Unveiling the Universe with Emerging Cosmological Probes

Abstract

The detection of the accelerated expansion of the Universe has been one of the major breakthroughs in modern cosmology. Several cosmological probes (CMB, SNe Ia, BAO) have been studied in depth to better understand the nature of the mechanism driving this acceleration, and they are being currently pushed to their limits, obtaining remarkable constraints that allowed us to shape the standard cosmological model. In parallel to that, however, the percent precision achieved has recently revealed apparent tensions between measurements obtained from different methods. These are either indicating some unaccounted systematic effects, or are pointing toward new physics. Following the development of CMB, SNe, and BAO cosmology, it is critical to extend our selection of cosmological probes. Novel probes can be exploited to validate results, control or mitigate systematic effects, and, most importantly, to increase the accuracy and robustness of our results. This review is meant to provide a state-of-art benchmark of the latest advances in emerging beyond-standard cosmological probes. We present how several different methods can become a key resource for observational cosmology. In particular, we review cosmic chronometers, quasars, gamma-ray bursts, standard sirens, lensing time-delay with galaxies and clusters, cosmic voids, neutral hydrogen intensity mapping, surface brightness fluctuations, stellar ages of the oldest objects, secular redshift drift, and clustering of standard candles. The review describes the method, systematics, and results of each probe in a homogeneous way, giving the reader a clear picture of the available innovative methods that have been introduced in recent years and how to apply them. The review also discusses the potential synergies and complementarities between the various probes, exploring how they will contribute to the future of modern cosmology.

arXiv commentInvited review article for Living Reviews in Relativity. Accepted version. 191 pages, 54 figures, 11 tables

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• Observational constraints on cosmological solutions of $f(Q)$ theories
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• Blind foreground subtraction for intensity mapping experiments
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• Concerns regarding the use of black hole shadows as standard rulers
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• Observational Constraints on Cosmological Models with the Updated Long Gamma-Ray Bursts
• CLASH-VLT: A Highly Precise Strong Lensing Model of the Galaxy Cluster RXC J2248.7-4431 (Abell S1063) and Prospects for Cosmography
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• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogues and Measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample
• Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters
• The abundance of voids and the excursion set formalism
• Quasars as standard candles I: The physical relation between disc and coronal emission
• Marginal evidence for cosmic acceleration from Type Ia supernovae
• Characterization of systematic error in Advanced LIGO calibration
• Cosmographic analysis with Chebyshev polynomials
• Gravitational Radiation, Inspiraling Binaries, and Cosmology
• The effect of peculiar velocities on supernova cosmology
• Physics of Gamma-Ray Bursts Prompt Emission
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Ultra large-scale cosmology in next-generation experiments with single tracers
• A measurement of the Hubble constant from Type II supernovae
• A first application of the Alcock-Paczynski test to stacked cosmic voids
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• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
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• The Epeak-Eiso plane of long Gamma Ray Bursts and selection effects
• Gamma-ray Burst Cosmology
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• The Santiago-Harvard-Edinburgh-Durham void comparison I: SHEDding light on chameleon gravity tests
• Discovery of a tight correlation among the prompt emission properties of long Gamma Ray Bursts
• Statistical 21-cm Signal Separation via Gaussian Process Regression Analysis
• Spectral-Luminosity relation within individual Fermi GRBs
