A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3

Abstract

We use the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope to determine the Hubble constant (H0) from optical and infrared observations of over 600 Cepheid variables in the host galaxies of 8 recent Type Ia supernovae (SNe Ia), providing the calibration for a mag-z relation of 253 SNe Ia. Increased precision over past measurements comes from: (1) more than doubling the number of infrared observations of Cepheids in nearby SN hosts; (2) increasing the sample of ideal SN Ia calibrators from six to eight; (3) increasing by 20% the number of Cepheids with infrared observations in the megamaser host NGC 4258; (4) reducing the difference in the mean metallicity of the Cepheid comparison samples from Δlog [O/H] = 0.08 to 0.05; and (5) calibrating all optical Cepheid colors with one camera, WFC3, to remove cross-instrument zero-point errors. Uncertainty in H0 from beyond the 1st rung of the distance ladder is reduced from 3.5% to 2.3%. The measurement of H0 via the geometric distance to NGC 4258 is 74.8 \pm 3.1 km s- 1 Mpc-1, a 4.1% measurement including systematics. Better precision independent of NGC 4258 comes from two alternative Cepheid absolute calibrations: (1) 13 Milky Way Cepheids with parallaxes and (2) 92 Cepheids in the Large Magellanic Cloud with multiple eclipsing binary distances, yielding 74.4 \pm 2.5 km s- 1 Mpc-1, a 3.4% uncertainty with systematics. Our best estimate uses all three calibrations but a larger uncertainty afforded from any two: H0 = 73.8 \pm 2.4 km s- 1 Mpc-1 including systematics, a 3.3% uncertainty. The improvement in H0, combined with WMAP7yr data, results in a constraint on the EOS parameter of dark energy of w = -1.08 \pm 0.10 and Neff = 4.2 \pm 0.7 for the number of relativistic species in the early universe. It also rules out the best-fitting gigaparsec-scale void models, posited as an alternative to dark energy. (abridged)

56 pages, 10 figures

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• Weyl-Cartan-Weitzenböck gravity through Lagrange multiplier
• Cosmological constraints on induced gravity dark energy models
• A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• Post-$Planck$ constraints on interacting vacuum energy
• Dark Energy Constraints after Planck
• Herschel-ATLAS: The Surprising Diversity of Dust-Selected Galaxies in the Local Submillimetre Universe
• Fitting the Union2.1 SN Sample with the R_h=ct Universe
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Independent Cosmological Constraints from high-z HII Galaxies
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• On the definition of superclusters
• Light sterile neutrinos after BICEP-2
• Coupled dark energy with perturbed Hubble expansion rate
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Parallax of Galactic Cepheids from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope: The Case of SS Canis Majoris
• Model-independent constraints on the cosmic opacity
• SHARP - III: First Use Of Adaptive Optics Imaging To Constrain Cosmology With Gravitational Lens Time Delays
• Constraints on neutrino and dark radiation interactions using cosmological observations
• Strong gravitational lensing of gravitational waves in Einstein Telescope
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Reconsidering the Effects of Local Star Formation On Type Ia Supernova Cosmology
• Forecasts for CMB μ- and i-type spectral distortion constraints on the primordial power spectrum on scales 8 < k < 10^4 Mpc^-1 with the future Pixie-like experiments
• The Carnegie Hubble Program
• Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz
• Combining Planck with Large Scale Structure gives strong neutrino mass constraint
• A search for sterile neutrinos with the latest cosmological observations
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• The impact of a new median statistics $H_0$ prior on the evidence for dark radiation
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Constraining $f(T)$ Theories with the Varying Gravitational Constant
• SN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phase
• New approaches to SNe Ia progenitors
• AIC and BIC for cosmological interacting scenarios
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Cosmography from two-image lens systems: overcoming the lens profile slope degeneracy
• Cosmological constraints on coupled dark energy
• Reconciling Large And Small-Scale Structure In Twin Higgs Models
• Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
• Large Magellanic Cloud Near-Infrared Synoptic Survey. II. The Wesenheit relations and their application to the Distance scale
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Aspects of Axion $F(R)$ Gravity
• Cosmological dynamics of dark energy in scalar-torsion $f(T,\varphi )$ gravity
• Constraining the Cosmology of the Phantom Brane using Distance Measures
• Clustering of Photometric Luminous Red Galaxies II: Cosmological Implications from the Baryon Acoustic Scale
• The very young resolved stellar populations around stripped-envelope supernovae
• Topology and Dark Energy: Testing Gravity in Voids
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
• K-inflationary Power Spectra at Second Order
• Singlet extensions and W boson mass in the light of the CDF II result
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Dark Radiation and interacting scenarios
• Wormhole geometries in Eddington-inspired Born-Infeld gravity
• Can all cosmological observations be accurately interpreted with a unique geometry?
• The Degree of Fine-Tuning in our Universe -- and Others
• A test of Gaia Data Release 1 parallaxes: implications for the local distance scale
• On the Bias of the Distance-Redshift Relation from Gravitational Lensing
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• An accurate measurement of the baryonic Tully-Fisher relation with heavily gas-dominated ALFALFA galaxies
• Gravitational wave background from rotating neutron stars
• Probing the neutrino mass hierarchy with CMB weak lensing
• New limits on Early Dark Energy from the South Pole Telescope
• Evidence for extra radiation? Profile likelihood versus Bayesian posterior
• A Council of Giants
• Is there a concordance value for $H_0$?
