baryons
• Characteristics of the Galaxy according to Cepheids
• Optical spectroscopy of metal-rich HII regions and circumnuclear hot spots in M83 and NGC 3351
• Constraining The Early-Universe Baryon Density And Expansion Rate
• Constraints on the Sound Speed of Dynamical Dark Energy
• Constraining the dark energy with galaxy clusters X-ray data
• The Metallicity Distribution of Intracluster Stars in Virgo
• Growth factor parametrization and modified gravity
• The Next Generation Virgo Cluster Survey (NGVS). XVIII. Measurement and Calibration of Surface Brightness Fluctuation Distances for Bright Galaxies in Virgo (and Beyond)
• The Type Ia supernova 2004S, a clone of SN 2001el, and the optimal photometric bands for extinction estimation
• Observational constraints on Hubble constant and deceleration parameter in power-law cosmology
• Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMC
• HI Fluctuations at Large Redshifts: I--Visibility correlation
• Energy Conditions and Cosmic Acceleration
• The Star Formation in Radio Survey: GBT 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions
• The Statistical Significance of the Low CMB Mulitipoles
• A Swift survey of accretion onto stellar-mass black holes
• Lower limits on the Hubble Constant from models of Type Ia Supernovae
• The Incidence of Highly-Obscured Star-Forming Regions in SINGS Galaxies
• Noether symmetry approach in phantom quintessence cosmology
• Globular cluster luminosity function as distance indicator
• Spectroscopic Gravitational Lensing and Limits on the Dark Matter Substructure in Q2237+0305
• Can a matter-dominated model with constant bulk viscosity drive the accelerated expansion of the universe?
• The Hubble Constant
• The 3D Structure of the Virgo Cluster Region from Tully-Fisher and HI Data
• CMB power spectra from cosmic strings: predictions for the Planck satellite and beyond
• Primordial Neutrinos
• Light propagation in statistically homogeneous and isotropic universes with general matter content
• Constraints on massive sterile neutrino species from current and future cosmological data
• Dynamics of the Magellanic Clouds in a LCDM Universe
• The $\gamma$-ray Emission of Star-Forming Galaxies
• The Outer Disks of Early-Type Galaxies. II. Surface-Brightness Profiles of Unbarred Galaxies and Trends with Hubble Type
• Real-time Cosmology
• WMAPping inflationary physics
• Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars
• Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
• Multiple Major Outbursts from a Restless Luminous Blue Variable in NGC 3432
• A preference for a non-zero neutrino mass from cosmological data
• The Beginning and Evolution of the Universe
• Is Our Universe Likely to Decay within 20 Billion Years?
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• 3D Velocity and Density Reconstructions of the Local Universe with Cosmicflows-1
• Measuring the value of the Hubble constant "à la Refsdal"
• Spitzer Infrared Spectrograph Observations of Magellanic Cloud Planetary Nebulae: the nature of dust in low metallicity circumstellar ejecta
• Supernova 2012aw - a high-energy clone of archetypal type IIP SN 1999em
• Hierarchical Star-Formation in M33: Fundamental properties of the star-forming regions
• Sloan Digital Sky Survey Spectroscopic Lens Search. I. Discovery of Intermediate-Redshift Star-Forming Galaxies Behind Foreground Luminous Red Galaxies
• Constraints on the sound speed of dark energy
• Exploring a matter-dominated model with bulk viscosity to drive the accelerated expansion of the Universe
• When Is a Bulge Not a Bulge? Inner Disks Masquerading as Bulges in NGC 2787 and NGC 3945
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
• The Galactic Nova Rate Revisited
• Late-Time Optical Emission From Core-Collapse Supernovae
• The formation of stellar nuclear discs in bar-induced gas inflows
• Luminous Supersoft X-Ray Sources in External Galaxies
• Scale dependence of cosmological backreaction
• Galactic abundance gradients from Cepheids : On the iron abundance gradient around 10-12 kpc
• f(R) theories of gravity in Palatini approach matched with observations
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Explosion Energies, Nickel Masses, and Distances of Supernovae of Type IIP
• The distance of M33 and the stellar population in its outskirts
• Optical Observations of LIGO Source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica
• Optical and IR observations of SN 2002dj: some possible common properties of fast expanding SNe Ia
• On the Progenitors of Two Type II-P Supernovae in the Virgo Cluster
• The CMB cold spot: texture, cluster or void?
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• WMAP and Inflation
• Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant
• Observational bounds on the cosmic radiation density
• A Field Theory Model for Dark Matter and Dark Energy in Interaction
• Cosmological parameter estimation using Very Small Array data out to l=1500
• Voids as a Precision Probe of Dark Energy
• Improved constraints on cosmological parameters from SNIa data
• Mid-Infrared Spectroscopy of Lensed Galaxies at 1<z<3: The Nature of Sources Near the MIPS Confusion Limit
• Structural Properties of Ultra-Compact Dwarf Galaxies in the Fornax and Virgo Clusters
• Interacting Ghost Dark Energy in Non-Flat Universe
• Determining $H_0$ with Bayesian hyper-parameters
• An independent determination of the local Hubble constant
• Old-Aged Stellar Population Distance Indicators
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• Does the fine-structure constant vary with cosmological epoch?
• Optical and Infrared Photometry of the Nearby Type Ia Supernovae 1999ee, 2000bh, 2000ca, and 2001ba
• The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• XMM observation of M~87 II. Abundance structure of the interstellar and intergalactic medium
• The Detection of a Light Echo from the Type Ia Supernova 2006X in M100
• The Lyman-alpha forest and WMAP year three
• The Opacity of Spiral Galaxy Disks IV: Radial Extinction Profiles from Counts of Distant Galaxies seen through Foreground Disks
• The EPOCH Project: I. Periodic variable stars in the EROS-2 LMC database
• Theoretical models for classical Cepheids. VIII. Effects of helium and heavy elements abundance on the Cepheid distance scale
• On the onset of cosmological backreaction
• Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae
• Near-Infrared Photometry of the Type IIn SN 2005ip: The Case for Dust Condensation
• The Type IIP Supernova 2012aw in M95: hydrodynamical modelling of the photospheric phase from accurate spectrophotometric monitoring
• Dark Coupling and Gauge Invariance
• Lightest Neutralino in Extensions of the MSSM
• Upper limits on neutrino masses from the 2dFGRS and WMAP: the role of priors
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• The Baryonic Tully-Fisher Relationship for S${}^4$G Galaxies and the "Condensed" Baryon Fraction of Galaxies
• The Metallicity Dependence of the High-Mass X-ray Binary Luminosity Function
• Thermal history of the plasma and high-frequency gravitons
• Constraints on backreaction in dust universes
• A census of X-ray nuclear activity in nearby galaxies
• Investigating dark energy experiments with principal components
• Fueling AGN-I: How the Global Characteristics of the Central Kiloparsec of Seyferts differ from Quiescent Galaxies
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• The JCMT Nearby Galaxies Legacy Survey VIII. CO data and the L(CO3-2)-L(FIR) correlation in the SINGS sample
• Spectral Energy Distributions of Weak Active Galactic Nuclei Associated With Low-Ionization Nuclear Emission Regions
• Dark Energy Constraints from Galaxy Cluster Peculiar Velocities
• Future Evolution of Structure in an Accelerating Universe
• The early-type dwarf galaxy population of the Hydra I cluster
• Pulsation and evolutionary masses of classical Cepheids. I. Milky Way variables
• Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory
• HST/WFPC2 Color-Magnitude Diagrams for Globular Clusters in M31
• On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations
• The Frequency and Stellar-Mass Dependence of Boxy/Peanut-Shaped Bulges in Barred Galaxies
• The Hubble time inferred from 10 time-delay lenses
• Dust and the type II-Plateau supernova 2004dj
• Searching for a holographic connection between dark energy and the low-l CMB multipoles
• Bolometric Light Curves for 33 Type II-Plateau Supernovae
• Toward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure
• Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
• The Abundance Scatter in M33 from HII Regions: Is There Any Evidence for Azimuthal Metallicity Variations?
• Testing intermediate-age stellar evolution models with VLT photometry of LMC clusters. III. Padova results
• Cosmological constraints on Chaplygin gas dark energy from galaxy clusters X-ray and supernova data
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• CMB polarization power spectra contributions from a network of cosmic strings
• Infall of nearby galaxies into the Virgo cluster as traced with HST
• Spectroscopic Observations of SN 2012fr: A Luminous Normal Type Ia Supernova with Early High Velocity Features and Late Velocity Plateau
• Red and dead: The progenitor of SN 2012aw in M95
• The Ages and Abundances of a Sample of Globular Clusters in M49 (NGC 4472)
• HST Snaphot Study of Variable Stars in Globular Clusters: Inner Region of NGC 6441
• SN 2004A: Another Type II-P Supernova with a Red Supergiant Progenitor
• The intergalactic medium thermal history at redshift z=1.7--3.2 from the Lyman alpha forest: a comparison of measurements using wavelets and the flux distribution
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• A Package for the Automated Classification of Periodic Variable Stars
• Cosmicflows-2: I-band Luminosity - HI Linewidth Calibration
• Mass Modeling of Disk Galaxies: Constraints, Degeneracies and Adiabatic Contraction
• High Redshift Quasars and Star Formation in the Early Universe
• Comparison of Distances from RR Lyrae Stars, the Tip of the Red-Giant Branch and Classical Cepheids
• Unified dark energy models : a phenomenological approach
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• Exact likelihood evaluations and foreground marginalization in low resolution WMAP data
• Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
• Constraining amplitude and slope of the mass fluctuation spectrum using cluster baryon mass function
• Spatially Resolved Ultraviolet, H-alpha, Infrared, and Radio Star Formation in M81
• Cepheids in Open Clusters: An 8-D All-sky Census
• Constraints on Distance Duality Relation from Sunyaev Zel'dovich Effect and Chandra X-ray measurements
• The Formation of the Local Group Planes of Galaxies
• A Study of Edge-On Galaxies with the Hubble Space Telescope's Advanced Camera for Surveys. I. Initial Results
• Effects of Explosion Asymmetry and Viewing Angle on the Type Ia Supernova Color and Luminosity Calibration
• The Megamaser Cosmology Project. II. The Angular-Diameter Distance to UGC 3789
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• The Multi-Wavelength Tully-Fisher relation with spatially resolved HI kinematics
• Evaluating backreaction with the peak model of structure formation
• Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics
• The Araucaria Project. Determination of the LMC Distance from Late-Type Eclipsing Binary Systems: I. OGLE-051019.64-685812.3
• Evolution in the Color-Magnitude Relation of Early-Type Galaxies in Clusters of Galaxies at z~=1
• The age problem in $\Lambda$CDM model
• Constraints on f(R) Cosmology in the Palatini Formalism
• On using the CMB shift parameter in tests of models of dark energy
• Cosmic shear analysis of archival HST/ACS data: I. Comparison of early ACS pure parallel data to the HST/GEMS Survey
• The Hubble constant from gravitational lens CLASS B0218+357 using the Advanced Camera for Surveys
• Star-Formation Rates of Local Blue Compact Dwarf Galaxies I: 1.4 GHz and 60 um luminosities
• Constraints on a mixed inflaton and curvaton scenario for the generation of the curvature perturbation
• The Color-Magnitude Relation for Metal-Poor Globular Clusters in M87: Confirmation From Deep HST/ACS Imaging
• How flat can you get? A model comparison perspective on the curvature of the Universe
• The SAURON Project - XIX. Optical and near-infrared scaling relations of nearby elliptical, lenticular and Sa galaxies
• The radial extinction profiles of late-type galaxies
• HALOGAS: Extraplanar gas in NGC 3198
• GMC Evolutions in the Nearby Spiral Galaxy M33
• Optical and Infrared Photometry of the Unusual Type Ia Supernova 2000cx
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods
• K-Band Red Clump Distance to the Large Magellanic Cloud
• Constraining the orbital history of the Magellanic Clouds: A new bound scenario suggested by the tidal origin of the Magellanic Stream
• Photometric Observations of the Type Ia SN 2002er in UGC 10743
• The VMC Survey. V. First results for Classical Cepheids
• Early-type Galaxy Distances from the Fundamental Plane and Surface Brightness Fluctuations
• The JCMT Nearby Galaxies Legacy Survey III: Comparisons of cold dust, polycyclic aromatic hydrocarbons, molecular gas, and atomic gas in NGC 2403
• Constraints on flat cosmologies with tracking Quintessence from Cosmic Microwave Background observations
• Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• Dynamical Constraints on The Masses of the Nuclear Star Cluster and Black Hole in the Late-Type Spiral Galaxy NGC 3621
• Models for the lens and source of B0218+357 - A LensClean approach to determine H0
• The PL calibration for Milky Way Cepheids and its implications for the distance scale
• Dynamical versus Stellar Masses of Ultracompact Dwarf Galaxies in the Fornax Cluster
• Local Group Dwarf Elliptical Galaxies: I. Mapping the Dynamics of NGC 205 Beyond the Tidal Radius
• Photometry of the Type Ia Supernovae 1999cc, 1999cl, and 2000cf
• The Distances to Open Clusters from Main-Sequence Fitting. IV. Galactic Cepheids, the LMC, and the Local Distance Scale
• Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background
• The Massive Progenitor of the Possible Type II-Linear Supernova 2009hd in Messier 66
• Deriving accurate peculiar velocities (even at high redshift)
• Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
• Probing the Friedmann equation during recombination with future CMB experiments
• Determination of the Hubble constant, the intrinsic scatter of luminosities of Type Ia SNe, and evidence for non-standard dust in other galaxies
• A Machian Model of Dark Energy
• A Study of Cepheids in M81 with the Large Binocular Telescope (Efficiently Calibrated with HST)
• No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data
• Radial Metallicity Distribution Breaks at Corotation Radius in Spiral Galaxies
• PKS 1830-211: A Face-On Spiral Galaxy Lens
• Entropy Injection as a Global Feedback Mechanism
• Brane inflation and the WMAP data: a Bayesian analysis
• Parallax Beyond a Kiloparsec from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope
• The Araucaria Project. The Distance to the Local Group Galaxy IC 1613 from Near-Infrared Photometry of Cepheid Variables
• A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder
• Scaling Laws for Dark Matter Halos in Late-Type and Dwarf Spheroidal Galaxies
• Tracking Dark Energy with the ISW effect: short and long-term predictions
• The past and future dynamics of quintom dark energy models
• The Very Massive Star Content of the Nuclear Star Clusters in NGC 5253
• Ionized gas kinematics and massive star formation in NGC 1530
• A pulsational distance to Omega Centauri based on Near-Infrared Period-Luminosity relations of RR Lyrae stars
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• Falsifying Paradigms for Cosmic Acceleration
• Near-Ultraviolet Properties of a Large Sample of Type Ia Supernovae as Observed with the Swift UVOT
• A Novel Color Parameter As A Luminosity Calibrator for Type Ia Supernovae
• The Internal Ultraviolet-to-Optical Color Dispersion: Quantifying the Morphological K-Correction
• A 5% measurement of the Hubble constant from Type II supernovae
• Unmasking the Supernova Impostors
• Beyond the perfect fluid hypothesis for dark energy equation of state
• Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• KL Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early SDSS Data
• Spatially resolved LMC star formation history: I. Outside in evolution of the outer LMC disk
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• A Spitzer IRS Spectral Atlas of Luminous 8 micron Sources in the Large Magellanic Cloud
• The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period-Luminosity Relations
• The first year of SN 2004dj in NGC 2403
• Cosmology with the Square Kilometre Array
• New near-infrared period-luminosity-metallicity relations for RR Lyrae stars and the outlook for Gaia
• Cosmic Bulk Flow and the Local Motion from Cosmicflows-2
• Testing For Azimuthal Abundance Gradients In M101
• Toward a New Geometric Distance to the Active Galaxy NGC4258: I. VLBI Monitoring of Water Maser Emission
• Early-time Spitzer observations of the type II-Plateau supernova, 2004dj
• Magnetized CMB observables: a dedicated numerical approach
• Determination of the Distance to M33 Based on the Tip of the Red Giant Branch and the Red Clump
• Distance Determination To Eight Galaxies Using Expanding Photosphere Method
• Theoretical uncertainty in baryon oscillations
• Age constraints and fine tuning in variable-mass particle models
• X-rays from the Globular Cluster G1: Intermediate Mass Black Hole or Low Mass X-ray Binary?
• Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
• The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101
• Calibration of the Mid-Infrared Tully-Fisher Relation
• Lookback time as a test for brane cosmology
• New optical and near-infrared Surface Brightness Fluctuations models. A primary distance indicator ranging from Globular Clusters to distant galaxies?
• The Carnegie Hubble Program: The Leavitt Law at 3.6 μm and 4.5 μm in the Large Magellanic Cloud
• An improved cosmological bound on the thermal axion mass
• Discovery of Water Maser Emission in Eight AGN with 70-m Antennas of NASA's Deep Space Network
• Constraints on Type Ia Supernova Progenitor Companions from Early Ultraviolet Observations with Swift
• Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71. I. Simultaneous broadband observations during November 2003
• X-ray emission from the extended disks of spiral galaxies
• Hubble flow variance and the cosmic rest frame
• On the association between core-collapse supernovae and HII regions
• The Subluminous Supernova 2007qd: A Missing Link in a Family of Low-Luminosity Type Ia Supernovae
• The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 micron surface brightness ratios
• The early-type dwarf galaxy population of the Centaurus cluster
• An old quasar in a young dark energy-dominated universe?
• The Parsec-scale Accretion Disk in NGC 3393
• The Brightest Young Star Clusters in NGC 5253
• Improved Constraints on the Gravitational Lens Q0957+561. II. Strong Lensing
• Constraints on cosmological parameters in power-law cosmology
• The contribution of galaxies to the UV ionising background and the evolution of the Lyman forest
• Further empirical evidence for the non-linearity of the period-luminosity relations as seen in the Large Magellanic Cloud Cepheids
• The Abundance Gradient in the Extremely Faint Outer Disk of NGC 300
• Making Sense Of The New Cosmology
• Strong Gravitational Lensing Time Delay Statistics and the Density Profile of Dark Halos
• Formation of the black-hole binary M33 X-7 via mass-exchange in a tight massive system
• The VMC Survey. XIII. Type II Cepheids in the Large Magellanic Cloud
• Planetary Nebula Spectrograph survey of S0 galaxy kinematics. II. Clues to the origins of S0 galaxies
• A Global Model of The Light Curves and Expansion Velocities of Type II-Plateau Supernovae
• SN 2002cv: A Heavily Obscured Type Ia Supernova
• Photometry of SN 2002ic and Implications for the Progenitor Mass-Loss History
• Observational Constraints on Chaplygin Quartessence: Background Results
• Halos of Spiral Galaxies. I. The Tip of the Red Giant Branch as a Distance Indicator
• SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• A Bayesian analysis of the primordial power spectrum
• Reproducing Cosmic Microwave Background anisotropies with mixed isocurvature perturbations
• The Case for Omega_M = 0.33 +/- 0.035
• SN 2006gy: was it really extra-ordinary?
• Gemini observations of Wolf-Rayet Stars in the Local Group Starburst Galaxy IC10
• Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Observational constraints on cosmology from modified Friedmann equation
• Observational constraints on late-time Lambda(t) cosmology
• Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies
• Intermediate-band Surface Photometry of the Edge-on Galaxy: NGC 4565
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• The Globular Cluster Systems in the Coma Ellipticals. IV: WFPC2 Photometry for Five Giant Ellipticals
• Radio and X-rays From SN 2013df Enlighten Progenitors of Type IIb Supernovae
• Distance determination to 12 Type II-P Supernovae using the Expanding Photosphere Method
• Cepheid distances from the SpectroPhoto-Interferometry of Pulsating Stars (SPIPS) - Application to the prototypes delta Cep and eta Aql
• Measuring the cosmological background of relativistic particles with WMAP
• Cepheid theoretical models and observations in HST/WFC3 filters: the effect on the Hubble constant Ho
• Cosmological Constraints on a Power Law Universe
• Do Distinct Cosmological Models Predict Degenerate Halo Populations?
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Constraints on the cosmic neutrino background
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds
• Distance determination to 12 Type II Supernovae using the Expanding Photosphere Method
• The Old Host-Galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational Wave Source
• A Spectroscopic and Photometric Survey of Novae in M31
• The Arecibo Legacy Fast ALFA Survey: IX. The Leo Region HI Catalog, Group Membership and the HI Mass Function for the Leo I Group
• Cosmology of neutrinos and extra light particles after WMAP3
• Neutrino mass limits from SDSS, 2dFGRS and WMAP
• SN 1993J VLBI (III): The Evolution of the Radio Shell
• A New Estimate of the Hubble Time with Improved Modeling of Gravitational Lenses
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• SN 2012fr: Ultraviolet, Optical, and Near-Infrared Light Curves of a Type Ia Supernova Observed Within a Day of Explosion
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Cosmological Constraints from Gravitational Lens Time Delays
• The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations
• The exact numerical treatment of inflationary models
• Globular Cluster and Galaxy Formation: M31, the Milky Way and Implications for Globular Cluster Systems of Spiral Galaxies
• Clustering of Local Group distances: publication bias or correlated measurements? II. M31 and beyond
• Testing CPT Symmetry with CMB Measurements
• Gone without a bang: An archival HST survey for disappearing massive stars
• Age of High Redshift Objects - a Litmus Test for the Dark Energy Models
• Three dimensional maps of the Magellanic Clouds using RR~Lyrae stars and Cepheids - I. The Large Magellanic Cloud
• An optical time delay for the double gravitational lens system FBQ 0951+2635
• Are cosmological neutrinos free-streaming?
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• Nebular Spectra of 111 Type Ia Supernovae Disfavor Single Degenerate Progenitors
• The Progenitor of the Type Ia Supernova that created SNR 0519-69.0 in the Large Magellanic Cloud
• The Standardizability of Type Ia Supernovae in the Near-Infrared: Evidence for a Peak Luminosity-Decline Rate Relation in the Near-Infrared
• Cosmic Equation of state from Strong Gravitational Lensing Systems
• Problems with Time-Varying Extra Dimensions or "Cardassian Expansion" as Alternatives to Dark Energy
• Constraining Modified Gravity and Growth with Weak Lensing
• A New Method for Measuring Extragalactic Distances
• The Araucaria Project. The Distance to the Local Group Galaxy NGC 6822 from Cepheid Variables discovered in a Wide-Field Imaging Survey
• Optical and near-infrared photometry of the Type Ia Supernova 2000E in NGC 6951
• Constraining Van der Waals quintessence by observations
• WMAP constraints on inflationary models with global defects
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• The Eclipsing Binary Cepheid OGLE-LMC-CEP-0227 in the Large Magellanic Cloud: pulsation modelling of light and radial velocity curves
• NGC 604, the Scaled OB Association (SOBA) Prototype. I: Spatial Distribution of the Different Gas Phases and Attenuation by Dust
• Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
• Can Dark Matter Decay in Dark Energy?
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Cosmic Flows : Green Bank and Parkes HI observations
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Redshift-Independent Distances in the NASA/IPAC Extragalactic Database: Methodology, Content and Use of NED-D
• The early-type dwarf galaxy population of the Fornax cluster
• Reconciling the local void with the CMB
• Quasar Parallax: a Method for Determining Direct Geometrical Distances to Quasars
• Observational constraint on generalized Chaplygin gas model
• The local Hubble flow: a manifestation of dark energy
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• HI Signal from Reionization Epoch
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Global Star Formation Rates and Dust Emission Over the Galaxy Interaction Sequence
• Forecasting the Bayes factor of a future observation
• Supernova Relic Neutrinos in Liquid Argon detectors
• A Concordance Model of the Lyman-alpha Forest at z = 1.95
• PHANGS-HST: Star Cluster Spectral Energy Distribution Fitting with CIGALE
• Metallicity-corrected Tip of the Red Giant Branch Distance to NGC 4258
• Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited
• First results from the Very Small Array -- IV. Cosmological parameter estimation
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• The Multiphase Intergalactic Medium towards PKS 2155-304
• Parallax of Galactic Cepheids from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope: The Case of SS Canis Majoris
• The Carnegie Hubble Program
• Uncertainties on the theoretical predictions for classical Cepheid pulsational quantities
• Extraordinary Late-Time Infrared Emission of Type IIn Supernovae
• Model-independent constraints on the cosmic opacity
• The VMC survey -- XLIII. The spatially resolved star formation history across the Large Magellanic Cloud
• Luminosity Indicators in the Ultraviolet Spectra of Type Ia Supernovae
• NGC 300 OT2008-1 As a Scaled-Down Version of the Eta Carinae Great Eruption
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• The Discovery of Cepheids and a New Distance to NGC 2841 Using the Hubble Space Telescope
• A Deep Chandra ACIS Survey of M83
• The Existence of an Old Quasar at $z=3.91$ and its Implications for $\Lambda (t)$ Deflationary Cosmologies
• Can scale-dependent cosmology alleviate the $H_0$ tension?
• Testing the Copernican Principle via Cosmological Observations
• The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations
• Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
• Extended quintessence with an exponential coupling
• GaBoDS: The Garching-Bonn Deep Survey -- I. Anatomy of galaxy clusters in the background of NGC 300
• Cosmic viscosity as a remedy for tension between PLANCK and LSS data
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Weak lensing in generalized gravity theories
• Quantifying the Faint Structure of Galaxies: The Late-type Spiral NGC 2403
• First Gaia Local Group Dynamics: Magellanic Clouds Proper Motion and Rotation
• Measuring the cosmological bulk flow using the peculiar velocities of supernovae
• Proper Motion Study of the Magellanic Clouds using SPM material
• X-ray Emitting GHz-Peaked Spectrum Galaxies: Testing a Dynamical-Radiative Model with Broad-Band Spectra
• The expansion field: The value of H_0
• Core collapse supernovae as Cosmic Ray sources
• The fast declining Type Ia supernova 2003gs, and evidence for a significant dispersion in near-infrared absolute magnitudes of fast decliners at maximum light
• SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phase
• Cosmic microwave anisotropies from BPS semilocal strings
• On the Progenitor and Supernova of the SN 2002cx-like Supernova 2008ge
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• SN 1993J VLBI (IV): A Geometric Determination of the Distance to M81 with the Expanding Shock Front Method
• Empirical calibration of the reddening maps in the Magellanic Clouds
• The High Redshift Integrated Sachs-Wolfe Effect
• The value of the equation of state of dark energy
• The Photometric Plane of Elliptical Galaxies
• Surface Brightness Profiles of Dwarf Galaxies: I. Profiles and Statistics
• Holographic hessence models
• The isocurvature fraction after WMAP 3-year data
• Cosmological model with interactions in the dark sector
• Evidence for an Intermediate-Mass Black Hole: Chandra and XMM-Newton Observations of the Ultraluminous Supersoft X-ray Source in M101 during its 2004 Outburst
• Generation of Magnetic Field in the Pre-recombination Era
• Cosmological measure with volume averaging and the vacuum energy problem
• Kinematics of the Atomic ISM in M33 on 80 pc scales
• The Spectral Energy Distributions of White Dwarfs in 47 Tucanae: The Distance to the Cluster
• Remarks on the formulation of the cosmological constant/dark energy problems
• Statefinder diagnostic for the modified polytropic Cardassian universe
• The Carnegie-Chicago Hubble Program. IX. Calibration of the Tip of the Red Giant Branch Method in the Mega-Maser Host Galaxy, NGC4258 (M106)
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• The Recent Cluster Formation Histories of NGC 5253 and NGC 3077: Environmental Impact on Star Formation
• Requiem for an FCHAMP?
• The Araucaria Project. A Distance Determination to the Local Group Spiral M33 from Near-Infrared Photometry of Cepheid Variables
• The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae
• The very young resolved stellar populations around stripped-envelope supernovae
• Comparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies
• Revealing Type Ia supernova physics with cosmic rates and nuclear gamma rays
• Old, Metal-Poor Extreme Velocity Stars in the Solar Neighborhood
• The non-Gaussianity of the cosmic shear likelihood - or: How odd is the Chandra Deep Field South?