• A Population of Massive and Evolved Galaxies at z$\ga$5
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• The fate of large-scale structure in modified gravity after GW170817 and GRB170817A
• Lens Modeling Abell 370: Crowning the Final Frontier Field with MUSE
• Using H(z) data as a probe of the concordance model
• First measurement of gravitational lensing by cosmic voids in SDSS
• The mass-sheet degeneracy and time-delay cosmography: Analysis of the strong lens RXJ1131-1231
• Simulating nonlinear cosmological structure formation with massive neutrinos
• Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data
• The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
• The story of supernova 'Refsdal' told by MUSE
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses IX. Time delays, lens dynamics and baryonic fraction in HE 0435-1223
• Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
• Hunting down horizon-scale effects with multi-wavelength surveys
• H0LiCOW III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435-1223 through weighted galaxy counts
• Cosmology with Void-Galaxy Correlations
• H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$
• An updated Gamma Ray Bursts Hubble diagram
• Setting the Stage for Cosmic Chronometers. I. Assessing the Impact of Young Stellar Populations on Hubble Parameter Measurements
• Cosmological versus Intrinsic: The Correlation between Intensity and the Peak of the nu F_nu Spectrum of Gamma Ray Bursts
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Dissecting the Gravitational Lens B1608+656. I. Lens Potential Reconstruction
• COSMOGRAIL XVI: Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring
• A ground-based 21cm Baryon acoustic oscillation survey
• Weak lensing by voids in modified lensing potentials
• Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints
• Clues on void evolution II: Measuring density and velocity profiles on SDSS galaxy redshift space distortions
• A Spectroscopic Study of the Environments of Gravitational Lens Galaxies
• A Spectroscopic Survey of X-ray Selected AGN in the Northern XMM-XXL Field
• Measuring the Hubble constant with neutron star black hole mergers
• Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry
• A New Survey for Giant Arcs
• The impact of cluster mergers on arc statistics
• Surface Brightness Fluctuations in the Hubble Space Telescope ACS/WFC F814W Bandpass and an Update on Galaxy Distances
• Inferring the Age of the Universe with Globular Clusters
• The VIMOS-VLT Deep Survey. Color bimodality and the mix of galaxy populations up to z~2
• Using the Marked Power Spectrum to Detect the Signature of Neutrinos in Large-Scale Structure
• Curvature vs Distances: testing the FLRW cosmology
• Redshift-space distortions around voids
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• Measuring q_0 from the Distortion of Voids in Redshift Space
• Are peculiar velocity surveys competitive as a cosmological probe?
• Standard sirens with a running Planck mass
• VLBI measurement of the secular aberration drift
• HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies
• The Next Generation Virgo Cluster Survey (NGVS). XVIII. Measurement and Calibration of Surface Brightness Fluctuation Distances for Bright Galaxies in Virgo (and Beyond)
• The MIXR sample: AGN activity versus star formation across the cross-correlation of WISE, 3XMM, and FIRST/NVSS
• A New Hybrid Framework to Efficiently Model Lines of Sight to Gravitational Lenses
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• The effect of foreground subtraction on cosmological measurements from Intensity Mapping
• A Synthesis of Data from Fundamental Plane and Surface Brightness Fluctuation Surveys
• Finding Strong Gravitational Lenses in the DESI DECam Legacy Survey
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• Sparse sampling, galaxy bias, and voids
• The X-ray properties of $z>6$ quasars: no evident evolution of accretion physics in the first Gyr of the Universe
• Demographics of Star-forming Galaxies since $z\sim 2.5$. I. The $UVJ$ Diagram in CANDELS
• Luminosity- and morphology-dependent clustering of galaxies
• Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
• A measurement of the Alcock-Paczynski effect using cosmic voids in the SDSS
• Measuring the value of the Hubble constant "à la Refsdal"