• LMC Blue Supergiant Stars and the Calibration of the Flux-weighted Gravity--Luminosity Relationship
• Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 -- II. Resolved common proper motion pairs
• Probing Dark Energy through Scale Dependence
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Planck intermediate results. XXIV. Constraints on variation of fundamental constants
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Constraining dark matter properties with Cosmic Microwave Background observations
• Constraining Supersymmetry using the relic density and the Higgs boson
• Horava Gravity in the Effective Field Theory formalism: from cosmology to observational constraints
• A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method
• Tuning in on Cepheids: Radial velocity amplitude modulations. A source of systematic uncertainty for Baade-Wesselink distances
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Real-space density profile reconstruction of stacked voids
• Hubble constant and dark energy inferred from free-form determined time delay distances
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Revisiting Studies of the Statistical Property of a Strong Gravitational Lens System and Model-independent Constraint on the Curvature of the Universe
• Investigating Cepheid $\ell$ Carinae's Cycle-to-cycle Variations via Contemporaneous Velocimetry and Interferometry
• Probing nuclear rates with Planck and BICEP2
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• Connecting neutrino physics with dark matter
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• Constraints on the CMB temperature redshift dependence from SZ and distance measurements
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Halo clustering and g_{NL}-type primordial non-Gaussianity
• A combined measurement of cosmic growth and expansion from clusters of galaxies, the CMB and galaxy clustering
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
• Standard-siren cosmology using gravitational waves from binary black holes
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• The Effect of Weak Lensing on Distance Estimates from Supernovae
• The VMC Survey. VIII. First results for Anomalous Cepheids
• Dark Matter properties through cosmic history
• Tension in the Void: Cosmic Rulers Strain Inhomogeneous Cosmologies
• Constraints on Galileon-induced precessions from solar system orbital motions
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• Cosmological perturbations and observational constraints on nonlocal massive gravity
• $H_0$ from ten well-measured time delay lenses
• Dark Radiation candidates after Planck
• Testing cosmic opacity from SNe Ia and Hubble parameter through three cosmological-model-independent methods
• Priors on the effective Dark Energy equation of state in scalar-tensor theories
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Differential cosmic expansion and the Hubble flow anisotropy
• Spitzer UltRa Faint SUrvey Program (SURFS UP) I: An Overview
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• On the local variation of the Hubble constant
• A Global Physical Model for Cepheids
• On the Application of Wesenheit Function in Deriving Distance to Galactic Cepheids
• Measurement of the expansion rate of the Universe from γ-ray attenuation
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Consistency of the local Hubble constant with the cosmic microwave background
• Exploring the evidence for a large local void with supernovae Ia data
• Viability of Bianchi type V Universe in $f(R,T)=f_1(R)+f_2(R)f_3(T)$ gravity
• $H_0$ tension and the String Swampland
• Low-l CMB Power Loss in String Inflation
• The Mid-Infrared Tully-Fisher Relation: Calibration of the SNIa Scale and Ho
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Ambiguous Tests of General Relativity on Cosmological Scales
• Is the Universe Transparent?
• The need for accurate redshifts in supernova cosmology
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• High-precision distance measurements with classical pulsating stars
• Observational calibration of the projection factor of Cepheids - III. The long-period Galactic Cepheid RS Puppis
• Model independent constraints on transition redshift
• The VMC Survey. XIX. Classical Cepheids in the Small Magellanic Cloud
• Constructing a cosmological model-independent Hubble diagram of type Ia supernovae with cosmic chronometers
• The trouble with Hubble: Local versus global expansion rates in inhomogeneous cosmological simulations with numerical relativity
• Virialisation-induced curvature as a physical explanation for dark energy
• Beyond H_0 and q_0: Cosmology is no longer just two numbers
• Constraining the dark energy models with H(z) data: an approach independent of $H_0$
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Cosmological implications of $n_s\approx 1$ in light of the Hubble tension
• Late time acceleration due to generic modification of gravity and Hubble tension
• Constraining Dust Extinction Properties via the VVV Survey
• Dark Energy and Fate of the Universe
• Constraining chameleon field driven warm inflation with Planck 2018 data
• The Araucaria Project: The First-Overtone Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Interacting dark sector with variable vacuum energy
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Observational calibration of the projection factor of Cepheids IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids
• Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos
• (Lack of) Cosmological evidence for dark radiation after Planck
• Red Supergiants as cosmic abundance probes: the first direct metallicity determination of NGC 4038 in the Antennae
• Parametrized modified gravity constraints after Planck
• Transition Redshift: New constraints from parametric and nonparametric methods
• Cosmicflows-2: SNIa Calibration and H0
• Spitzer observations of SN 2014J and properties of mid-IR emission in Type Ia supernovae
• Quintessence with Yukawa Interaction
• Using the Tip of the Red Giant Branch as a Distance Indicator in the Near Infrared
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Redshift drift exploration for interacting dark energy
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Are $H_0$ and ${\sigma }_8$ tensions generic to present cosmological data?