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• Reconciliation of the Surface Brightness Fluctuations and Type Ia Supernovae Distance Scales
• Lookback time bounds from energy conditions
• Unified 1-D Simulations of Gamma-Ray Line Emission from Type Ia Supernovae
• Hypervelocity stars in the Gaia era: Runaway B stars beyond the velocity limit of classical ejection mechanisms
• The Discovery of Quasisoft and Supersoft Sources in External Galaxies
• The Road to Precision Cosmology
• Revisiting the abundance gradient in the maser host galaxy NGC 4258
• The Hubble constant inferred from 18 time-delay lenses
• Cosmological Information from Quasar-Galaxy Correlations induced by Weak Lensing
• Cosmological implications of APM 08279+5255, an old quasar at z = 3.91
• Testing The Friedmann Equation: The Expansion of the Universe During Big-Bang Nucleosynthesis
• Photometric Solutions for Detached Eclipsing Binaries: selection of ideal distance indicators in the SMC
• Current Observational Constraints on Cosmic Doomsday
• CCD time-series photometry of the globular cluster NGC 6981: Variable star census and physical parameter estimates
• The Carnegie-Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch
• Is the present expansion of the universe really accelerating?
• Detailed HI kinematics of Tully-Fisher calibrator galaxies
• The Heraklion Extragalactic Catalogue (HECATE): a value-added galaxy catalogue for multi-messenger astrophysics
• WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation
• The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
• Determining Cosmological Parameters with Latest Observational Data
• Unresolved and diffuse components of X-ray emission and X/K luminosity ratios in nearby early-type and late-type galaxies
• Can all cosmological observations be accurately interpreted with a unique geometry?
• Baryon asymmetry from hypermagnetic helicity in dilaton hypercharge electromagnetism
• Late universe dynamics with scale-independent linear couplings in the dark sector
• Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
• Globular Clusters and the Mira Period-Luminosity Relation
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Time-dependent lepto-hadronic modeling of the emission from blazar jets with SOPRANO: the case of TXS 0506+056, 3HSP J095507.9+355101 and 3C 279
• Swiss Cheese and a Cheesy CMB
• Cosmological parameter estimation and Bayesian model comparison using VSA data
• The signature of dark energy on the local Hubble flow
• The Araucaria Project. The Distance of the Large Magellanic Cloud from Near-Infrared Photometry of RR Lyrae Variables
• Thick Disks of Lenticular Galaxies
• Growth factor parametrization in curved space
• Optical observations of type IIP supernova 2004dj: Evidence for the asymmetry of ${}^{56}$Ni ejecta
• Metallicity gradients in small and nearby spiral galaxies
• Is there a concordance value for $H_0$?
• A Council of Giants
• Inflationary Potential Reconstruction for a WMAP Running Power Spectrum
• Metallicity gradients in Local Universe galaxies: time evolution and effects of radial migration
• Reconstruction of the Primordial Power Spectrum by Direct Inversion
• Confrontation of MOND Predictions with WMAP First Year Data
• Dynamical Models of Elliptical Galaxies in z=0.5 Clusters: II. Mass-to-Light Ratio Evolution without Fundamental Plane Assumptions
• $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
• A Bayesian Analysis of the Cepheid Distance Scale
• Gemini GMOS spectroscopy of HeII nebulae in M33
• A Classical Cepheid in a LMC eclipsing binary: evidence of shortcomings in current stellar evolutionary models?
• Pulsation Models for Ultra-Low (Z=0.0004) Metallicity Classical Cepheids
• Observational constraints on the LLTB model
• The Type Ib SN 1999dn: One Year of Photometric and Spectroscopic Monitoring
• Do observations prove that cosmological neutrinos are thermally distributed?
• The Linearity of the Wesenheit function for the Large Magellanic Cloud Cepheids
• New coupled quintessence cosmology
• Cosmological constraints combining H(z), CMB shift and SNIa observational data
• Cosmic rays and non-thermal emission in simulated galaxies. II. $\gamma$-ray maps, spectra and the far infrared-$\gamma$-ray relation
• Interacting Energy Components and Observational $H(z)$ Data
• Testing SNe Ia distance measurement methods with SN 2011fe
• Quintessence Cosmology and the Cosmic Coincidence
• Cold gas in a complete sample of group-dominant early-type galaxies
• RR Lyrae-based calibration of the Globular Cluster Luminosity Function
• Measuring our universe from galaxy redshift surveys
• Internal dynamics of the Large Magellanic Cloud from Gaia DR2
• Chandra ACIS Survey of M33 (ChASeM33): A First Look
• Surface Brightness Fluctuations of Fornax Cluster Galaxies: Calibration of Infrared SBFs and Evidence for Recent Star Formation
• Kinematics and Mass Modeling of Messier 33: Halpha observations
• The quiescent Hubble flow, local dark energy tests, and pairwise velocity dispersion in a $\Omega =1$ universe
• Infrared Properties of Star Forming Dwarf Galaxies: I. Dwarf Irregular Galaxies in the Local Volume
• A Two-Component Power Law Covering Nearly Four Orders of Magnitude in the Power Spectrum of Spitzer Far-Infrared Emission from the Large Magellanic Cloud
• The JCMT Nearby Galaxies Legacy Survey IV. Velocity Dispersions in the Molecular Interstellar Medium in Spiral Galaxies
• Two New Tests of the Metallicity Sensitivity of the Cepheid Period-Luminosity Relation (The Leavitt Law)
• New Evidence for Mass Loss from delta Cephei from HI 21-cm Line Observations
• Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621
• Consequences on some dark energy-candidates from the type Ia supernova SN 1997ff
• Testing AGN outflow and accretion models with CIV and HeII emission line demographics in z=2 quasars
• Determination of the Distance to M33 Based on Single Epoch I-band HST Observations of Cepheids
• Surface Brightness Fluctuations from archival ACS images: a stellar population and distance study
• The Gravitational Lens -- Galaxy Group Connection. II. Groups Associated with B2319+051 and B1600+434
• WISDOM project -- V. Resolving molecular gas in Keplerian rotation around the supermassive black hole in NGC 0383
• On the Nature of Star Formation at Large Galactic Radii
• Testing galaxy formation models with the GHOSTS survey: The color profile of M81's stellar halo
• Time Delay Lens Modelling Challenge
• Constraining ultra-compact dwarf galaxy formation with galaxy clusters in the local universe
• An improved approach to measuring H_0 using X-ray and SZ observations of galaxy clusters
• Applications of Bayesian model averaging to the curvature and size of the Universe
• Halos of Spiral Galaxies. III. Metallicity Distributions
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Emergent Universe from Scale Invariant Two Measures Theory
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Period-Luminosity Relations for Type II Cepheids and their Application
• Observational Constraints on Silent Quartessence
• Primordial magnetic fields and formation of molecular hydrogen
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes
• Spatially Resolved Kinematics of an Ultra-Compact Dwarf Galaxy
• Probing the Effective Number of Neutrino Species with Cosmic Microwave Background
• The population of planetary nebulae and HII regions in M81. A study of radial metallicity gradients and chemical evolution
• Dark energy as a mirage
• A QUMOND galactic N-body code I: Poisson solver and rotation curve fitting
• Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
• X-ray Source Population in the Elliptical Galaxy NGC 720 with Chandra
• Carbon Monoxide in the Type Ic SN 2000ew
• Science Programs for a 2 m-class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope
• The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations
• The VMC Survey. VIII. First results for Anomalous Cepheids
• Testing CPT Symmetry with CMB Measurements: Update after WMAP5
• M31N 2007-11d: A Slowly-Rising, Luminous Nova in M31
• Is the evidence for dark energy secure?
• Can Brans-Dicke scalar field account for dark energy and dark matter?
• Primordial Nucleosynthesis with varying fundamental constants: A semi-analytical approach
• Possible Detection of Baryonic Fluctuations in the Large-Scale Structure Power Spectrum
• Gaia DR2 reveals a very massive runaway star ejected from R136
• Globular cluster clustering and tidal features around ultra compact dwarf galaxies in the halo of NGC1399
• Minimization of Biases in Galaxy Peculiar Velocity Catalogs
• The JCMT Nearby Galaxies Legacy Survey II: Warm Molecular Gas and Star Formation in Three Field Spiral Galaxies
• Quantitative spectral analysis of early B-type supergiants in the Sculptor galaxy NGC 300
• WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
• Planetary nebulae in M33: probes of AGB nucleosynthesis and ISM abundances
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• Production and dilution of gravitinos by modulus decay
• HST Photometry for the Halo Stars in the Leo Elliptical NGC 3377
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• The Araucaria Project: The effect of blending on the Cepheid distance to NGC 300 from Advanced Camera for Surveys images
• Reconstructing Cepheid Light Curve with Fourier Techniques I: The Fourier Expansion and Interrelations
• Ultraviolet Observations of Super-Chandrasekhar Mass Type Ia Supernova Candidates with Swift UVOT
• $H_0$ from ten well-measured time delay lenses
• The Size of the Radio-Emitting Region in Low-luminosity Active Galactic Nuclei
• Constraining the shape of the CMB: a Peak-by-Peak analysis
• A new search for features in the primordial power spectrum
• Forecasting Cosmic Doomsday from CMB/LSS Cross-Correlations
• Gravitational Lens Time Delays in CDM
• The MACHO Project Large Magellanic Cloud Variable Star Inventory. XIII. Fourier Parameters for the First Overtone RR Lyrae Variables and the LMC Distance
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• Detection of CO Hotspots Associated with Young Clusters in the Southern Starburst Galaxy NGC 1365
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• On Neural Architectures for Astronomical Time-series Classification with Application to Variable Stars
• TESS observations of Cepheid stars: first light results
• Measuring distances to low-luminosity galaxies using surface brightness fluctuations
• The Cosmological Mean Density and its Local Variations Probed by Peculiar Velocities
• Reconstructing the primordial power spectrum from the CMB
• The Spatially Resolved Dust-to-Metals Ratio in M101
• A massive warm baryonic halo in the Coma cluster
• The Period-Luminosity Relation for the Large Magellanic Cloud Cepheids Derived from Spitzer Archival Data
• The distance to Hydra and Centaurus from surface brightness fluctuations: Consequences for the Great Attractor model
• Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters
• Testing Cosmology with Cosmic Sound Waves
• The Araucaria Project. The Distance to the Sculptor Galaxy NGC 247 from Near-Infrared Photometry of Cepheid Variables
• WMAP 3-year primordial power spectrum
• Hubble Space Telescope Observations of cD Galaxies and their Globular Cluster Systems
• A large Wolf-Rayet population in NGC300 uncovered by VLT-FORS2
• Swift Ultraviolet Observations of Supernova 2014J in M82: Large Extinction from Interstellar Dust
• Cosmic age problem revisited in the holographic dark energy model
• Age constraints on the cosmic equation of state
• A Global Physical Model for Cepheids
• Kinematic Structure in the Galactic Halo at the North Galactic Pole: RR Lyrae and BHB Stars show different kinematics
• Constraints on growth index parameters from current and future observations
• Progenitors of low-luminosity Type II-Plateau supernovae
• Exploring the evidence for a large local void with supernovae Ia data
• Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
• Galaxy Mass Models: MOND versus Dark Matter Halos
• Type Ia Supernovae are Excellent Standard Candles in the Near-Infrared
• Low-l CMB Power Loss in String Inflation
• Large-scale magnetic fields from inflation due to Chern-Simons-like effective interaction
• Is Our Universe Decaying at an Astronomical Rate?
• Searches for Ultra-Compact Dwarf Galaxies in Galaxy Groups
• Chandra & XMM-Newton Observations of NGC5253. Analysis of the X-ray Emission from a Dwarf Starburst Galaxy
• Constraints on Kinetically Modified Inflation from WMAP5
• Lens Galaxy Properties of SBS1520+530: Insights from Keck Spectroscopy and AO Imaging
• Screening of cosmological constant for De Sitter Universe in non-local gravity, phantom-divide crossing and finite-time future singularities
• Early Dark Energy at High Redshifts: Status and Perspectives
• The Araucaria Project. An improved distance to the Sculptor spiral galaxy NGC 300 from its Cepheid variables
• Low-Level Nuclear Activity in Nearby Spiral Galaxies
• High-precision distance measurements with classical pulsating stars
• New CMBR data and the cosmic neutrino background
• Type Ia Supernovae and Cosmology
• The VMC Survey. XIX. Classical Cepheids in the Small Magellanic Cloud
• Revisiting the ultraluminous supersoft source in M101: an optically thick outflow model
• A Comparison of surface brightness profiles for ultra-compact dwarfs and dwarf elliptical nuclei: implications for the `threshing' scenario
• On the 3 dimensional structure of edge-on disk galaxies
• On the density of Cold Dark Matter
• Accuracy of environmental tracers and consequence for determining the Type Ia Supernovae magnitude step
• The Chandra ACIS Survey of M33 (ChASeM33): The final source catalog
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• The metallicity dependence of the Cepheid PL-relation
• Using Ultra Long Period Cepheids to Extend the Cosmic Distance Ladder to 100 Mpc and Beyond
• The spectacular evolution of Supernova 1996al over 15 years: a low energy explosion of a stripped massive star in a highly structured environment
• Global and Local Effects of Rotation: Observational Aspects
• Cosmological implications and structure formation from a time varying vacuum
• The Mira Distance to M101 and a 4% Measurement of H0
• An Unusual Spectral State of an Ultra-luminous Very Soft X-ray Source during Outburst
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• A New Catalogue of Galactic Novae: Investigation of the MMRD relation & Spatial Distribution
• Detecting Topology in a Nearly Flat Spherical Universe
• A Point Source Excess in Abell 1185: Intergalactic Globular Clusters?
• Forecasts for Dark Energy Measurements with Future HI Surveys
• The XMM-{\em Newton}/2dF Survey - VI: Clustering and Bias of the Soft X-ray Point Sources
• Evolution of the Dark Matter Distribution with 3-D Weak Lensing
• High spatial resolution mid-infrared spectroscopy of NGC 5253: The stellar content of the embedded super-star cluster
• Observational Constraints on Superbubble X-ray Energy Budgets
• Distances to Populous Clusters in the LMC via the K-Band Luminosity of the Red Clump
• Bar imprints on the inner gas kinematics of M33
• Infrared Surface Brightness Fluctuations of the Coma Elliptical NGC 4874 and the Value of the Hubble Constant
• Model-independent dark energy test with sigma_8 using results from the Wilkinson Microwave Anisotropy Probe
• The Planetary Nebula Spectrograph survey of S0 galaxy kinematics. Data and Overview
• The Gamma-Ray Emitting Radio-Loud Narrow-Line Seyfert 1 Galaxy PKS 2004-447 II. The Radio View
• Inflows and Outflows in the Dwarf Starburst Galaxy NGC 5253: High-Resolution HI Observations
• A First Glimpse of String Theory in the Sky?