• Self-accelerating universe in scalar-tensor theories after GW170817
• Gravitationally lensed quasars in Gaia: III. 22 new lensed quasars from Gaia Data Release 2
• Lensing Measurements of the Mass Distribution in SDSS Voids
• Infrared color selection of massive galaxies at z > 3
• The VIMOS Public Extragalactic Redshift Survey: Measuring the growth rate of structure around cosmic voids
• Gamma-Ray Bursts in $1.8<z<5.6$ Suggest that the Time Variation of the Dark Energy is Small
• Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant
• A marked correlation function for constraining modified gravity models
• Strong lensing in the MareNostrum Universe: biases in the cluster lens population
• Probing observational bounds on scalar-tensor theories from standard sirens
• Voids as a Precision Probe of Dark Energy
• Stellar Populations and Surface Brightness Fluctuations: New Observations and Models
• The Dragonfly Nearby Galaxies Survey. V. HST/ACS Observations of 23 Low Surface Brightness Objects in the Fields of NGC1052, NGC1084, M96, and NGC4258
• Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
• Strong lensing models of eight CLASH clusters from extensive spectroscopy: accurate total mass reconstructions in the cores
• Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction
• Precise Time Delays from Strongly Gravitationally Lensed Type Ia Supernovae with Chromatically Microlensed Images
• Clues on void evolution I: Large scale galaxy distributions around voids
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• A Possible Cold Imprint of Voids on the Microwave Background Radiation
• Measuring cosmological parameters with Gamma-Ray Bursts
• Measuring Distances Using Infrared Surface Brightness Fluctuations
• LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)
• Quantifying Environmental and Line-of-Sight Effects in Models of Strong Gravitational Lens Systems
• Cosmology on Ultralarge Scales with Intensity Mapping of the Neutral Hydrogen 21 cm Emission: Limits on Primordial Non-Gaussianity
• The X-ray Energy Dependence of the Relation between Optical and X-ray Emission in Quasars
• Spot the difference. Impact of different selection criteria on observed properties of passive galaxies in zCOSMOS 20-k sample
• Why multi-tracer surveys beat cosmic variance
• SuperRAENN: A Semi-supervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium Deep Survey Supernovae
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Over-constrained Gravitational Lens Models and the Hubble Constant
• Fast Radio Bursts and cosmological tests
• Synthetic stellar populations: single stellar populations, stellar interior models and primordial proto-galaxies
• Lens galaxies in the Illustris simulation: power-law models and the bias of the Hubble constant from time-delays
• Detecting the integrated Sachs-Wolfe effect with stacked voids
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Constraining the Dark Energy Equation of State with Cosmic Voids
• Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids
• A halo model for cosmological neutral hydrogen: abundances and clustering
• The Age and Metallicity Range of Early-Type Galaxies in Clusters
• Improving the precision of time-delay cosmography with observations of galaxies along the line of sight
• The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Ages of globular clusters: a new approach
• The Void Size Function in Dynamical Dark Energy Cosmologies
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• Precision cosmology with voids in the final BOSS data
• Large-Scale Clustering of Cosmic Voids
• SDSS J1029+2623: A Gravitationally Lensed Quasar with an Image Separation of 22.5 Arcseconds
• New Optical and Near-Infrared Surface Brightness Fluctuations Models. II. Young and Intermediate Age Stellar Populations
• Arc sensitivity to cluster ellipticity, asymmetries and substructures
• Beyond UVJ: More Efficient Selection of Quiescent Galaxies With UV / Mid-IR Fluxes
• Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses VII. Time delays and the Hubble constant from WFI J2033-4723
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Measurements of $H_0$ in modified gravity theories: The role of lensed quasars in the late-time Universe
• Detection of Radial Surface Brightness Fluctuation and Color Gradients in elliptical galaxies with ACS
• When are LIGO/Virgo's Big Black-Hole Mergers?