• Large Magellanic Cloud Near-Infrared Synoptic Survey. III. A Statistical Study of Non-Linearity in the Leavitt Laws
• Neutrino and Dark Radiation properties in light of latest CMB observations
• Light propagation and the average expansion rate in near-FRW universes
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• Detecting the cosmological neutrino background in the CMB
• Simultaneous constraints on the number and mass of relativistic species
• Galaxy cluster number count data constraints on cosmological parameters
• Interacting viscous dark fluids
• $\nu$Galileon: modified gravity with massive neutrinos as a testable alternative to $\Lambda$CDM
• Soft singularity crossing and transformation of matter properties
• A direct measurement of tomographic lensing power spectra from CFHTLenS
• GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle
• Analysis of Generalized Ghost Pilgrim Dark Energy in Non-flat FRW Universe
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• High Redshift Standard Candles: Predicted Cosmological Constraints
• The luminosity of supernovae of type Ia from TRGB distances and the value of H_0
• Constraining Variations in the Fine Structure Constant in the presence of Early Dark Energy
• The fate of the Antennae galaxies
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• New Limits on Coupled Dark Energy from Planck
• A Comparative Study of Dark Energy Constraints from Current Observational Data
• On Cepheid Distance Scale Bias due to Stellar Companions and Cluster Populations
• Probing the time dependence of dark energy
• The Fine Structure Constant and the CMB Damping Scale
• Probing spatial homogeneity with LTB models: a detailed discussion
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• Non-thermal WIMPs as "Dark Radiation" in Light of ATACAMA, SPT, WMAP9 and Planck
• An extended theoretical scenario for Classical Cepheids. I. Modeling Galactic Cepheids in the Gaia photometric system
• A hint of matter underdensity at low $z$?
• The Distance to M101 Hosting Type Ia SN 2011fe Based on the Tip of the Red Giant Branch
• Constraints on a $\varphi$CDM model from strong gravitational lensing and updated Hubble parameter measurements
• New Constraints On The Dark Energy Equation of State
• The Secret Lives of Cepheids: Evolutionary Changes and Pulsation-Induced Shock Heating in the Prototype Classical Cepheid δ Cep
• Transit cosmological models with observational constraints in f(Q, T) gravity
• Zero Impact Parameter White Dwarf Collisions in FLASH
• The Dark Side of the Universe after Planck
• Are Light Sterile Neutrinos Preferred or Disfavored by Cosmology?
• Theoretical fit of Cepheid light an radial velocity curves in the Large Magellanic Cloud cluster NGC 1866
• Still Brighter than Pre-Explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Holographic Dark Energy with Cosmological Constant
• Stability of scalar perturbations in scalar-torsion $f(T,\varphi )$ gravity theories in the presence of a matter fluid
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Vetting Galactic Leavitt Law Calibrators using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids
• The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic Cloud
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• A highly magnified supernova at z=1.703 behind the massive galaxy cluster Abell 1689
• Probing the dynamics of dark energy with divergence-free parametrizations: A global fit study
• A Direct Stellar Metallicity Determination in the Disk of the Maser Galaxy NGC4258
• Revisiting the interacting model of new agegraphic dark energy
• A supernova distance to the anchor galaxy NGC 4258
• Spherically symmetric Einstein-aether perfect fluid models
• Parameters of cosmological models and recent astronomical observations
• Interacting two-component fluid models with varying EoS parameter
• Information Gains from Cosmological Probes
• A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude - Rate of Decline Relation for Novae as a Non-Standard Candle, and a Prediction of the Existence of Ultrafast Novae
• Evaluating Systematic Dependencies of Type Ia Supernovae: The Influence of Central Density
• Two Fluid Scenario in Bianchi Type-I Universe
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
• Timescape cosmology with radiation fluid
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Generalized Second Law of Thermodynamics in $f(T,T_G)$ gravity
• Testing standard and non-standard neutrino physics with cosmological data
• The KBC Void: Consistency with Supernovae Type Ia and the Kinematic SZ Effect in a $\Lambda$LTB Model
• Properties of M31. II: A Cepheid disk sample derived from the first year of PS1 PAndromeda data
• A Perturbative Approach to the Redshift Space Correlation Function: Beyond the Standard Model
• W-WIMP Annihilation as a Source of the Fermi Bubbles
• HARPS-N high spectral resolution observations of Cepheids I. The Baade-Wesselink projection factor of δ Cep revisited
• What is the distance to the CMB?
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Post-Planck Dark Energy Constraints
• Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9
• Distance Dependent Offsets between Parallaxes for Nearby Stars and Gaia DR1 Parallaxes
• Inflationary Freedom and Cosmological Neutrino Constraints
• Do the observational data favor a local void?