• Carbon, nitrogen and oxygen abundance gradients in M101 and M31
• Observational constraints on particle production during inflation
• A "pulsational" distance determination for the Large Magellanic Cloud
• The signature of dark energy perturbations in galaxy cluster surveys
• Theoretical Limb Darkening for Pulsating Cepheids
• Estimating Luminosity Function Constraints from High-Redshift Galaxy Surveys
• Pseudospectrum of de Sitter black holes
• Noether analysis of Scalar-Tensor Cosmology
• Cosmicflows-2: SNIa Calibration and H0
• Some remarks about non-minimally coupled scalar field models
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• A Luminous Recurrent Supersoft X-ray Source in NGC 300
• What the small angle CMB really tells us about the curvature of the Universe
• Parametrized modified gravity constraints after Planck
• Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
• Dust Attenuation in Hydrodynamic Simulations of Spiral Galaxies
• Resolving the Stellar Population of the Standard Elliptical Galaxy NGC3379
• Fine Tuning Free Paradigm of Two Measures Theory: K-Essence, Absence of Initial Singularity of the Curvature and Inflation with Graceful Exit to Zero Cosmological Constant State
• Rendering Dark Energy Void
• A CO J=3-2 map of M51 with HARP-B: Radial properties of the spiral structure
• On the temperature profile of radiatively efficient geometrically thin disks in black hole binaries with the ASCA GIS
• Current and future supernova constraints on decaying $\Lambda$ cosmologies
• Primordial magnetic fields and the HI signal from the epoch of reionization
• Seven years of coordinated Chandra-NuSTAR observations of SN2014C unfold the extreme mass-loss history of its stellar progenitor
• Status of Cold Dark Matter Cosmology
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• The Planetary Nebula Luminosity Function at the Dawn of Gaia
• Structure and kinematics of edge-on galaxy discs -- IV. The kinematics of the stellar discs
• LOSS's First Supernova? New Limits on the "Impostor" SN 1997bs
• Recurrent Novae in M31
• Cosmological limit on the neutrino mass
• Impact of Chandra calibration uncertainties on galaxy cluster temperatures: application to the Hubble Constant
• Is There a Disc in the Superluminal Quasars?
• Non-Friedmann cosmology for the Local Universe, significance of the universal Hubble constant and short-distance indicators of dark energy
• Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions
• MMT Spectroscopy of Supernova Remnant Candidates in M33
• Supernova 1954J (Variable 12) in NGC 2403 Unmasked
• The dark haloes of early-type galaxies in low-density environments: XMM-Newton and Chandra observations of NGC 57, NGC 7796 and IC 1531
• A new perspective on the relation between dark energy perturbations and the late-time ISW effect
• Can Planck-scale physics be seen in the cosmic microwave background ?
• Global 8.4-GHz VLBI observations of JVAS B0218+357
• Light to Mass Variations with Environment
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• CCD time-series photometry of the globular cluster NGC 5053: RR Lyrae, Blue Stragglers and SX Phoenicis stars revisited
• The Cepheid Period-Luminosity Relation at Mid-Infrared Wavelengths: I. First-Epoch LMC Data
• Source subtraction for the extended Very Small Array and 33-GHz source count estimates
• The Globular Cluster System of the Virgo Dwarf Elliptical Galaxy VCC 1087
• The luminosity of supernovae of type Ia from TRGB distances and the value of H_0
• Holography and the large number hypothesis
• The VMC survey - XXIII. Model fitting of light and radial velocity curves of Small Magellanic Cloud classical Cepheids
• The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics
• The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
• Near-infrared light curves of Type Ia supernovae: Studying the properties of the second maximum
• Cosmological CPT Violation, Baryon/Leptogenesis and CMB Polarization
• Insights on bar quenching from a multi-wavelength analysis: The case of Messier 95
• The Mass, Baryonic Fraction, and X-ray Temperature of the Luminous, High Redshift Cluster of Galaxies, MS0451.6-0305
• Cepheid distances from infrared long-baseline interferometry - II. Calibration of the Period-Radius and Period-Luminosity relations
• On a century of extragalactic novae and the rise of the rapid recurrent novae
• Photometric Properties of the M33 Star Cluster System
• A comprehensive study of Cepheid variables in the Andromeda galaxy. Period distribution, blending and distance determination
• Calibrating Type Ia Supernovae using the Planetary Nebula Luminosity Function I. Initial Results
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• On Cepheid Distance Scale Bias due to Stellar Companions and Cluster Populations
• Determining the equation of state of dark energy from angular size of compact radio sources and X-ray gas mass fraction of galaxy clusters
• Detectability of a phantom-like braneworld model with the integrated Sachs-Wolfe effect
• The global stability of M33: still a puzzle
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• The Long-Lived UV "Plateau" of SN 2012aw
• Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - II. Kinematics
• A unified model for age-velocity dispersion relations in Local Group galaxies: Disentangling ISM turbulence and latent dynamical heating
• The Tully-Fisher Relation for 25,000 SDSS Galaxies as Function of Environment
• A Panoply of Cepheid Light Curve Templates
• An Oxygen Abundance Gradient into the Outer Disk of M81
• Breaking the self-averaging properties of spatial galaxy fluctuations in the Sloan Digital Sky Survey - Data Release Six
• Type II-P supernovae as standardised candles: improvements using near infrared data
• Toward an internally consistent astronomical distance scale
• Cosmological parameters and the WMAP data revisited
• Extended Born-Infeld Dynamics and Cosmology
• CMB constraints on the fine structure constant
• Model Independent Primordial Power Spectrum from Maxima, Boomerang, and DASI Data
• Beyond Two Dark Energy Parameters
• Precision Cosmology
• A Chandra view of NGC 3621: a bulgeless galaxy hosting an AGN in its early phase?
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Calibration of the distance scale from galactic Cepheids:II Use of the HIPPARCOS calibration
• The Distance to M101 Hosting Type Ia SN 2011fe Based on the Tip of the Red Giant Branch
• An extended theoretical scenario for Classical Cepheids. I. Modeling Galactic Cepheids in the Gaia photometric system
• Supernova tests of the timescape cosmology
• The metallicity - redshift relations for emission-line SDSS galaxies: examination of the dependence on the star formation rate
• The Opacity of Spiral Galaxy Disks III: Automating the "Synthetic Field Method"
• Virialization of cosmological structures in models with time varying equation of state
• The angular size - redshift relation in power-law cosmologies
• The Selection Function of SZ Cluster Surveys
• The Nature and Geometry of the Light Echo from SN 2006X
• Supernova SN 2012dn: A spectroscopic clone of SN 2006gz
• Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations
• NGC 770: A Counter-Rotating Core in a Low-Luminosity Elliptical Galaxy
• On the photometric variability of blue supergiants in NGC 300 and its impact on the Flux-weighted Gravity-Luminosity Relationship
• How did the Virgo cluster form?
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• Non-linear perturbations in scalar-tensor cosmologies
• Properties of RR Lyrae stars in the inner regions of the Large Magellanic Cloud. II. The extended sample
• On the Recovery of the Star Formation History of the LMC from the VISTA Survey of the Magellanic System
• GAIA and the Extragalactic Distance Scale
• Coupled quintessence and vacuum decay
• Cosmological constraints on the Hu-Sawicki modified gravity scenario
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• The Cold Dark Matter crisis on galactic and subgalactic scales
• The first two transient supersoft X-ray sources in M 31 globular clusters and the connection to classical novae
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• The Cepheid Period-Luminosity Relation at Mid-Infrared Wavelengths: II. Second-Epoch LMC Data
• Affine parameterization of the dark sector: costraints from WMAP5 and SDSS
• New Baade-Wesselink distances and radii for four metal-rich Galactic Cepheids
• Confronting dark energy models mimicking $\Lambda$CDM epoch with observational constraints: future cosmological perturbations decay or future Rip?
• Observational constraints on generalized Chaplygin gas model
• Reddening map and recent star formation in the Magellanic Clouds based on OGLE IV Cepheids
• The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source
• Are Type Ia Supernovae in Restframe $H$ Brighter in More Massive Galaxies?
• Initial conditions for quintessence after inflation
• Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
• The Star Formation in Radio Survey: 3 - 33 GHz Imaging of Nearby Galaxy Nuclei and Extranuclear Star-forming Regions
• Dark energy, gravitation and supernovae
• Two classes of fast-declining type Ia supernovae
• Constraints on Neutrino Degeneracy from the Cosmic Microwave Background and Primordial Nucleosynthesis
• Measuring the Chaplygin gas equation of state from angular and luminosity distances
• Legacy data and cosmological constraints from the angular-size/redshift relation for ultra-compact radio sources
• The Extinction and Distance of Maffei 1
• Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II Supernovae
• Observational tests for Λ(t)CDM cosmology
• Natural Phantom Dark Energy, Wiggling Hubble Parameter $H(z)$ and Direct $H(z)$ Data
• A Chandra ACIS Observation of the X-ray Luminous SN1988Z
• Can Old Galaxies at High Redshifts and Baryon Acoustic Oscillations Constrain H_0?
• A Study on the Chemical Properties of Blue Compact Dwarf Galaxies
• Optical Surface Brightness Fluctuations of shell galaxies towards 100 Mpc
• Vetting Galactic Leavitt Law Calibrators using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids
• Precise reddening and metallicity of NGC6752 from FLAMES spectra
• Evidence for a Black Hole Remnant in the Type IIL Supernova 1979C
• Theoretical fit of Cepheid light an radial velocity curves in the Large Magellanic Cloud cluster NGC 1866
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• The distance to NGC1316 (Fornax A): yet another curious case
• The Neutral Hydrogen Content of Fornax Cluster Galaxies
• VLT observations of metal-rich extra galactic HII regions. I. Massive star populations and the upper end of the IMF
• The distribution of dark and luminous matter inferred from extended rotation curves
• Infrared Properties of Star Forming Dwarf Galaxies: Blue Compact Dwarfs in the Virgo Cluster
• Do We Have Evidence for New Physics in the Sky?
• An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
• Hubble Space Telescope Observations of Star Clusters in M101
• Exotic Low Density Fermion States in the Two Measures Field Theory: Neutrino Dark Energy
• Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
• CORS Baade-Wesselink method in the Walraven photometric system: the Period-Radius and the Period-Luminosity relation of Classical Cepheids
• Property of the spectrum of large-scale magnetic fields from inflation
• Extended Tidal Structure In Two Lyman Alpha-Emitting Starburst Galaxies
• Unified model of baryonic matter and dark components
• H-alpha Imaging of Early-type (Sa-Sab) Spiral Galaxies II. Global Properties
• Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE
• The Distance to the Massive Eclipsing Binary LMC-SC1-105 in the Large Magellanic Cloud
• Confronting the Hubble Diagram of Gamma-Ray Bursts with Cardassian Cosmology
• A Direct Stellar Metallicity Determination in the Disk of the Maser Galaxy NGC4258
• Ejection of Supernova-Enriched Gas From Dwarf Disk Galaxies
• Constraints on the Cosmological Relativistic Energy Density
• A supernova distance to the anchor galaxy NGC 4258
• The Most Slowly Declining Type Ia Supernova 2001ay
• The Globular Cluster System of NGC4374
• Identification of 13 Cepheids and 333 Other Variables in M31
• Optical and Near-Infrared Observations of the Peculiar Type Ia Supernova 1999ac
• Clustering, Angular Size and Dark Energy
• Exploring Parameter Constraints on Quintessential Dark Energy: the Inverse Power Law Model
• Spectroscopy of planetary nebulae in M33
• Concerning the Classical Cepheid VIc Wesenheit Function's Strong Metallicity Dependence
• The NGC 5253 star cluster system. I. Standard modelling and infrared-excess sources
• The Opacity of Spiral Galaxy Disks VI: Extinction, stellar light and color
• An Unbiased Measurement of Ho through Cosmic Background Imager Observations of the Sunyaev-Zel'dovich Effect in Nearby Galaxy Clusters
• Backreaction of Cosmological Perturbations in Covariant Macroscopic Gravity
• The Cosmic Neutrino Background and the Age of the Universe
• Two Fluid Scenario in Bianchi Type-I Universe
• First results from SAPAC: towards a 3D-picture of the Fornax cluster core
• TeV physics and the Planck scale
• The Star Formation in Radio Survey: Jansky Very Large Array 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions
• Discs in early-type lensing galaxies: effects on magnification ratios and measurements of $H_0$
• Synthetic photometry for carbon-rich giants. III. Tracing the sequence of mass-losing galactic C-type Miras
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• An extensive catalogue of early-type galaxies in the nearby Universe
• Semi-analytical approach to magnetized temperature autocorrelations
• On the dependence between UV luminosity and Lyman-alpha equivalent width in high redshift galaxies
• The Dark Matter Distribution in the Spiral $NGC3198$ out to 0.22 $R_{vir}$
• Constraining $H_0$ from Sunyaev-Zel'dovich effect, Galaxy Clusters X-ray data, and Baryon Oscillations
• Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
• The Astrophysical Distance Scale III: Distance to the Local Group Galaxy WLM using Multi-Wavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars
• The Progenitors and Lifetimes of Planetary Nebula
• Surface brightness fluctuation distances for nearby dwarf elliptical galaxies
• The EFIGI catalogue of 4458 nearby galaxies with morphology II. Statistical properties along the Hubble sequence
• The peculiar Ca-rich SN 2019ehk: Evidence for a Type IIb core-collapse supernova from a low mass stripped progenitor
• Modelling the flyby anomalies using a modification of inertia
• Study of changes in the pulsation period of 148 Galactic Cepheid variables
• Period-luminosity relations for Galactic Cepheid variables with independent distance measurements
• Constraining the time variation of the coupling constants from cosmic microwave background: effect of Λ_{QCD}
• Late-time Light Curves of Type II Supernovae: Physical Properties of SNe and Their Environment
• Swift UV/Optical Telescope Imaging of Star Forming Regions in M81 and Holmberg IX
• Hobby-Eberly Telescope Observations of the Dark Halo in NGC 821
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• Addendum to: Update on neutrino mixing in the early Universe
• Probing Dark Energy Dynamics from Current and Future Cosmological Observations
• Weighing the Universe with Photometric Redshift Surveys and the Impact on Dark Energy Forecasts
• Cosmicflows-4: The Baryonic Tully-Fisher Relation Providing ~10,000 Distances
• Probing Inflation and Dark Energy with Current Cosmological Observations
• On the degeneracy between primordial tensor modes and cosmic strings in future CMB data from Planck
• A Lyα blob and zabs {\approx} zem damped Lyα absorber in the dark matter halo of the binary quasar Q 0151+048
• Period-Age-Metallicity and Period-Age-Color-Metallicity relations for Classical Cepheids: an application to the Gaia EDR3 sample
• Complementary Constraints on Brane Cosmology
• NGC 4654: polarized radio continuum emission as a diagnostic tool for a galaxy--cluster interaction
• Using Galactic Cepheids to verify Gaia parallaxes
• Properties of M31. II: A Cepheid disk sample derived from the first year of PS1 PAndromeda data
• The disappearance of the progenitor of SN 2012aw in late-time imaging
• The changing-type SN 2014C may come from an 11-$M_{\odot }$ star stripped by binary interaction and violent eruption
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
• Reconstructing cosmological initial conditions from galaxy peculiar velocities. II. The effect of observational errors
• Reconstructing the history of dark energy using maximum entropy
• Supernova 2014C: ongoing interaction with extended circumstellar material with silicate dust
• Did Boomerang hit MOND?