• Interpreting the unresolved intensity of cosmologically redshifted line radiation
• Early-type Galaxy Distances from the Fundamental Plane and Surface Brightness Fluctuations
• Rates and Properties of Strongly Gravitationally Lensed Supernovae and their Host Galaxies in Time-Domain Imaging Surveys
• HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations
• Degeneracies and scaling relations in general power-law models for gravitational lenses
• Mass distribution in the core of MACS J1206: robust modeling from an exceptionally large sample of central multiple images
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Probing the existence of the E_peak-E_iso correlation in long Gamma Ray Bursts
• MultiDark-Galaxies: data release and first results
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
• HOLISMOKES -- II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
• Galaxy luminosity function per morphological type up to z=1.2
• Gamma-ray burst prompt correlations: selection and instrumental effects
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• Improving time-delay cosmography with spatially resolved kinematics
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Cosmic voids in modified gravity models with massive neutrinos
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• The Nature of Extremely Red H-[4.5]>4 Galaxies revealed with SEDS and CANDELS
• Cosmic Voids in the SDSS DR12 BOSS Galaxy Sample: The Alcock-Paczynski Test
• The bias of cosmic voids in the presence of massive neutrinos
• Fast simulations for intensity mapping experiments
• Two new tests to the distance duality relation with galaxy clusters
• Theoretical Predictions for Surface Brightness Fluctuations and Implications for Stellar Populations of Elliptical Galaxies
• Massive Dead Galaxies at z~2 with HST Grism Spectroscopy I. Star Formation Histories and Metallicity Enrichment
• A Cosmic Void Catalog of SDSS DR12 BOSS Galaxies
• Optimizing spectroscopic follow-up strategies for supernova photometric classification with active learning
• The GIGANTES dataset: precision cosmology from voids in the machine learning era
• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• Voids in the SDSS DR9: observations, simulations, and the impact of the survey mask
• Distinguishing Between Void Models and Dark Energy with Cosmic Parallax and Redshift Drift
• New optical and near-infrared Surface Brightness Fluctuations models. A primary distance indicator ranging from Globular Clusters to distant galaxies?
• Jumping the gap: searching for LIGO's biggest black holes
• Multipole analysis of redshift-space distortions around cosmic voids
• Simulations for single-dish intensity mapping experiments
• CLEAR I: Ages and Metallicities of Quiescent Galaxies at $1.0<\mathbf{z}<1.8$ Derived from Deep Hubble Space Telescope Grism Data
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• The trouble beyond $H_0$ and the new cosmic triangles
• On the linearity of tracer bias around voids
• The star formation activity in cosmic voids
• 21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies
• Hubble Frontier Fields: systematic errors in strong lensing models of galaxy clusters - Implications for cosmography
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
• Gravitational lenses as cosmic rulers: density of dark matter and dark energy from time delays and velocity dispersions
• Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions
• Linear redshift space distortions for cosmic voids based on galaxies in redshift space
• The local and distant Universe: stellar ages and $H_0$
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• The Impact of Microlensing on the Standardisation of Strongly Lensed Type Ia Supernovae
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys
• Cosmic voids in coupled dark energy cosmologies: the impact of halo bias
• Standardized long gamma-ray bursts as a cosmic distance indicator
• We do not live in the R_h = c t universe
• The Optical Luminosity-Time Correlation for More Than 100 Gamma-Ray Burst Afterglows
• Using Voids to Unscreen Modified Gravity
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Soundness of Dark Energy properties
• Gravitational lensing of type Ia supernovae by galaxy clusters
• The ACS Virgo Cluster Survey IV: Data Reduction Procedures for Surface Brightness Fluctuation Measurements with the Advanced Camera for Surveys
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• The lensing and temperature imprints of voids on the Cosmic Microwave Background
• Black hole shadow as a standard ruler in cosmology
• On the accuracy of time-delay cosmography in the Frontier Fields Cluster MACS J1149.5+2223 with supernova Refsdal
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• New measurements of ${\Omega }_m$ from gamma-ray bursts
• A Pixelated Approach to Galaxy Catalogue Incompleteness: Improving the Dark Siren Measurement of the Hubble Constant
• Quasar standardization: Overcoming Selection Biases and Redshift Evolution
• Cosmological redshift-space distortion on clustering of high-redshift objects: correction for nonlinear effects in power spectrum and tests with N-body simulations
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Magnified or multiply imaged? - Search strategies for gravitationally lensed supernovae in wide-field surveys
• Weighing neutrinos with cosmic neutral hydrogen
• KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7
• Constraints on H_0 from the Central Velocity Dispersions of Lens Galaxies
• Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• On the universality of void density profiles
• The Gravitational Lens -- Galaxy Group Connection: I. Discovery of a Group Coincident with CLASS B0712+472
• The most luminous blue quasars at $3.0<z<3.3$. I. A tale of two X-ray populations
• Could quasar lensing time delays hint to a core component in halos, instead of H0 tension?