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• An Empirical Explanation of the Anomalous Increases in the Astronomical Unit and the Lunar Eccentricity
• First experimental constraints on the disformally coupled Galileon model
• Constraint on $f(R)$ Gravity through the Redshift Space Distortion
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Tickling the CMB damping tail: scrutinizing the tension between the ACT and SPT experiments
• Localizing modes of massive fermions and a U(1) gauge field in the inflating baby-skyrmion branes
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Cepheid limb darkening, angular diameter corrections, and projection factor from static spherical model stellar atmospheres
• The Tip of the Red Giant Branch Distance to the Perfect Spiral Galaxy M74 Hosting Three Core-Collapse Supernovae
• The Structure of the Strongly Lensed Gamma-ray Source B2 0218+35
• Persistent C II Absorption in the Normal Type Ia Supernova 2002fk
• Composition of Low Redshift Halo Gas
• Testing modified gravity models with recent cosmological observations
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• Dark Matter from Late Invisible Decays to/of Gravitinos
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• Convection, granulation and period jitter in classical Cepheids
• Constraints on Lema\^ıtre-Tolman-Bondi models from Observational Hubble Parameter data
• Modified Brans-Dicke cosmology with matter-scalar field interaction
• Testing nonstandard cosmological models with SNLS3 supernova data and other cosmological probes
• How SN Ia host-galaxy properties affect cosmological parameters
• Emergent Dark Universe and the Swampland Criteria
• Current Challenges in Cepheid Distance Calibrations Using Gaia EDR3
• The M31 Near-Infrared Period-Luminosity Relation and its non-linearity for $\delta$ Cep Variables with $0.5\le \log (P)\le 1.7$
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Separate Constraints on Early and Late Cosmology
• The absolute age of the globular cluster M15 using near-infrared adaptive optics images from PISCES/LBT
• Cosmological Analysis of Pilgrim Dark Energy in Loop Quantum Cosmology
• Cosmological model of the interaction between dark matter and dark energy
• Dark Radiation in Anisotropic LARGE Volume Compactifications
• Hubble Frontier Field Photometric Catalogues of Abell 370 and RXC J2248.7-4431: Multiwavelength photometry, photometric redshifts, and stellar properties
• Studying the precision of ray tracing techniques with Szekeres models
• Formulation and constraints on decaying dark matter with finite mass daughter particles
• On the equivalence of Lambda(t) and gravitationally induced particle production cosmologies
• Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data
• A Mid-infrared Study of RR Lyrae Stars with the WISE All-Sky Data Release
• A comment on power-law inflation with a dark radiation component
• Observational effects of a running Planck mass
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Polarization Predictions for Inflationary CMB Power Spectrum Features
• General Analysis of Dark Radiation in Sequestered String Models
• Generalized Holographic Dark Energy and its Observational Constraints
• MeV dark matter in the 3+1+1 model
• Ultra Long Period Cepheids: a primary standard candle out to the Hubble flow
• Variability, periodicity and contact binaries in WISE
• Significant Luminosity Differences of Two Twin Type Ia Supernovae
• Updated constraints from the PLANCK experiment on modified gravity
• Testing for a large local void by investigating the Near-Infrared Galaxy Luminosity Function
• Pre-flight integration and characterization of the SPIDER balloon-borne telescope
• Measuring growth index in a universe with sterile neutrinos
• The Cepheid distance to the maser-host galaxy NGC 4258: Studying systematics with the Large Binocular Telescope
• Searching for deviations from the General Relativity Theory with gas mass fraction of galaxy clusters and complementary probes
• Cosmographic Degeneracy
• A global fit study on the new agegraphic dark energy model
• Cosmological evidence for leptonic asymmetry after Planck
• The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence
• Observational calibration of the projection factor of Cepheids I. The Type II Cepheid kappa Pavonis
• Growth Index after the Planck Results
• Cosmological Parameter Determination in Free-Form Strong Gravitational Lens Modeling
• GERLUMPH Data Release 2: 2.5 billion simulated microlensing light curves
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• Phantom braneworld and the Hubble tension
• On dark energy models of single scalar field
• Sound speed of scalar field dark energy: weak effects and large uncertainties
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Violation of the FRW consistency condition as a signature of backreaction
• Consistent radial velocities of classical Cepheids from the cross-correlation technique
• String Cosmology - Large-Field Inflation in String Theory
• An updated Type II supernova Hubble diagram
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Bulk Viscous Matter-dominated Universes: Asymptotic Properties
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Parameter estimation with Sandage-Loeb test
• A one-parameter formula for testing slow-roll dark energy: observational prospects
• Relations between canonical and non-canonical inflation
• Some clarifications about Lemaître-Tolman models of the Universe used to deal with the dark energy problem
• Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31
• Dark Radiation after Planck
• The HI content of extremely metal-deficient blue compact dwarf galaxies
• VEGA/CHARA interferometric observations of Cepheids. I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range
• Constraining the local variance of $H_0$ from directional analyses
• Cosmological Constraints on the Gravitational Interactions of Matter and Dark Matter
• Hubble constant and sound horizon from the late-time Universe
• Dark Radiation and Decaying Matter
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• A tachyonic scalar field with mutually interacting components
• Cosmological Effects of Scalar-Photon Couplings: Dark Energy and Varying-alpha Models
• A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
• Gravitational Lenses as High-Resolution Telescopes
• The variance of the locally measured Hubble parameter explained with different estimators
• Dark radiation and dark matter in supersymmetric axion models with high reheating temperature
• Quantum Gravity and Inflation
• Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
• Confronting DGP Braneworld Gravity with Cosmic Observations after Planck Data
• Redshift drift constraints on holographic dark energy
• The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit
• Probing bulk viscous matter-dominated models with Gamma-ray bursts
• Hořava-Lifshitz cosmology in light of new data
• Globular Clusters and Spur Clusters in NGC 4921, the Brightest Spiral Galaxy in the Coma Cluster
• Surface Brightness Fluctuations as Primary and Secondary Distance Indicators
• Neutrino Anisotropies after Planck
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• New Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Bolometric Lightcurves of Peculiar Type II-P Supernovae
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. II. M66 and M96 in the Leo I Group
• The long-period Galactic Cepheid RS Puppis - III. A geometric distance from HST polarimetric imaging of its light echoes
• Non-Gaussian isocurvature perturbations in dark radiation
• Quantifying the impact of future Sandage-Loeb test data on dark energy constraints
• Updated theoretical Period-Age and Period-Age-Color relations for Galactic Classical Cepheids: an application to the Gaia DR2 sample
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Application of Bayesian graphs to SN Ia data analysis and compression
• Planck Satellite Constraints on Pseudo-Nambu--Goldstone Boson Quintessence
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Early dark energy and its interaction with dark matter
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• A 3% Determination of $H_0$ at Intermediate Redshifts
• HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• How Flat is Our Universe Really?