• Multiwavelength Study of High-Redshift Blazars
• Domain wall solution in $F(R)$ gravity and variation of the fine structure constant
• The JCMT Nearby Galaxies Legacy Survey VII: Hα imaging and massive star formation properties
• Collision-induced galaxy formation: semi-analytical model and multi-wavelength predictions
• Wavelet Band Powers of the Primordial Power Spectrum from CMB Data
• Astrophotonics: astronomy and modern optics
• Ultraviolet Spectroscopy of Type IIb Supernovae: Diversity and the Impact of Circumstellar Material
• Cluster correlations in redshift space
• Photometric and Spectroscopic Properties of Novae in the Large Magellanic Cloud
• The Stellar Content and Star Formation History of the late-type spiral galaxy NGC 300 from Hubble Space Telescope observations
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• The transition of equation of state of effective dark energy in the DGP model with bulk contents
• The ZTF Source Classification Project: II. Periodicity and variability processing metrics
• Spheroidal post-mergers in the local Universe
• HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure
• Determination of Cepheid parameters by light-curve template-fitting
• Is dark energy an effect of averaging?
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Supernova Remnants in M33: X-ray Properties as Observed by XMM-Newton
• Uncertainty on w from large-scale structure
• Inferring the presence of very massive stars in local star-forming regions
• Constraints on Models for TeV Gamma Rays from Gamma-Ray Bursts
• Basics of inflationary cosmology
• Do Observations Favour Galileon Over Quintessence?
• Broad-band Spectroscopy of the Ongoing Large Eruption of the Luminous Blue Variable R71
• The cosmological constant and general isocurvature initial conditions
• The Herschel Fornax Cluster Survey I: The Bright Galaxy Sample
• Integral field spectroscopy of HII regions in M33
• An alternative to dark matter and dark energy: Scale-dependent gravity in superfluid vacuum theory
• The radial metallicity gradient and the history of elemental enrichment in M81 through emission-line probes
• Radio Point Sources and the Thermal SZ Power Spectrum
• The Continuing Story of SN IIb 2013df: New Optical and IR Observations and Analysis
• Generalized CMB initial conditions with pre-equality magnetic fields
• The Structure of the Strongly Lensed Gamma-ray Source B2 0218+35
• Convection, granulation and period jitter in classical Cepheids
• An AGN Identification for 3EG J2006-2321
• Inertia from an asymmetric Casimir effect
• Cepheid limb darkening, angular diameter corrections, and projection factor from static spherical model stellar atmospheres
• Temperature Differences in the Cepheid Instability Strip Require Differences in the Period-Luminosity Relation in Slope and Zero Point
• The impact of a massive Sagittarius dSph on GD-1-like streams
• Supernovae and Cosmology
• Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach
• Using the cluster mass function from weak lensing to constrain neutrino masses
• The Mass Distribution of the Central Stars of Planetary Nebulae in the Large Magellanic Cloud
• The Extinction and Distance of Maffei 2 and a New View of the IC 342/Maffei Group
• Breaking the sigma_8-Omega_m degeneracy using the clustering of high-z X-ray AGN
• Variability of Luminous Stars in the Large Magellanic Cloud Using 10 Years of ASAS Data
• Early Spectral Evolution of the Rapidly Expanding Type Ia SN 2006X
• Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
• Current Challenges in Cepheid Distance Calibrations Using Gaia EDR3
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations
• Seven Years of SN 2014C: a Multi-Wavelength Synthesis of an Extraordinary Supernova
• The Extragalactic Distance Scale without Cepheids
• Effect of Helium Sedimentation on X-ray Measurements of Galaxy Clusters
• Inspecting the Cepheid distance ladder: The Hubble Space Telescope distance to the SNIa host galaxy NGC 5584
• A low upper mass limit for the central black hole in the late-type galaxy NGC 4414
• The Tip of the Red Giant Branch Distance to the Perfect Spiral Galaxy M74 Hosting Three Core-Collapse Supernovae
• Kinematical Structure of the Magellanic System
• Power-law Parameterized Quintessence Model
• Galaxy clusters in simulations of the local Universe: a matter of constraints
• Cosmological parameters estimation in the Quintessence Paradigm
• Spectroscopy of M81 Globular Clusters
• Observational evidence for a correlation between peak-luminosities and beaming in GRBs
• The Nature of SN 1961V
• White Dwarfs Near Black Holes: A New Paradigm for Type I Supernovae
• When a Period Is Not a Full Stop: Light Curve Structure Reveals Fundamental Parameters of Cepheid and RR Lyrae Stars
• Testing quantised inertia on galactic scales
• Discovery and quantitative spectral analysis of an Ofpe/WN9 (WN11) star in the Sculptor spiral galaxy NGC 300
• Scalar-tensor theories, trace anomalies and the QCD-frame
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• The Absolute Magnitude of RRc Variables From Statistical Parallax
• Future dark energy constraints from measurements of quasar parallax: Gaia, SIM and beyond
• The metallicity and distance of NGC 2403 from blue supergiants
• On the contribution of microlensing to X-ray variability of high-redshifted QSOs
• A New Detection of Extragalactic Anomalous Microwave Emission in a Compact, Optically-Faint Region of NGC\,4725
• Early Preheating and Galaxy Formation
• Galaxy clusters in local Universe simulations without density constraints: a long uphill struggle
• The Swift/UVOT catalogue of NGC4321 star forming sources: A case against density wave theory
• Precise space-time positioning for entanglement harvesting
• SNe observations in a meatball universe with a local void
• ALMA CO Observations of a Giant Molecular Cloud in M33: Evidence for High-Mass Star Formation Triggered by Cloud-Cloud Collisions
• Dynamical Models of Elliptical Galaxies in z=0.5 Clusters: I. Data-Model Comparison and Evolution of Galaxy Rotation
• Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry
• FIRST-based survey of Compact Steep Spectrum sources I. MERLIN images of arc-second scale objects
• Large Scale Magnetic Fields: Galaxy Two-Point correlation function
• HST observations of nuclear stellar disks
• Observational Constraints on Dynamical Dark Energy Models
• Prospects for the Determination of H_0 through Observation of Multiply Imaged Supernovae in Galaxy Cluster Fields
• Constraints on the Formation of the Globular Cluster IC 4499 from Multi-Wavelength Photometry
• Dark matter, and its darkness
• Effects of voids on the reconstruction of the equation of state of Dark Energy
• Microwave Continuum Emission and Dense Gas Tracers in NGC 3627: Combining Jansky VLA and ALMA Observations
• Principal Component Analysis of the Cosmic Microwave Background Anisotropies: Revealing The Tensor Degeneracy
• BVRIJK light curves and radial velocity curves for selected Magellanic Cloud Cepheids
• Dark Energy Accretion onto black holes in a cosmic scenario
• Constraints on the solid dark universe model
• Variable stars in the bar of the Large Magellanic Cloud: the photometric catalogue
• HST Survey of Clusters in Nearby Galaxies. I. Detection and Photometry
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Features in the primordial power spectrum: constraints from the CMB and the limitation of the 2dF and SDSS redshift surveys to detect them
• Cosmological evidence for leptonic asymmetry after Planck
• Bias in Absolute Magnitude Determination from Parallaxes
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Calibration of the distance scale from galactic Cepheids: I Calibration based on the GFG sample
• Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations II. Predictions and Tests of the OGLE-III Fundamental-Mode Cepheids
• Ultra Long Period Cepheids: a primary standard candle out to the Hubble flow
• Observational Constraints on Interacting Dark Matter Model Without Dark Energy
• Testing flatness of the universe with probes of cosmic distances and growth
• Constraints on intergalactic dust from quasar colours
• The electron temperatures of SDSS high-metallicity giant extragalactic HII regions
• Stellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence
• Non-Gaussian Error Distributions of LMC Distance Moduli Measurements
• Model independent constraints on mass-varying neutrino scenarios
• On the influence of the environment on galactic chemical abundances
• Dark energy models toward observational tests and data
• A lack of constraints on the cold opaque HI mass: HI spectra in M31 and M33 prefer multi-component models over a single cold opaque component
• Steepened inner density profiles of group galaxies via interactions: An N-body analysis
• The oxygen abundance gradient in M81 and the robustness of abundance determinations in H II regions
• The origin of the X-ray, radio and HI structures in the NGC 5903 galaxy group
• Period-colour and amplitude-colour relations in classical Cepheid variables IV: The multi-phase relations
• Supernovae and radio transients in M 82
• Galaxy Evolution and Cosmology with the Square Kilometre Array
• Constraining the dark energy dynamics with the cosmic microwave background bispectrum
• The Evolution of Late-Time Optical Emission From SN 1979C
• New optical spectra and general discussion on the nature of ULX's
• Galaxy Bias in Quintessence Cosmological Models
• Early Observations of the MHONGOOSE Galaxies: Getting Ready for MeerKAT
• The Cosmic Baryon Fraction and the Extragalactic Ionizing Background
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• Constraining the parameters of globular cluster NGC 1904 from its variable star population
• An updated Type II supernova Hubble diagram
• The distance to the LMC cluster NGC 1866 and the surrounding field
• Neutrino mass bounds from cosmology
• Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31
• Nonlinear Period-Luminosity Relation for the Large Magellanic Cloud Cepheids: Myths and Truths
• A Census of Variability in Globular Cluster M68 (NGC 4590)
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• High-resolution temporal constraints on the dynamics of dark energy
• General Relativity in the Undergraduate Physics Curriculum
• Tangled magnetic fields and CMBR signal from reionization epoch
• Stellar structures in the outer regions of M33
• Period-colour and amplitude-colour relations in classical Cepheid variables II: the Galactic Cepheid model
• Measuring the Cosmic Equation of State with Galaxy Clusters in the DEEP2 Redshift Survey
• String Cosmology - Large-Field Inflation in String Theory
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• Cosmic slowing down of acceleration using $f_{gas}$
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• Cosmography and large scale structure by f(R) gravity: new results
• Dynamics and constraints of the Unified Dark Matter flat cosmologies
• Assessing potential cluster Cepheids from a new distance and reddening parameterization and 2MASS photometry
• Estimating cosmological parameters from future gravitational lens surveys
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Vacuum Energy as the Origin of the Gravitational Constant
• Shell revealed in SN 1979C
• Probing for the Cosmological Parameters with PLANCK Measurement
• Testing MOND with Local Group spiral galaxies
• Constraining the Variation of G by Cosmic Microwave Background Anisotropies
• Cosmic acceleration and extra dimensions: constraints on modifications of the Friedmann equation
• The Detailed Forms of the LMC Cepheid PL and PLC Relations
• Hubble Space Telescope Photometry of Globular Clusters in M81
• Complementary constraints from FR IIb radio galaxies and X-ray gas mass fractions in clusters on non-standard cosmological models
• X-ray observations of the Large Magellanic Cloud pulsar PSR B0540-69 and its PWN
• How big were the first cosmological objects?