• The Distance of the Dark Matter Deficient Galaxy NGC1052-DF2
• The Infrared Surface Brightness Fluctuation Hubble Constant
• Gemini Deep Deep Survey VI: Massive Hdelta-strong galaxies at z=1
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses XII. Time delays of the doubly lensed quasars SDSS J1206+4332 and HS 2209+1914
• Recovery of 21 cm intensity maps with sparse component separation
• A new cosmological distance measure using AGN X-ray variability
• Gravitational lensing model degeneracies: Is steepness all-important?
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Studying galaxy troughs and ridges using Weak Gravitational Lensing with the Kilo-Degree Survey
• The atomic Hydrogen content of the post-reionization Universe
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• Conjoined constraints on modified gravity from the expansion history and cosmic growth
• Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
• DES meets Gaia: discovery of strongly lensed quasars from a multiplet search
• Gamma-Ray Burst Prompt Emission
• Modelling Void Abundance in Modified Gravity
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Probing 3D Structure with a Large MUSE Mosaic: Extending the Mass Model of Frontier Field Abell 370
• Unbiased Hubble constant estimation from binary neutron star mergers
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• Distances from Surface Brightness Fluctuations
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses V. The time delay in SDSS J1650+4251
• Data Mining for Gravitationally Lensed Quasars
• Voids in Real Space and in Redshift Space
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Model-independent constraints on the cosmic opacity
• Void Lensing as a Test of Gravity
• Connecting early and late epochs by f(z)CDM cosmography
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• Redshift-space distortions with split densities
• Absolute Ages and Distances of 22 GCs using Monte Carlo Main-Sequence Fitting
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses XIV. Time delay of the doubly lensed quasar SDSS J1001+5027
• SHARP - III: First Use Of Adaptive Optics Imaging To Constrain Cosmology With Gravitational Lens Time Delays
• Comparing Foreground Removal Techniques for Recovery of the LOFAR-EoR 21cm Power Spectrum
• SDSSJ2222+2745 A Gravitationally Lensed Sextuple Quasar with Maximum Image Separation of 15.1" Discovered in the Sloan Giant Arcs Survey
• Stellar Metallicities and Elemental Abundance Ratios of z~1.4 Massive Quiescent Galaxies
• Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers
• What Are the Progenitors of Compact, Massive, Quiescent Galaxies at z=2.3? The Population of Massive Galaxies at z>3 from NMBS and CANDELS
• A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403
• Cosmic voids in modified gravity scenarios
• The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties
• Determining the HI content of galaxies via intensity mapping cross-correlations
• H0LiCOW VIII. A weak lensing measurement of the external convergence in the field of the lensed quasar HE0435$-$1223
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Multiple-Images in the Cluster Lens Abell 2218: Constraining the Geometry of the Universe ?