• Modified theory of gravity and the history of cosmic evolution
• Uncertainties in The Interstellar Extinction Curve and the Cepheid Distance to M101
• 3.5 keV X-ray line and R-Parity Conserving Supersymmetry
• Tilt of primordial gravitational wave spectrum in a universe with sterile neutrinos
• A Minimal Model of Majoronic Dark Radiation and Dark Matter
• The fate of small classically stable Q-balls
• Noether symmetry in $f(T)$ teleparallel gravity
• Cosmological acceleration
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• Multicomponent Dark Matter in Radiative Seesaw Models
• Bayesian correction of $H(z)$ data uncertainties
• Galaxy clusters, type Ia supernovae and the fine structure constant
• The Local Value of $H_0$ in an Inhomogeneous Universe
• The traces of anisotropic dark energy in light of Planck
• Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars
• Pulse-wise Amati correlation in Fermi GRBs
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• The Baade-Wesselink p-factor applicable to LMC Cepheids
• Light dark matter versus astrophysical constraints
• Light Sterile Neutrinos and Inflationary Freedom
• Age Problem in Lemaitre-Tolman-Bondi Void Models
• Constraints on decaying early modified gravity from cosmological observations
• A 4% measurement of $H_0$ using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
• Anchors for the Cosmic Distance Scale: the Cepheids U Sgr, CF Cas and CEab Cas
• Integrated Cosmological Probes: Extended Analysis
• Cold dark energy constraints from the abundance of galaxy clusters
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• Structure growth in $f(Q)$ cosmology
• Observable Quantities in Weyl Gravity
• Late-time vacuum phase transitions: Connecting sub-eV scale physics with cosmological structure formation
• Local cosmological effects of the order of H in the orbital motion of a binary system
• Confronting Tracker Field Quintessence with Data
• Testing dark energy using pairs of galaxies in redshift space
• X-ray Binaries and Star Clusters in the Antennae: Optical Cluster Counterparts
• Radio Monitoring Campaigns of Six Strongly Lensed Quasars
• Planck constant as adiabatic invariant characterized by Hubble's and cosmological constants
• Period-Luminosity Relations for Cepheid Variables: From Mid-Infrared to Multi-Phase
• The Scale of Inflation in the Landscape
• Bounds on Neutrino Mass in Viscous Cosmology
• A Brief History of Curvature
• The effect of different observational data on the constraints of cosmological parameters
• Tracing the cosmic velocity field at z ~ 0.1 from galaxy luminosities in the SDSS DR7
• Inflation with F(T) Teleparallel Gravity
• Phantom crossing dark energy in Horndeski's theory
• Relationship between the CMB, SZ Cluster Counts, and Local Hubble Parameter Measurements in a Simple Void Model
• A First Look at Cepheids in a SN Ia Host with JWST
• Discovery of the Host Cluster for the Fundamental Cepheid Calibrator Zeta Gem
• Addressing Cosmological Tensions by Non-Local Gravity
• Blending of Cepheids in M33
• On general features of warm dark matter with reduced relativistic gas
• Cepheid Variables in the Maser-Host Galaxy NGC 4258
• Phenomenology of Gravitational Aether as a solution to the Old Cosmological Constant Problem
• Cosmological constraints on the new holographic dark energy model with action principle
• Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope
• Probing interactions within the dark matter sector via extra radiation contributions
• Precision cosmology with time delay lenses: high resolution imaging requirements
• Differentiating dark interactions with perturbation
• Gravitational Waves: A Test for Modified Gravity
• Forecasts on interacting dark energy with standard sirens
• The strange evolution of the Large Magellanic Cloud Cepheid OGLE-LMC-CEP1812
• A Rich Tapestry: Supersymmetric Axions, Dark Radiation, and Inflationary Reheating
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods
• Is the CMB telling us that dark matter is weaker than weakly interacting?