• The Araucaria Project. The Distance to the Sculptor Group Galaxy NGC 7793 from Near-Infrared Photometry of Cepheid Variables
• Disk Stability and Neutral Hydrogen as a Tracer of Dark Matter
• ALMA Observations of Giant Molecular Clouds in M33 I: Resolving Star Formation Activities in the Giant Molecular Filaments Possibly Formed by a Spiral Shock
• Observational constraints on the dark energy density evolution
• A new method for the estimate of H_0 from quadruply imaged gravitational lens systems
• Gravitational Lenses as High-Resolution Telescopes
• ALMA Observations toward the starburst dwarf galaxy NGC 5253: I. Molecular cloud properties and scaling relations
• Searching for Intermediate Mass Black Holes in galaxies with Low Luminosity AGN: A multiple-method approach
• The chemistry of planetary nebulae in the outer regions of M31
• The Cepheid Period-Luminosity Relation (The Leavitt Law) at Mid-Infrared Wavelengths: III. Cepheids in NGC 6822
• The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit
• The Cepheid Period-Luminosity relation and the maser distance to NGC 4258
• A simple analysis of halo density profiles using gravitational lensing time delays
• LBT Discovery of a Yellow Supergiant Eclipsing Binary in the Dwarf Galaxy Holmberg IX
• New Constraints on the Variable Equation of State Parameter from X-Ray Gas Mass Fractions and SNe Ia
• Cosmological Recombination of Lithium and its Effect on the Microwave Background Anisotropies
• The far side of the Galactic bar/bulge revealed through semi-regular variables
• A counter-rotating core in the dwarf elliptical galaxy VCC 510
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• The Resolved Stellar Populations of a Dwarf Spheroidal Galaxy in the Virgo Cluster
• Subaru Hyper Suprime-Cam Survey for An Optical Counterpart of GW170817
• New Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei
• The PSCz Dipole Revisited
• Scaling of the photon index vs mass accretion rate correlation and estimate of black hole mass in M101 ULX-1
• Constrained simulations of the local universe: II. The nature of the local Hubble flow
• A spectroscopic study of blue supergiant stars in Local Group spiral galaxies: Andromeda and Triangulum
• The Carnegie RR Lyrae Program: Mid-infrared Period-Luminosity relations of RR Lyrae stars in Reticulum
• A fluid os strings as a viable candidate to the dark side of the universe
• Mapping of the SZ effect in the cluster Cl 0016+16 with the Ryle Telescope
• Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects
• The Distance to Supernova 1998aq in NGC3982
• Revisiting Attenuation Curves: the Case of NGC 3351
• Colors and Mass-to-Light Ratios of Bulges and Disks of Nearby Spiral Galaxies
• Minimal HCN emission from Molecular Clouds in M33
• A Survey for Planetary Nebulae in M31 Globular Clusters
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• A New, Deep JVLA Radio Survey of M33
• The Unsettled Number: Hubble's Tension
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Cosmological Constraints from a Combined Analysis of the Cluster Mass Function and Microwave Background Anisotropies
• The Standard Cosmological Model
• Cosmological Acceleration Through Transition to Constant Scalar Curvature
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• A 3% Determination of $H_0$ at Intermediate Redshifts
• The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group
• Star formation history of KDG 61 and KDG 64 from spectroscopy and colour-magnitude diagrams
• The population of variable stars in M54 (NGC6715)
• Constraining photon-axion oscillations using quasar spectra
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. II. M66 and M96 in the Leo I Group
• Age of the Universe in the Cardassian Model
• Unearthing Foundations of a Cosmic Cathedral: Searching the Stars for M33's Halo
• Period-color and amplitude-color relations in classical Cepheid variables V: The Small Magellanic Cloud Cepheid models
• Spitzer Photometry of ~1 Million Stars in M31 and 15 Other Galaxies
• Generation of large-scale magnetic fields from inflation in teleparallelism
• Large extra dimensions, the galaxy power spectrum and the end of inflation
• The Metallicity Dependence of the Cepheid P-L Relation in M101
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Chandra ACIS Survey of M33 (ChASeM33): The enigmatic X-ray emission from IC131
• Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda$CDM model
• Cosmic Degeneracy with Dark Energy Equation of State
• CCD Photometry of the globular cluster NGC 5466. RR Lyrae light curve decomposition and the distance scale
• A theoretical analysis of the systematic errors in the Red Clump distance to the LMC
• The Connection Between Diffuse Light and Intracluster Planetary Nebulae in the Virgo Cluster
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• X-ray spectral evolution of the extragalactic Z-source, LMC X-2
• Accurate Extra-Galactic Distances and Dark Energy: Anchoring the Distance Scale with Rotational Parallaxes
• The long-period Galactic Cepheid RS Puppis - III. A geometric distance from HST polarimetric imaging of its light echoes
• Testing Cosmological General Relativity against high redshift observations
• The Detection of Bright Asymptotic Giant Branch Stars in the Nearby Elliptical Galaxy Maffei 1
• Spatial Power Spectra of Dust across the Local Group: No Constraint on Disc Scale Height
• The ACS Nearby Galaxy Survey Treasury III: Cepheids in the Outer Disk of M81
• XMMU J0541.8-6659, a new supernova remnant in the Large Magellanic Cloud
• Optical supernova remnants in nearby galaxies and their influence on star formation rates derived from H$\alpha$ emission
• Friedmann Equation for Brans Dicke Cosmology
• Concerning the Slope of the Cepheid Period-Luminosity Relation
• Inflation and Quintessence: Theoretical Approach of Cosmological Reconstruction
• Realistic Cyclic Magnetic Universe
• Time delay between images of the lensed quasar UM673
• A Radio and X-Ray Study of Historical Supernovae in M83
• Constraints on the Cardassian Expansion from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
• Inflessence: a phenomenological model for inflationary quintessence
• Dark and luminous matter in the NGC 3992 group of galaxies, I. The large barred spiral NGC 3992
• Extragalactic Water Masers, Geometric Estimation of H_o and Characterization of Dark Energy
• Uncertainties in The Interstellar Extinction Curve and the Cepheid Distance to M101
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses IV. Models of prospective time-delay lenses
• Dynamical state of superclusters of galaxies: do superclusters expand or have they started to collapse?
• Can Cosmic Parallax Distinguish Between Anisotropic Cosmologies?
• Combined constraints on Cardassian models from supernovae, CMB and large-scale structure observations
• Constraints on the cosmic equation of state: age conflict versus phantom energy. Age-redshift relations in an accelerated universe
• Calcium-rich Transient SN 2019ehk in A Star-Forming Environment: Yet Another Candidate for An Ultra-Stripped Envelope Supernova
• The near-IR Surface Brightness Method applied to six Cepheids in the young LMC cluster NGC1866
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Reddened, Redshifted, or Intrinsically Red? Understanding Near-Ultraviolet Colors of Type Ia Supernovae
• Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars
• The old globular cluster system of the dIrr galaxy NGC1427A in the Fornax cluster
• X-ray properties of NGC 300 I. Global properties of X-ray point sources and their optical counterparts
• Time variation of the fine structure constant in the early universe and the Bekenstein model
• Current constraints on Cosmological Parameters from Microwave Background Anisotropies
• Probing the nature of cosmic acceleration
• Mid-Infrared Spectroscopy of Two Lensed Star-forming Galaxies
• The Chandra ACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium in NGC604
• Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbv
• A Deep XMM-Newton Survey of M33: Point Source Catalog, Source Detection and Characterization of Overlapping Fields
• Warping of accretion disk and launching of jet by a spinning black hole in NGC 4258
• Nearby Galaxies in the 2micron All Sky Survey I. K-band Luminosity Functions
• Kinematic classification of non-interacting spiral galaxies
• Dynamics and chaos in the unified scalar field Cosmology
• A Spitzer/IRAC Characterization of Galactic AGB and RSG Stars
• SN 2011fe: A Laboratory for Testing Models of Type Ia Supernovae
• The Star Formation Reference Survey. I. Survey Description and Basic Data
• An Upper Limit on the Mass of a Central Black Hole in the Large Magellanic Cloud from the Stellar Rotation Field
• How does the grouping scheme affect the Wiener Filter reconstruction of the local Universe?
• Young stars in the periphery of the Large Magellanic Cloud
• The distance to the LMC cluster NGC 1866; clues from the cluster Cepheid population
• ASTRO-F - Super IRAS - The All Sky Infra-Red Survey
• Tests of star formation metrics in the low metallicity galaxy NGC 5253 using ALMA observations of H30$\alpha$ line emission
• Variation in GMC Association Properties Across Bars, Spiral Arms, Inter-Arms, and Circumnuclear Region of M100 (NGC 4321) Extracted from ALMA Observations
• Toward an Optimal Sampling of Peculiar Velocity Surveys For Wiener Filter Reconstructions
• Period-Luminosity Relations for Cepheid Variables: From Mid-Infrared to Multi-Phase
• Time variation of the electron mass in the early universe and the Barrow-Magueijo model
• Classification of X-ray Sources in the XMM-Newton Serendipitous Source Catalog: Objects of Special Interest
• On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation. II. The Effect of Metallicity
• Dark Energy and the Hubble Age
• Transverse Wave Propagation in Relativistic Two-fluid Plasmas around Schwarzschild-de Sitter Black Hole
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• Time Delays for the Giant Quadruple Lensed Quasar SDSS J1004+4112: Prospects for Determining the Density Profile of the Lensing Cluster
• Dark Energy: The Observational Challenge
• On the Stellar Populations in Faint Red Galaxies in the Hubble Ultra Deep Field
• The influence of Red Spiral Galaxies on the Shape of the Local K-Band Luminosity Function
• New constraint on the cosmological background of relativistic particles
• Dynamical Masses for the Large Magellanic Cloud Massive Binary System [L72] LH 54-425
• The Influence of Evolving Dark Energy on Cosmology
• Using 1991T/1999aa-like Type Ia Supernovae as Standardizable Candles
• Can particle creation phenomena replace dark energy?
• Dark energy, curvature, and cosmic coincidence
• The Hubble Constant from Type Ia Supernova Calibrated with the Linear and Non-Linear Cepheid Period-Luminosity Relation
• The stellar mass to light ratio in the isolated spiral NGC 4414
• A Study on the Universality and Linearity of the Leavitt Law in the LMC and SMC Galaxies
• The environments of hyperluminous infrared galaxies at 0.44<z<1.55
• Effects of Alpha-Element Enhancement and the Thermally Pulsing-Asymptotic Giant Branch on Surface Brightness Fluctuation Magnitudes and Broadband Colors
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Search for Neutron Star Binaries in the Local Group Galaxies Using LISA
• SN 2016esw: a luminous Type II supernova observed within the first day after the explosion
• Luminous and Variable Stars in NGC 2403 and M81
• An upper limit on the sulphur abundance in HE 1327-2326
• Constraints on the Compact Object Mass in the Eclipsing HMXB XMMU J013236.7+303228 in M33
• The S4G perspective on circumstellar dust extinction of AGB stars in M100
• Discovery of the Host Cluster for the Fundamental Cepheid Calibrator Zeta Gem
• Constraining Thawing Quintessence
• Gravitational orbits in the expanding universe revisited
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Aperture Synthesis Observations of CO, HCN, and 89GHz Continuum Emission toward NGC 604 in M 33: Sequential Star Formation Induced by Supergiant Hii region
• Star Cluster Candidates in M81
• A First Look at Cepheids in a SN Ia Host with JWST
• From model dynamics to oscillating dark energy parameterisation
• Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
• Relationship between the Line Width of the Atomic and Molecular ISM in M33
• Tracing the Assembly History of NGC 1395 through its Globular Cluster System
• Properties of M31. V: 298 Eclipsing Binaries from PAndromeda
• Investigation of the Progenitors of the Type Ia Supernovae Associated With the LMC Supernova Remnants 0505-67.9 and 0509-68.7
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Inverse Power Law Quintessence with Non-Tracking Initial Conditions
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• On the Reality of the Accelerating Universe
• The New Cosmology
• UBVI Surface Photometry of the Spiral Galaxy NGC 300 in the Sculptor Group
• Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae
• Intrinsic Degeneracy of Gravitational Lens Time Delays: the case for a simple quadruple system in $\Lambda$CDM cosmology
• The distance modulus determined from Carmeli's cosmology fits the accelerating universe data of the high-redshift type Ia supernovae without dark matter
• An investigation of gravitational lens determinations of H_o in quintessence cosmologies
• Cosmological constraints in the presence of ionizing and resonance radiation at recombination
• Results of optical monitoring of 5 SDSS double QSOs with the Nordic Optical Telescope
• Lyman alpha absorbers in motion: consequences of gravitational lensing for the cosmological redshift drift experiment
• An infrared study of local galaxy mergers
• Cosmological neutrino mass limit and the dynamics of dark energy
• Cosmological constrains from X-ray AGN clustering and SNIa data
• Improved cosmological constraints on the curvature and equation of state of dark energy
• NGC 5253 and ESO 269-G058: Dwarf Galaxies with a Past
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Infrared photometry of Cepheids in the LMC clusters NGC 1866 and NGC 2031
• Determining $H_0$ with the latest HII galaxy measurements
• The Inflationary Gravity Waves in light of recent Cosmic Microwave Background Anisotropies data
• Constraining scalar-tensor quintessence by cosmic clocks
• The primordial baryonic clouds and their contribution to the CMB anisotropy and polarization formation
• Empirical evidences in favor of a varying-speed-of-light
• Populations of super-soft X-ray sources in galaxies of different morphological types
• FLRW accelerating universe with interactive dark energy
• On the Form of the Spitzer Leavitt Law and its Dependence on Metallicity
• Observational Tests of FRW World Models
• Hα to FUV ratios in resolved star forming region populations of nearby spiral galaxies
• SN 2015bp: adding to the growing population of transitional type Ia supernovae
• Galactic open cluster Cepheids -- a census based on Gaia EDR3
• Are the HI deficient galaxies on the outskirts of Virgo recent arrivals?
• Superhorizon perturbations: A possible explanation of the Hubble--Lemaître Tension and the Large Scale Anisotropy of the Universe
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Period Change Rates in Large Magellanic Cloud Cepheids Revisited
• Flat Tree-level Inflationary Potentials in Light of CMB and LSS Data
• Pan-chromatic observations of the remarkable nova LMC 2012
• Cosmic microwave background polarization analysis
• Introduction to neutrino cosmology
• Cosmological Consequences of Exponential Gravity in Palatini Formalism
• Quaternion algebra on 4D superfluid quantum space-time. Gravitomagnetism
• Is Thick Brane Model Consistent with the Recent Observations?
• Discovery of $\sim$2200 new supernova remnants in 19 nearby star-forming galaxies with MUSE spectroscopy
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• Imprint of spatial curvature on inflation power spectrum
• Gaia TGAS search for Large Magellanic Cloud runaway supergiant stars:Candidate hypervelocity star discovery, and the nature of R71
• Observational tests of a two parameter power-law class modified gravity in Palatini formalism
• Interstellar communication network. I. Overview and assumptions
• Compact stellar systems in the Fornax cluster: a UV perspective
• Average luminosity distance in inhomogeneous universes
• A Cepheid-Based Distance to the Seyfert Galaxy NGC 6814
• Precision Primordial ${}^4$He Measurement with CMB Experiments
• Kinematics of the Broad Line Region in M81
• Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
• Red Supergiants in the Disk of M81: Tracing the Spatial Distribution of Star Formation 25 Million Years in the Past
• Optical Spectra of SNR Candidates in NGC 300
• Observational Cosmology
• Reeling in the Whirlpool: the distance to M 51 clarified by Cepheids and the Type IIP SN 2005cs
• Data analysis methods for the cosmic microwave background
• Grey Milky Way Extinction from SDSS Stellar Photometry
• Accidental Inflation from Kähler Uplifting
• Observations of the High Redshift Universe
• Hubble tensions: a historical statistical analysis
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• Implications of Two Type Ia Supernova Populations for Cosmological Measurements
• Nuclear Radio Jet from a Low-Luminosity Active Galactic Nucleus in NGC 4258
• GRB Hubble diagram and constraints on a Λ(t)CDM model
• ALMA Observations of Giant Molecular Clouds in M33. II. Triggered High-mass Star Formation by Multiple Gas Colliding Events at the NGC 604 Complex
• Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D
• Instability analysis for spiral arms of local galaxies: M51, NGC3627 and NGC628
• Cosmic rays at ultra high energies (Neutrinos!)