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• Impact of Foregrounds on HI Intensity Mapping Cross-Correlations with Optical Surveys
• Measuring the growth rate of structure with Type IA Supernovae from LSST
• Topology and Dark Energy: Testing Gravity in Voids
• A universal scaling for short and long gamma-ray bursts: E_{X,iso}-E_{gamma,iso}-E_{pk}
• Reconciliation of the Surface Brightness Fluctuations and Type Ia Supernovae Distance Scales
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• Massive and old quiescent galaxies at high redshift
• The Tianlai Dish Pathfinder Array: design, operation and performance of a prototype transit radio interferometer
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Toward a Direct Measurement of the Cosmic Acceleration
• SRG/eROSITA uncovers the most X-ray luminous quasar at z>6
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• The resilience of the Etherington-Hubble relation
• Dissection of the collisional and collisionless mass components in a mini sample of CLASH and HFF massive galaxy clusters at $z\approx 0.4$
• The halo-model description of marked statistics
• A hierarchy of voids: More ado about nothing
• TDCOSMO II: 6 new time delays in lensed quasars from high-cadence monitoring at the MPIA 2.2m telescope
• The ACS Survey of Galactic Globular Clusters XIV: Bayesian Single-Population Analysis of 69 Globular Clusters
• On the Choice of Lens Density Profile in Time Delay Cosmography
• The Age of the Universe with Globular Clusters: Reducing Systematic Uncertainties
• Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
• Calibrating CHIME, A New Radio Interferometer to Probe Dark Energy
• Fermi/GBM and BATSE Gamma-Ray Bursts: comparison of the spectral properties
• Tracing dark energy history with gamma ray bursts
• Dark Energy Survey Year 1 results: The relationship between mass and light around cosmic voids
• Cluster-Void Degeneracy Breaking: Dark Energy, Planck and the Largest Cluster & Void
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
• Line-of-sight effects in strong lensing: Putting theory into practice
• Hubble diagram at higher redshifts: Model independent calibration of quasars
• Joint Analysis of near-infrared properties and surface brightness fluctuations of LMC star clusters
• Real-space density profile reconstruction of stacked voids
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• On the relative bias of void tracers in the Dark Energy Survey
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Cosmography by orthogonalized logarithmic polynomials
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• A First Comparison of the SBF Survey Distances with the Galaxy Density Field: Implications for H_0 and Omega
• The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes
• MACS J0416.1-2403: Impact of line-of-sight structures on strong gravitational lensing modelling of galaxy clusters
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• Assessment of the cosmic distance duality relation using Gaussian Process
• Benchmark ages for the Gaia benchmark stars
• Lensing convergence and the neutrino mass scale in galaxy redshift surveys
• Real-time cosmography with redshift derivatives
• Standard-siren cosmology using gravitational waves from binary black holes
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• Cosmology with Standard Sirens at Cosmic Noon
• Null test for interactions in the dark sector
• Cosmological Information in the Marked Power Spectrum of the Galaxy Field
• Line-of-sight effects in strong gravitational lensing
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Testing cosmic geometry without dynamic distortions using voids
• Cosmological test using the Hubble diagram of high-z quasars
• Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• A Two-Year Time Delay for the Lensed Quasar SDSS J1029+2623
• The final SDSS-IV/SPIDERS X-ray point source spectroscopic catalogue
• Measuring distances to low-luminosity galaxies using surface brightness fluctuations
• Cosmology with gravitationally lensed repeating Fast Radio Bursts
• Cosmological constraints from a joint analysis of cosmic growth and expansion
• The distance to Hydra and Centaurus from surface brightness fluctuations: Consequences for the Great Attractor model
• Clues on void evolution III: Structure and dynamics in void shells
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• A Study of Massive and Evolved Galaxies at High Redshift
• New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasets
• Method for Direct Measurement of Cosmic Acceleration by 21-cm Absorption Systems
• Measuring the Hubble constant with black sirens
• The Tianlai Cylinder Pathfinder Array: System Functions and Basic Performance Analysis
• Dark matter voids in the SDSS galaxy survey
• What does the Marked Power Spectrum Measure? Insights from Perturbation Theory
• Constraints on the growth of structure around cosmic voids in eBOSS DR14
• Spectral classification and composites of galaxies in LAMOST DR4
• Shot noise and biased tracers: a new look at the halo model
• The life and death of cosmic voids
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Gaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply-Imaged Lensed Quasars
• Searching for signals of inhomogeneity using multiple probes of the cosmic expansion rate H(z)
• The view from the boundary: a new void stacking method