• Non-Canonical Inflation in Supergravity
• Dynamics and constraints of the dissipative Liouville cosmology
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: Implications for $H_0$
• Determining $H_0$ with the latest HII galaxy measurements
• Distance Probes of Dark Energy
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Revisiting a model-independent dark energy reconstruction method
• Galactic open cluster Cepheids -- a census based on Gaia EDR3
• The tension on the cosmological parameters from different observational data
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• The Reactor Anomaly after Daya Bay and RENO
• Estimating the uncorrelated dark energy evolution in the Planck era
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• Consequences of f(R)-theories of gravity on gravitational leptogenesis
• The BICEP2 data and a single Higgs-like interacting tachyonic field
• Weinberg's Higgs portal confronting recent LUX and LHC results together with upper limits on B^+ and K^+ decay into invisibles
• A Multiband Generalization of the Analysis of Variance Period Estimation Algorithm and the Effect of Inter-band Observing Cadence on Period Recovery Rate
• Unified cosmology with Non-minimally coupled scalar-tensor theory of gravity
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• Constraints on Modified Gravity from ACT and SPT
• Dynamics of Elliptical Galaxies with Planetary Nebulae in Modified Newtonian Dynamics
• Isocurvature perturbations and tensor mode in light of Planck and BICEP2
• A Cepheid-Based Distance to the Seyfert Galaxy NGC 6814
• FLRW accelerating universe with interactive dark energy
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• An FLRW interacting dark energy model of the Universe
• Accidental Inflation from Kähler Uplifting
• Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
• Revised cosmological parameters after BICEP 2 and BOSS
• The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Frequency analysis of OGLE-IV photometry for classical Cepheids in Galactic fields: non-radial modes and modulations
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• Anchoring the Distance Scale via X-ray/IR Data for Cepheid Clusters: SU Cas
• HARPS-N high spectral resolution observations of Cepheids II. The impact of the surface-brightness color relation on the Baade-Wesselink projection factor of eta Aql
• Cosmological constraints from low-redshift data
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• Cosmological Tests with the Joint Lightcurve Analysis
• Supernovae as probes of cosmic parameters: estimating the bias from under-dense lines of sight
• Detection of a Light Echo from the Otherwise Normal SN 2007af
• Probing a light dark sector at future lepton colliders via invisible decays of the SM-like and dark Higgs bosons
• FRW dark energy cosmological model with hybrid expansion law
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• The Cepheids of NGC1866: A Precise Benchmark for the Extragalactic Distance Scale and Stellar Evolution from Modern UBVI Photometry
• Integrated cosmological probes: Concordance quantified
• Period-Luminosity relations derived from the OGLE-III First-overtone mode Cepheids in the Magellanic Clouds
• Some consequences of the Majoron being the dark radiation
• Constraints on Lepton Asymmetry from Nucleosynthesis in a Linearly Coasting Cosmology
• Confronting brane inflation with Planck and pre-Planck data
• Constraints on $\Lambda (t)$CDM models as holographic and agegraphic dark energy with the observational Hubble parameter data
• Kinematic Bias in Cosmological Distance Measurement
• Combined cosmological tests of a bivalent tachyonic dark energy scalar field model
• A gauge-invariant approach to interactions in the dark sector
• Redshift drift constraints on f(T) gravity
• Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
• Constraints on single-field inflation with WMAP, SPT and ACT data -- A last-minute stand before Planck
• A New Collisional Ring Galaxy at z = 0.111: Auriga's Wheel
• The effective Lagrangian of dark energy from observations
• Directional dependence of the local estimation of $H_0$ and the non perturbative effects of primordial curvature perturbations
• Deviation From ΛCDM With Cosmic Strings Networks
• Confronting Dark Energy Anisotropic Stress
• Dark Energy Scaling from Dark Matter to Acceleration
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• On Silicon Group Elements Ejected by Supernovae Type Ia
• Testing the nature of Dark Energy with Precision Cosmological constraints
• Observational tests of backreaction with recent data
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Evolution of shifted cosmological parameter and shifted dust matter in a two-phase tachyonic field universe
• Light Dark Matter and Dark Radiation
• Updated 24 $\mu \mathrm{m}$ Period-Luminosity Relation Derived from Galactic Cepheids
• Young and Intermediate-age Distance Indicators
• The effect of interacting dark energy on local measurements of the Hubble constant
• Reactor sterile neutrinos, dark energy and the age of the universe
• First cosmological constraints on the Superfluid Chaplygin gas model
• Dark Energy and Inflation in a Gravitational Wave Dominated Universe
• Gamma ray burst distances and the timescape cosmology
• Impact of distance determinations on Galactic structure. II. Old tracers
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Testing the $R_{\mathrm{h}}=ct$ Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances
• Mathematical Underpinnings of the Multi-Wavelength Structure of the TRGB
• Optimizing parameter constraints: a new tool for Fisher matrix forecasts
• Cosmology with powerful radio-loud AGNs
• Non-Gaussian forecasts of weak lensing with and without priors
• Evidence for Rapid Variability in the Optical Light Curve of the Type Ia SN 2014J
• Angular distribution of cosmological parameters as a probe of inhomogeneities: a kinematic parametrisation
• The Dark Energy Cosmic Clock: A New Way to Parametrise the Equation of State
• Cosmological data and indications for new physics
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Investigating the Hubble Tension: Effect of Cepheid Calibration
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• The Tilt of Primordial Gravitational Waves Spectra from BICEP2
• Phi Zeta Delta: Growth of Perturbations in Parameterized Gravity for an Einstein-de Sitter Universe
• Robustness of $H_0$ determination at intermediate redshifts
• Cosmic Bose dark matter
• Modified Regge calculus as an explanation of dark energy
• Dark matter indirect detection signals and the nature of neutrinos in the supersymmetric $U(1{)}_{B-L}$ extension of the standard model
• No stable dissipative phantom scenario in the framework of a complete cosmological dynamics
• The Darkness of Spin-0 Dark Radiation
• Observational constraints from SNe Ia and Gamma-Ray Bursts on a clumpy universe
• Strongly Lensed Jets, Time Delays, and the Value of H0
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Hubble Constant, Lensing, and Time Delay in Relativistic MOND
• Model-independent measurement of the absolute magnitude of Type Ia Supernovae with gravitational-wave sources
• The parameter space of Cubic Galileon models for cosmic acceleration
• Parameter estimation of a nonlinear magnetic universe from observations
• Interacting warm dark matter
• Resonant non-Gaussianity with equilateral properties
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Identifying Contaminated K-band Globular Cluster RR Lyrae Photometry
• Cosmological surveys with multi-object spectrographs
• Effects of anisotropy on interacting ghost dark energy in Brans-Dicke theories
• Is there another coincidence problem at the reionization epoch?