• Frequency analysis of OGLE-IV photometry for classical Cepheids in Galactic fields: non-radial modes and modulations
• Constraining the CDM spectrum normalization in flat dark energy cosmologies
• SDSS galaxies with double-peaked emission lines: double starbursts or AGNs?
• Cosmological constraints from low-redshift data
• VLT Optical BVR observations of two bright Supernova Ia hosts in the Virgo cluster
• Systematic Errors in the Hubble Constant Measurement from the Sunyaev-Zel'dovich effect
• Scalar potential model of redshift and discrete redshift
• Infrared spectroscopy of nearby radio active elliptical galaxies
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• The Rate and Spatial Distribution of Novae in M101 (NGC 5457)
• Arguments for a Hubble Constant near $H_0$ = 55
• The Cepheids of NGC1866: A Precise Benchmark for the Extragalactic Distance Scale and Stellar Evolution from Modern UBVI Photometry
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Does cosmological expansion affect local physics?
• The impact of the Universe's expansion rate on constraints on modified growth of structure
• A Search for Infrared Emission from Core-Collapse Supernovae at the Transitional Phase
• The Kinematic State of the Local Volume
• Light and Motion in the Local Volume
• Composite Bulges -- IV. Detecting Signatures of Gas Inflows in the IFU data: The MUSE View of Ionized Gas Kinematics in NGC 1097
• Dipole anisotropies of IRAS galaxies and the contribution of a large-scale local void
• Scaling Dark Energy
• Current lookback time-redshift bounds on dark energy
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• GASP VIII: Capturing the birth of a Tidal Dwarf Galaxy in a merging system at z~0.05
• Symmetric-Bounce Quantum State of the Universe
• Classical Cepheids: Yet another version of the Baade-Becker-Wesselink method
• Nontrivial Geometries: Bounds on the Curvature of the Universe
• Investigating The Hubble Tension Through Hubble Parameter Data
• [CII] map of the molecular ring and arms of the spiral galaxy NGC 7331
• FRW dark energy cosmological model with hybrid expansion law
• The Hubble constant and dark energy from cosmological distance measures
• Broad band polarimetric follow-up of Type IIP SN 2012aw
• The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83
• Cosmic Flows surveys and CLUES simulations
• Calibration of AGN Reverberation Distance Measurements
• The IC133 Water Vapor Maser in the Galaxy M33: A Geometric Distance
• Observational tests for oscillating expansion rate of the Universe
• Probing galaxy density profiles with future supernova surveys
• Probing for variation of neutrino mass with current observations
• Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal
• Constraints on Models with a Break in the Primordial Power Spectrum
• The Rate and Spatial Distribution of Novae in M31 as Determined by a Twenty-Year Survey
• Cosmology with the Planck cluster sample
• Extragalactic Stellar Astronomy with the Brightest Stars in the Universe
• Prospects in Constraining the Dark Energy Potential
• PG 1115+080: variations of the A2/A1 flux ratio and new values of the time delays
• Predicted properties of Galactic and Magellanic Classical Cepheids in the SDSS filters
• Constraints on Generalized Dark Energy from Recent Observations
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Updated 24 $\mu \mathrm{m}$ Period-Luminosity Relation Derived from Galactic Cepheids
• Calibrating Long Period Variables as Standard Candles with Machine Learning
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• Hydrogen Radio Recombination Line Emission from M51 and NGC628
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Mathematical Underpinnings of the Multi-Wavelength Structure of the TRGB
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• AstroSat view of LMC X-2: Evolution of broadband X-ray spectral properties along a complete Z-track
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• Simultaneous determination of ${\Omega }_{M0}$ and $H_0$ from joint Sunyaev-Zeldovich effect and X-ray observations with median statistics
• The effect of interacting dark energy on local measurements of the Hubble constant
• Photometric Analysis of the Optical Counterpart of the Black Hole HMXB M33 X-7
• Gamma ray burst distances and the timescape cosmology
• Period-Color and Amplitude-Color Relations in Classical Cepheid Variables - VI. New Challenges for Pulsation Models
• Young and Intermediate-age Distance Indicators
• Intergalactic globular clusters and the faint end of the galaxy number counts in A1656 (Coma)
• Coordinated JWST Imaging of Three Distance Indicators in a SN Host Galaxy and an Estimate of the TRGB Color Dependence
• Standardized Luminosity of the Tip of the Red Giant Branch utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
• Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
• Hide and seek between Andromeda's halo, disk, and giant stream
• A Detection of an X-ray Wind and an Ionized Disk in the Chandra HETGS Observation of the Seyfert 2 Galaxy IRAS 18325-5926
• Chandra ACIS Survey of M33 (ChASeM33): X-ray Imaging Spectroscopy of M33SNR21, the Brightest X-ray Supernova Remnant in M33
• CMB-Normalized Predictions for Sunyaev-Zel'dovich effect fluctuations
• Building the cosmic distance scale: from Hipparcos to Gaia
• Nainital Microlensing Survey -- detection of short period Cepheids in the disk of M31
• Observational Constraints on Axions as Quintessence in String Theory
• The Extragalactic Distance Scale without Cepheids IV
• Halting eternal acceleration with an effective negative cosmological constant
• The current status of observational cosmology
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• Breaking the degeneracy between gas inflow and outflows with stellar metallicity: Insights on M101
• Einstein-de Sitter model re-examined for the newly discovered SNe Ia
• Examining the Infrared Variable Star Population Discovered in the Small Magellanic Cloud Using the SAGE-SMC Survey
• Ho Measurement from VLT Deep I-band Surface Brightness Fluctuations in NGC 564 and NGC 7619
• Dark and luminous matter in the NGC 3992 group of galaxies, II. The dwarf companions UGC 6923, UGC 6940, UGC 6969, and the Tully-Fisher relation
• Predicting the clustering properties of galaxy clusters detectable for the Planck satellite
• Designing Decisive Detections
• Weighing neutrinos using high redshift galaxy luminosity functions
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Geometry of the Large Magellanic Cloud Using Multi- wavelength Photometry of Classical Cepheids
• Halo Model Analysis of Cluster Statistics
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Radial Gas Inflow and Shock Excitation in NGC 1042
• Fractal Bubble Cosmology: A concordant cosmological model?
• Gluon condensate, modified gravity, and the accelerating Universe
• The influence of chemical composition on the properties of Cepheid stars I - Period-Luminosity relation vs iron abundance
• Astrophysical Observations: Lensing and Eclipsing Einstein's Theories
• Constraints from the Old Quasar APM 08279+5255 on Two Classes of $\Lambda ($t$)$-Cosmologies
• The Ultraviolet Brightest Type Ia Supernova 2011de
• The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey IX: ${}^{12}$CO $J=3\to 2$ Observations of NGC 2976 and NGC 3351
• A Possible High Nova Rate for Two Local Group Dwarf Galaxies: M32 and NGC 205
• Strongly Lensed Jets, Time Delays, and the Value of H0
• Observational constraints on electromagnetic Born-Infeld cosmology
• Thirty Years of Radio Observations of Type Ia SN 1972E and SN 1895B: Constraints on Circumstellar Shells
• The Nova Rate in NGC 2403
• Constraints on Cardassian universe from Gamma ray bursts
• An original constraint on the Hubble constant: h>0.74
• A Survey of Eclipsing Binary Stars in the Eastern Spiral Arm of M31
• Large Cold Dust Reservoir Revealed in Transitional SN Ib 2014C by James Webb Space Telescope Mid-Infrared Spectroscopy
• Blast From the Past: Constraining Progenitor Models of SN 1972E
• The Radio Variability of the Gravitational Lens PMN J1838-3427
• Particle Physics Approach to Dark Matter
• The Axis-Ratio Distribution of Galaxy Clusters in the SDSS-C4 Catalog as a New Cosmological Probe
• Constraining Perturbative Early Dark Energy with Current Observations
• Bulk viscous cosmological model with interacting dark fluids
• Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
• Systematic errors in the determination of Hubble constant due to the asphericity and non-isothermality of clusters of galaxies
• Strong lensing, cosmology and lensing halos
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• Size estimates for intervening C IV absorbers from high resolution spectroscopy of APM 0827+5255
• Further Evidence that the Redshifts of AGN Galaxies May Contain Intrinsic Components
• Swift-XRT 6-year monitoring of the ultraluminous X-ray source M33-X8
• PHANGS-HST: Globular Cluster Systems in 17 Nearby Spiral Galaxies
• Distortion of Infall Regions in Redshift Space-I
• A Distance Measurement to M33 Using Optical Photometry of Mira Variables
• A nearly constant CN/HCN line ratio in nearby galaxies: CN as a new tracer of dense gas
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Predicted masses of Galactic Cepheids in the Gaia Data Release 2
• Relativistic cosmology number densities in void-Lemaitre-Tolman-Bondi models
• The Hubble constant from two sibling Type Ia supernovae in the nearby galaxy NGC 4414: SN 1974G and SN 2021J
• The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
• An extension of the cosmological standard model with a bounded Hubble expansion rate
• Mid and Far-Infrared Color-Color Relations within Local Galaxies
• Dissecting Galaxies with Quantitative Spectroscopy of the Brightest Stars in the Universe
• Rescued from oblivion: detailed analysis of archival {\it Spitzer} data of SN~1993J
• ALMA Observations of Giant Molecular Clouds in M33 III: Spatially Resolved Features of the Star-Formation Inactive Million-solar-mass Cloud
• An Arecibo Search for Pulsars and Transient Sources in M33
• The tension of cosmological magnetic fields as a contribution to dark energy
• Modelling the two point correlation function of galaxy clusters in the Sloan Digital Sky Survey
• The universe is accelerating. Do we need a new mass scale?
• Sub-kiloparsec empirical relations and excitation conditions of HCN and HCO+ J=3-2 in nearby star-forming galaxies
• Peculiar velocity measurement in a clumpy universe
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• The 2dF Galaxy Redshift Survey as a Cosmological Laboratory
• Near-infrared and Optical Nebular-phase Spectra of Type Ia Supernovae SN 2013aa and SN 2017cbv in NGC 5643
• An HST/NICMOS view of the prototypical giant HII region NGC604 in M33
• CI and CO in Nearby Spiral Galaxies -- I. Line Ratio and Abundance Variations at ~ 200 pc Scales
• The Hubble Catalog of Variables (HCV)
• Age problem in holographic dark energy
• Holographic field theory models of dark energy in interaction with dark matter
• Large-scale magnetic fields from inflation due to a $CPT$-even Chern-Simons-like term with Kalb-Ramond and scalar fields
• The Tajmar effect from quantised inertia
• Latest Observational Constraints on Cardassian Models
• VI-Band Follow-Up Observations of Ultra-Long-Period Cepheid Candidates in M31
• Time delay of photons of different energies in multi-dimensional cosmological models
• Decades' long-term variations in NS-LMXBs observed with MAXI/GSC, RXTE/ASM and Ginga/ASM
• HI Spectroscopy of Reverberation-Mapped Active Galactic Nuclei
• Bimodality of Galaxy Disk Central Surface Brightness Distribution in the Spitzer 3.6 micron band
• Blue luminous stars in nearby galaxies - UIT005: a possible link to the luminous blue variable stage
• Search for Classical Cepheids in Galactic Open Clusters and Calibration of the Period Wesenheit Metallicity Relation in the Gaia Bands
• Searching for star-forming dwarf galaxies in the Antlia cluster
• Stellar Contents and Globular Cluster Candidates in the Sculptor Group Galaxy NGC 300
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities
• Identifying Candidate Optical Variables Using Gaia Data Release 2
• Four hints and test candidates of the local cosmic expansion
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• Elliptical Solutions to the Standard Cosmology Model with Realistic Values of Matter Density
• Precise Photometric Measurements from a 1903 Photographic Plate Using a Commercial Scanner
• A study of the remarkable galaxy system AM 546-324 (the core of Abell S0546)
• A conjecture on the origin of dark energy
• Detectability of Cosmic Topology in Generalized Chaplygin Gas Models
• A Search for Mass Loss on the Cepheid Instability Strip using HI 21-cm Line Observations
• Hubble law: measure and interpretation
• Can Dust Injected by SNe Explain the NIR-MIR Excess in Young Massive Stellar Clusters?
• Flat Cosmology with Coupled Matter and Dark Energies
• What have we learned from observational cosmology ?
• Systematic Errors in Sunyaev-Zeldovich Surveys of Galaxy Cluster Velocities
• A hierarchical Bayesian model to infer PL(Z) relations using Gaia parallaxes
• Primordial Feature at the Scale of Superclusters of Galaxies
• Tailoring galaxies: size-luminosity-surface brightness relations of bulges and disks along the morphological sequence
• Searching for star-forming galaxies in the Fornax and Hydra clusters
• The role of environment on the star formation history of disc galaxies
• $\Lambda$-CDM type Heckmann - Suchuking model and union 2.1 compilation
• The Distance of the First Overtone RR Lyrae Variables in the MACHO LMC Database: A New Method to Correct for the Effects of Crowding
• The massive star population of the Virgo Cluster galaxy NGC 4535
• Determining $H_0$ using a model-independent method
• A starburst in the core of a galaxy cluster: The dwarf irregular NGC 1427A in Fornax
• No-Bang Quantum State of the Cosmos
• Where's the Dust?: The Deepening Anomaly of Microwave Emission in NGC 4725 B
• FM 047-02: a collisional pair of galaxies with a ring
• Unveiling the Universe with Emerging Cosmological Probes
• Tests of photometry: the case of the NGC 3370 ACS field
• Clustering of Local Group distances: publication bias or correlated measurements? VI. Extending to Virgo cluster distances
• Sub-milliarcsecond imaging of a bright flare and ejection event in the extragalactic jet 3C 111
• Intrinsic Redshifts and the Tully-Fisher Distance Scale
• Measuring the matter energy density and Hubble parameter from Large Scale Structure
• Using bright ellipticals as dark energy cosmic clocks
• Improvement of the CORS method for Cepheids radii determination based on Stromgren photometry
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• The First Candidate Colliding-Wind Binary in M33
• A note on observational signatures in superluminal unified dark matter models
• `Hyper Parameters' Approach to Joint Estimation: Applications to Cepheid-Calibrated Distances and X-Ray Clusters
• Measuring the cosmological density perturbation
• The Ups and Downs of the Hubble Constant
• Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
• Growing a nuclear star cluster from star formation and cluster mergers: The JWST NIRSpec view of NGC 4654
• Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
• Survival of the Fittest: Numerical Modeling of Supernova 2014C
• Further Evidence for Intrinsic Redshifts in Normal Spiral Galaxies
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• A Multi-epoch X-ray Study of the Spiral Galaxy NGC 7331
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• A deep narrowband survey for planetary nebulae at the outskirts of M33
• New constraints on H_0 and Omega_M from SZE/X-RAY data and Baryon Acoustic Oscillations
• Possible relation between galactic flat rotational curves and the Pioneers' anomalous acceleration
• Measurement of Hubble constant: Non-Gaussian Errors in HST key project data
• Cosmological implications of the KATRIN experiment
• Distances to Galaxies from the Brightest Stars in the Universe
• Goodness-of-fit analysis of the Cosmicflows-2 database of velocities
• Neutrino Properties from High Energy Astrophysical Neutrinos
• "Expansion" around the vacuum: how far can we go from Lambda?
• Kinematical Conformal Cosmology: fundamental parameters from astrophysical observations
• Unveiling the new generation of stars in NGC 604 with Gemini-NIRI
• The cosmological constant and the paradigm of adiabaticity
• The Cosmology of Asymmetric Brane Modified Gravity
• Time-Series Surveys and Pulsating Stars: The Near-Infrared Perspective
• Probing for cosmological parameters with LAMOST measurement
• Improved Cosmological Parameter Constraints from CMB and H(z) Data
• Kinematical Analysis of Substructure in the Southern Periphery of the Large Magellanic Cloud
• The Ks-band Tully-Fisher Relation - A Determination of the Hubble Parameter from 218 ScI Galaxies and 16 Galaxy Clusters
• Large-scale structure and the Cardassian fluid
• On the Paradoxical Impact of Blending by Red Clump Giants
• Searching for Balmer-dominated Type Ia Supernova Remnants in M33
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Variability search in M 31 using Principal Component Analysis and the Hubble Source Catalog
• The baryon mass function for galaxy clusters
• Constraining $f(R)$ Theories with Temporal Variation of Fine Structure Constant
• Neutral atomic and molecular gas dynamics in the nearby spiral galaxies NGC 1512, NGC 4535, and NGC 7496
• Hydrogen 2p--2s transition: signals from the epochs of recombination and reionization
• Inflowing Gas in the Central Parsec of M81
• New Globular Cluster Candidates in the M81 group
• CAHA/PPAK Integral-field Spectroscopic Observations of M81 -- I. Circumnuclear ionized gas
• From Cosmos to Intelligent Life: The Four Ages of Astrobiology
• Advancing the Physics of Cosmic Distances: Conference Summary
• Evidence for Intrinsic Redshifts in Normal Spiral Galaxies
• The Measure of Cosmological Parameters
• A Long-term photometric variability and spectroscopic study of luminous blue variable AF And in M31
• The HST Key Project galaxies NGC 1326A, NGC 1425 and NGC 4548: New variable stars and massive star population
• Towards Machine-assisted Meta-Studies: The Hubble Constant
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Can LISA Resolve Distance to the Large Magellanic Cloud?
• Equilibrium boundary conditions, dynamic vacuum energy, and the Big Bang
• Density perturbations from both the inflaton and the curvaton
• Cosmic acceleration from second order gauge gravity
• Spatially Resolved Chandra Spectroscopy of Supernova Remnant DEM L71 in the Large Magellanic Cloud
• A very extended reionization epoch ?
• WISDOM Project -- XXII. A 5% precision CO-dynamical supermassive black hole mass measurement in the galaxy NGC 383
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Cosmology and the Hubble Constant: On the Megamaser Cosmology Project (MCP)
• Can the Tajmar effect be explained using a modification of inertia?
• The Carnegie-Chicago Hubble Program: Calibration of the Near-Infrared RR Lyrae Period-Luminosity Relation With HST
• More satellites around the nearby spiral galaxy NGC 7331
• Constraints on the unified dark energy-dark matter model from latest observational data
• Simulating non-axisymmetric flows in disc galaxies
• The Complex Upper HR Diagram
• Precision Cosmology from X-ray AGN clustering
• Transient Detection and Classification
• Self-Similar Shocks and Winds in Galaxy Clusters
• Cosmological Parameters and Cosmic Topology
• 20+ years of Inflation
• JWST/MIRI detects the dusty SN1993J about 30 years after explosion
• Crossing the phantom divide with a classical Dirac field
• Exploring Hubble Constant Data in an Introductory Course
• Is there any evidence for extra-dimensions or quantum gravity effects from the delayed MeV-GeV photons in GRB 940217?
• Point Source Confusion in SZ Cluster Surveys
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
• Probing the star formation epoch with Wilkinson Microwave Anisotropy Probe (WMAP) data and high-redshift QSOs
• Star formation drivers across the M33 disk
• Extragalactic Planetary Nebulae: tracers of the chemical evolution of nearby galaxies
• Observing Baryonic Dark Matter with ALMA
• Discovery of an eclipsing X-ray binary with a 32.69 hour period in M101: an analog of Her X-1 or LMC X-4?
• Distance Measurements and Stellar Population Properties via Surface Brightness Fluctuations
• An Information Theory Approach on Deciding Spectroscopic Follow Ups
• Distance-Redshift Relations in an Anisotropic Cosmological Model
• Scaling Hydrodynamical Evolution of a Gravitating Dark-fluid Universe
• ALMA FACTS. II. Large Scale Variations in the 12CO(J=2-1) to 12CO(J=1-0) Line Ratio in Nearby Galaxies
• XMM-Newton discovery of transient 285.4 s X-ray pulsar XMMU J013359.5+303634 in M33
• Clustering of Local Group distances: publication bias or correlated measurements? VII. A distance framework out to 100 Mpc
• Allan Sandage and the Distance Scale
• The establishment of the Standard Cosmological Model through observations
• A Century of Cosmology
• Time delays in PG1115+080: new estimates
• Testing X-ray Measurements of Galaxy Cluster Gas Mass Fraction Using the Cosmic Distance-Duality Relation
• Cosmological parameter estimation with large scale structure and supernovae data
• The outskirts of M33: Tidally induced distortions versus signatures of gas accretion
• Large-scale magnetic fields from inflation in teleparallel gravity
• Accelerated closed universes in scalar-tensor theories
• Pioneer 10 and 11 Spacecraft Anomalous Acceleration in the light of the Nonsymmetric Kaluza-Klein (Jordan-Thiry) Theory
• Generalized particle dynamics in anti de Sitter spaces: A source for dark energy
• Neutrino mass constraint from CMB and its degeneracy with other cosmological parameters
• How Many Universes Do There Need To Be?
• New variable stars in the Galactic Bulge: I. The bright regime
• Predicting extragalactic distance errors using Bayesian inference in multi-measurement catalogs
• Probing Cosmology beyond $\Lambda$CDM using the SKA
• Soft band X/K luminosity ratios in late-type galaxies and constraints on the population of supersoft X-ray sources
• Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect
• The Lenses Structure & Dynamics Survey: The internal structure and evolution of E/S0 galaxies and the determination of H_0 from time-delay systems
• Distance determination from the Cepheids and RR Lyrae period-luminosity relations
• The Cosmic Microwave Background anisotropies: open problems
• The Legacy of Henrietta Leavitt: A Re-analysis of the First Cepheid Period-Luminosity Relation
• A First-look at Spatially-resolved Infrared Supernova Remnants in M33 with JWST
• Observational dynamics of low-mass stellar systems
• First Detection of Radio Emission Associated with a Classical Cepheid
• Detecting the progenitors of core collapse supernovae
• Interacting Constituents in Cosmology
• Behavior of $F(R)$ gravity around a crossing of the phantom divide
• The Effect of Superpositions on the Planetary Nebula Luminosity Function
• Statistically bias-minimized peculiar velocity catalogs from Gibbs point processes and Bayesian inference
• Considering light-matter interactions in the Friedmann equations
• Highly reddened type Ia supernova SN 2004ab: another case of anomalous extinction
• Emergence of smooth distance and apparent magnitude in a lumpy Universe
• A New Approach to Testing Dark Energy Models by Observations
• On the impact of Helium abundance on the Cepheid Period-Luminosity and Wesenheit relations and the Distance Ladder
• Reconstruction of 5D Cosmological Model From Recent Observations
• An overview of the current status of CMB observations
• Cosmological constraints in Lambda-CDM and Quintessence paradigms with Archeops
• Cosmic Microwave Background Polarization
• New variable sources revealed by DECam toward the LMC: the first 15 deg2
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Measuring the Hubble Constant with the Hubble Space Telescope
• Can MONDian vector theories explain the cosmic speed up ?
• The pride of lions around Messier 105
• Unified Dark Energy and Dark Matter from Dynamical Spacetime Cosmology
• Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Low-mass disc galaxies and the issue of stability: MOND vs dark matter
• Non-Gaussianity and direction dependent systematics in HST key project data
• Bounce and Collapse in the Slotheonic Universe
• A critical review of the evidence for M32 being a compact dwarf satellite of M31 rather than a more distant normal galaxy
• Citation measures and impact within astronomy
• Intrinsic color diversity of nearby type Ia supernovae
• Scalar field dark energy and Cosmic Microwave Background
• Testing the CMB Data for Systematic Effects
• Eclipsing Binaries: Tools for Calibrating the Extragalactic Distance Scale
• Bayesian analysis of the backreaction models
• Observing the CMB at High-l using the VSA and AMI
• The Baade-Becker-Wesselink technique and the fundamental astrophysical parameters of Cepheids
• Parameter space stability of multiple soft interactions
• Multicolor photometry of 145 of the HII regions in M33
• A graceful multiversal link of particle physics to cosmology
• Cloud populations versus galactic environment in NGC4689, NGC628, NGC1566, and NGC4321
• Cosmological Constraints on Radion Evolution in the Universal Extra Dimension Model
• Cosmology in a Higher-Curvature Gravity
• Median Statistics Estimate of the Distance to M87
• Pulsation and Mass Loss Across the HR Diagram: From OB stars to Cepheids to Red Supergiants
• Broadband Spectrum of the X-ray Binary M33 X-6 from NuSTAR and Swift-XRT Data: An Extragalactic Z-Source?
• Archeops: an instrument for present and future cosmology
• Pulsating variable stars in the Magellanic Clouds
• An Alcock-Paczynski Test on Reionization Bubbles for Cosmology
• Monitoring the X-ray Variability of Bright X-ray Sources in M33
• AT 2016dah and AT 2017fyp: the first classical novae discovered within a tidal stream
• The Local Velocity Anomaly
• Temperature based radial metallicity gradients in nearby galaxies
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• A neutrino model fit to the CMB power spectrum
• The DESI DR1 Peculiar Velocity Survey: global zero-point and $H_0$ constraints
• Thermodynamics of irreversible particle creation phenomena and its cosmological consequence
• Exploring the origins of high-velocity features in SNe Ia with the spectral synthesis code TARDIS
• Precision cosmological measurements: independent evidence for dark energy
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• Dependence of pulsation mode of Cepheids on metallicity
• The Magellanic Edges Survey -- II. Formation of the LMC's northern arm
• Multiwavelength light curve analysis of Cepheid variables
• Analysis of the angular dependence of time delay in gravitational lensing
• The Large Magellanic Cloud: A power spectral analysis of Spitzer images
• Interesting Evidence for a Low-Level Oscillation Superimposed on the Local Hubble Flow
• Type Ia supernovae SN 2013bz, PSN J0910+5003 and ASASSN-16ex: similar to 09dc-like?
• Using the Modified Lognormal Power Law Distribution to Model the Mass Function of NGC 1711
• CMB Constraint on Radion Evolution in the Brane World Scenario
• Target-based Optimization of Advanced Gravitational-Wave Detector Network Operations
• Techniques for Observing Binaries in Other Galaxies
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• More Evidence for an Oscillation Superimposed on the Hubble Flow
• A semi-cosmographic approach to study cosmological evolution in phase space
• Large-Scale Surveys of Pulsating Stars for Studying Stellar Populations in the Inner Galaxy
• The Local Void is Really Empty
• Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance
• An update on Archeops: flights and data products
• Simultaneous inference of periods and period-luminosity relations for Mira variable stars
• Free-Floating HI Clouds in the M 81 Group
• Is the Pre-WMAP CMB Data Self-consistent?
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Variable stars in the Gaia era: Mira, RR Lyrae, delta and Type-II Cepheids
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• The Astrophysical Distance Scale: V. A 2% Distance to the Local Group Spiral M33 via the JAGB Method, Tip of the Red Giant Branch, and Leavitt Law
• The orbital dynamics of the LMC and SMC about the Milky Way
• OGLE-IV Period-Luminosity relation of the LMC: an analysis using mean and median magnitudes
• On curvature coupling and quintessence fine-tuning
• Measuring Type Ia Supernova Distances and Redshifts From Their Multi-band Light Curves
• Bar-driven gas redistribution suppresses star formation in spiral galaxies: Evidence from dust lanes in NGC 3351
• Genetic algorithm demystified for cosmological parameter estimation
• Stellar populations -- the next ten years
• The Rees-Sciama effect and the primordial nucleosynthesis
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Semiresolved Stellar Populations as Distance Indicators
• Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters -- II. Kinematic structure of young and intermediate-age clusters
• Near-infrared observations of OGLE classical and type II Cepheid variables in the LMC
• Maps of the Cosmos: The Cosmic Microwave Background
• Differences between the globular cluster systems of the Virgo and Fornax Galaxy Clusters
• Zwicky Transient Facility and Globular Clusters: The RR Lyrae gri-Band Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations
• Catalogue of central stars of extragalactic planetary nebulae
• The Hubble Catalog of Variables (HCV)
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Bending Waves in Velocity Space: a First Look at the THINGS sample
• A likely inverse-Compton emission from the Type IIb SN 2013df
• Distances on Cosmological Scales with VLTI
• The Variable Sky Through the OGLE Eye
• Linearized Treatment of Scalar perturbations in the Asymptotic Cosmological Model