• Being, Becoming and the Undivided Universe: A Dialogue between Relational Blockworld and the Implicate Order Concerning the Unification of Relativity and Quantum Theory
• Calibrating the Galactic Cepheid Period-Luminosity relation from the maximum-likelihood technique
• Predicted masses of Galactic Cepheids in the Gaia Data Release 2
• Extra relativistic degrees of freedom without extra particles using Planck data
• VI-Band Follow-Up Observations of Ultra-Long-Period Cepheid Candidates in M31
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Testing LTB Void Models Without the Cosmic Microwave Background or Large Scale Structure: New Constraints from Galaxy Ages
• Dark energy from instantons
• Interacting parametrized post-Friedmann method
• The Araucaria Project : the Baade-Wesselink projection factor of pulsating stars
• New insights into the use of Ultra Long Period Cepheids as cosmological standard candles
• Testing Distance Estimators with the Fundamental Manifold
• Astrophysical Tests of Kinematical Conformal Cosmology in Fourth-Order Conformal Weyl Gravity
• Determining $H_0$ using a model-independent method
• A hierarchical Bayesian model to infer PL(Z) relations using Gaia parallaxes
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Orbital and physical parameters, and the distance of the eclipsing binary system OGLE-LMC-ECL-25658 in the Large Magellanic Cloud
• Planck constraints on neutrino isocurvature density perturbations
• High accuracy on $H_0$ constraints from gravitational wave lensing events
• The AGN Hubble Diagram and Its Implications for Cosmology
• Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves
• Constraints on Vacuum Energy from Structure Formation and Nucleosynthesis
• Impacts on Cosmological Constraints from Degeneracies
• Reconciling BICEP2 and Planck results with right-handed Dirac neutrinos in the fundamental representation of grand unified E_6
• The Diffuse Light of the Universe - On the microwave background before and after its discovery: open questions
• Is interacting vacuum viable?
• Measuring the matter energy density and Hubble parameter from Large Scale Structure
• Distances to Galaxies from the Brightest Stars in the Universe
• A More Accurate and Competitive Estimative of $H_0$ in Intermediate Redshifts
• Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
• Constraints on the $\Lambda$CDM model with redshift tomography
• Re-Examination of Globally Flat Space-Time
• Testing the local-void alternative to dark energy using galaxy pairs
• Entropic force between two horizons of dilaton black holes with a power-Maxwell field
• Backreaction mechanism in multifluid and extended cosmologies
• Angular distribution of cosmological parameters as a probe of space-time inhomogeneities
• Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations
• Backreaction and the Covariant Formalism of General Relativity
• Gravitational Interactions and Neutrino Masses
• Generalized Ghost Dark Energy in DGP Model
• Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\varphi$) Gravity: Investigating Energy and Momentum Couplings
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• The Two-Point Correlation Function of Gamma-ray Bursts
• Milestones of general relativity: Hubble's law (1929) and the expansion of the universe
• Holographic dark information energy: Predicted dark energy measurement
• Hubble Hullabaloo and String Cosmology
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Seeking the Epoch of Maximum Luminosity for Dusty Quasars
• Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
• The Shared Causal Pasts and Futures of Cosmological Events
• CO luminosity-Linewidth correlation of low and high redshift galaxies and its possible cosmological utilization
• Stellar photometry with Multi Conjugate Adaptive Optics
• Observational constraints to a unified cosmological model
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• Phenomenological models of Universe with varying $G$ and $\Lambda$
• Complementary cosmological tests of RSII brane models
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• Impact of our local environment on cosmological statistics
• Comparing the light curves of simulated Type Ia Supernovae with observations using data-driven models
• The influence of weak lensing on measurements of the Hubble constant with quad-image gravitational lenses
• Dark matter component decaying after recombination: constraints from diffuse gamma-ray and neutrino flux measurements
• Testing Dvali-Gabadadze-Porrati Gravity with Planck
• Cosmology and the Hubble Constant: On the Megamaser Cosmology Project (MCP)
• The Circular Velocity Function of Group Galaxies
• Dynamics of cosmological perturbations in modified Brans-Dicke cosmology with matter-scalar field interaction
• The Environment of HII Galaxies revisited
• Allan Sandage and the Distance Scale
• Distance Measurements and Stellar Population Properties via Surface Brightness Fluctuations
• A Bayesian Approach to Calibrating Period-Luminosity Relations of RR Lyrae Stars in the Mid-Infrared
• The consistency test on the cosmic evolution
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
• Luminous Satellites versus Dark Subhaloes: Clustering in the Milky Way
• The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
• Averaged universe confronted with cosmological observations: A fully covariant approach
• Testing X-ray Measurements of Galaxy Cluster Gas Mass Fraction Using the Cosmic Distance-Duality Relation
• The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
• Can Massive Gravity Explain the Mass Discrepancy - Acceleration Relation of Disk Galaxies?
• Dynamical System Analysis for Scalar Field Potential in Teleparallel Gravity
• Star Formation Rate in late-type galaxies: I- The H(alpha) and FUV integrated values
• Neutrino oscillations in the presence of super-light sterile neutrinos
• Estimating a Common Period for a Set of Irregularly Sampled Functions with Applications to Periodic Variable Star Data
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Matter-wave coherence limit owing to cosmic gravitational wave background
• Stretch to stretch, dust to dust: lower-value local $H_0$ measurement from two-population modelling of type Ia supernovae
• Einstein's cosmological considerations
• Noncommutative cosmological models induced by a symplectic formalism coupled to phantom fluids
• Dark energy model with very large-scale inhomogeneity
• The expansion of the universe observed with supernovae
• Critical points of the cosmic velocity field and the uncertainties in the value of the Hubble constant
• Viability tests of \textit{f(R)}-gravity models with Supernovae Type 1A data
• $g_{\mathrm{NL}}$ in the curvaton model constrained by PLANCK
• Tomographic Alcock-Paczynski Method with Redshift Errors
• Anisotropic cosmological solutions to the $Y(R)F^2$ gravity
• Non-linear coupling in the dark sector as a running vacuum model
• Einstein-aether models III: conformally static metrics, perfect fluid and scalar fields
• On the possible onset of the Pioneer anomaly
• Inflation of the Universe by the Non-minimal $Y(R)F^2$ Models
• Exploring neutralino dark matter resonance annihilation via bA,bH -> b mu^+ mu^- at the LHC
• Giant monopoles as a dark matter candidate
• Considering light-matter interactions in the Friedmann equations
• Neutrino physics from future weak lensing surveys
• Distance determination from the Cepheids and RR Lyrae period-luminosity relations
• An approach to robust Bayesian regression in astronomy
• Dark energy with rigid voids versus relativistic voids alone
• The First Three Rungs of the Cosmological Distance Ladder
• Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSST
• A Dynamic Dark Information Energy Consistent with Planck Data
• Asteroseismology, standard candles and the Hubble Constant: what is the role of asteroseismology in the era of precision cosmology?
• On Direct Estimation of Density Parameters and Hubble Constant for $\Lambda$CDM Universe using Hubble Measurements
• A note on dark matter and dark energy
• Toward a Measurement of the Transverse Peculiar Velocity of Galaxy Pairs
• Consistencies and inconsistencies in redshift-independent distances
• Super-horizon second-order perturbations for cosmological random fluctuations and the Hubble-constant problem
• Dark aspects of massive spinor electrodynamics
• Inhomogeneous Cosmology Redux
• Cosmic microwave background constraints on coupled dark matter
• Observable predictions of generalised inflationary scenarios
• Toy models of Universe with an Effective varying $\Lambda$-Term in Lyra Manifold
• Parameter space stability of multiple soft interactions
• The Constraint of H0from Galaxy clusters and Hubble parameter data
• Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy
• The Cosmological Effect of CMB/BAO Measurements
• Low-velocity cosmic strings in accelerating universe
• A scaling relation in [C II]-detected galaxies and its likely application in cosmology
• Thermodynamics of irreversible particle creation phenomena and its cosmological consequence
• Irreversible Thermodynamics of the Universe: Constraints from Planck Data
• Semi-realistic Bouncing Domain Wall Cosmology
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST
• Gravitational lensing by a black hole in Poincar{é} gauge theory of gravity
• Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
• Dusty Quasars at High Redshifts
• Finding Possibility of Dynamical Dark Energy with Hubble Parameters
• Viscous Cold Dark Matter in agreement with observations
• Cosmic Dark Energy Emerging from Gravitationally Effective Vacuum Fluctuations
• Hubble tension problem encompassed by phase-space quantum cosmology
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• $G_3$ -- interacting scalar tensor dark energy
• Near-infrared observations of OGLE classical and type II Cepheid variables in the LMC
• From Solar Eclipse of 1919 to the Spectacle of Gravitational Lensing
• K-matter as Mach's principle realization
• Cosmological constraints on sterile neutrino Dark Matter production mechanisms
• Dark energy model selection with current and future data
• Influence from cosmological uncertainties on galaxy number count at faint limit
• Dark Radiation and Inflationary Freedom
• A Relationship between the Comoving Particle Number and the Effective Cosmological Constant
• Constraints on a vacuum energy from both SNIa and CMB temperature observations
• Dark Radiation and Inflationary Freedom
• Understanding the wicked world that surrounds you
• Modelling the current accelerated expansion of the Universe with Holographic Dark Energy
• Amplitude Modulation of Cepheid Radial Velocity Curves as a Systematic Source of Uncertainty for Baade-Wesselink Distances
• A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time
• El Modelo Estandar de la Cosmologia Moderna en Jaque
• Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA
• A partially occulting MACHO-microlensing event in the Twin Quasar Q0957+561
• Qualitative analysis of Einstein-aether models with perfect fluid and scalar fields
• PISCOLA: a data-driven transient light-curve fitter
• Optimizing Observational Strategy for Future Fgas Constraints
• Spatial disconnection between stellar and dust emissions: the test of the Antennae Galaxies (Arp 244)
• Prospects of the multi-channel photometric survey telescope in the cosmological application of Type Ia supernovae