• Radial density profiles of time-delay lensing galaxies
• HI intensity mapping with MeerKAT: 1/f noise analysis
• Simulated multi-tracer analyses with HI intensity mapping
• Cluster-void degeneracy breaking: Neutrino properties and dark energy
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Cosmological inference from standard sirens without redshift measurements
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Transverse Velocities with the Moving Lens Effect
• Over-constrained Models of Time Delay Lenses Redux: How the Angular Tail Wags the Radial Dog
• The three-parameter correlations about optical plateaus of gamma-ray bursts
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• Prospects for clustering and lensing measurements with forthcoming intensity mapping and optical surveys
• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics
• Cosmological test of gravity using weak lensing voids
• H0LiCOW X: Spectroscopic/imaging survey and galaxy-group identification around the strong gravitational lens system WFI2033-4723
• The Chandra view of the relation between X-ray and UV emission in quasars
• Giving Cosmic Redshift Drift a Whirl
• Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• Cosmic Growth and Expansion Conjoined
• Constraint of Void Bias on Primordial non-Gaussianity
• Robust Strong Lensing Time Delay Estimation
• Statistical study of gamma-ray bursts with jet break feature in multi-wavelength afterglow emissions
• Probing the primordial Universe with MeerKAT and DES
• DIVE in the cosmic web: voids with Delaunay Triangulation from discrete matter tracer distributions
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
• Measurement of the thermal Sunyaev-Zel'dovich effect around cosmic voids
• Broad band time-resolved E_{p,i}--L_{iso} correlation in GRBs
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Testing the imprint of non-standard cosmologies on void profiles using Monte Carlo random walks
• Deepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South survey
• A Detection of $z$~2.3 Cosmic Voids from 3D Lyman-$\alpha$ Forest Tomography in the COSMOS Field
• Redshift-space effects in voids and their impact on cosmological tests. Part II: the void-galaxy cross-correlation function
• Near term measurements with 21 cm intensity mapping: neutral hydrogen fraction and BAO at z<2
• The full Fisher matrix for galaxy surveys
• HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
• Voids in cosmological simulations over cosmic time
• Cosmological exploitation of cosmic void statistics - New numerical tools in the CosmoBolognaLib to extract cosmological constraints from the void size function
• Optical Surface Brightness Fluctuations of shell galaxies towards 100 Mpc
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Ambiguities in gravitational lens models: the density field from the source position transformation
• Forecasts of redshift drift constraints on cosmological parameters
• Gravitational lensing formalism in a curved arc basis: A continuous description of observables and degeneracies from the weak to the strong lensing regime
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the $\Lambda$CDM model
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• Influence of the Bounds of the Hyperparameters on the Reconstruction of Hubble Constant with Gaussian Process
• Cosmography with cluster strong lensing
• Cosmological test with the QSO Hubble diagram
• The degeneracy between primordial non-Gaussianity and foregrounds in 21cm intensity mapping experiments
• Mass profile decomposition of the Frontier Fields cluster MACS J0416-02403. Insights on the Dark-Matter inner profile
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Measuring the growth of structure with intensity mapping surveys
• Voids in Lyα Forest Tomographic Maps
• Cosmic voids uncovered -- first-order statistics of depressions in the biased density field
• The MASSIVE Survey -- XV. A Stellar Dynamical Mass Measurement of the Supermassive Black Hole in Massive Elliptical Galaxy NGC 1453
• Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
• Joining X-ray to lensing: an accurate combined analysis of MACS J0416.1$-$2403
• Quasars as high-redshift standard candles
• The search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
• Potential Impact of Global Navigation Satellite Services on Total Power HI Intensity Mapping Surveys
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• The sparkling Universe: the coherent motions of cosmic voids
• The VIMOS Public Extragalactic Redshift Survey - Searching for Cosmic Voids
• Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data
• VLT/MUSE observations of SDSS J1029+2623: towards a high-precision strong lensing model
• A Quasar Catalog with Simultaneous UV, Optical and X-ray Observations by Swift
• Time Delay Measurements for the Cluster-lensed Sextuple Quasar SDSS J2222+2745
• The ages and distances of globular clusters with the luminosity function method: the case of M5 and M55
• A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: The Group Catalog
• Non-fiducial cosmological test from geometrical and dynamical distortions around voids
• Possible identification of massive and evolved galaxies At z > 5
• First measurement of ${\sigma }_8$ using supernova magnitudes only
• Power spectrum modelling of galaxy and radio intensity maps including observational effects
• Gravitational Lens Recovery with GLASS: Measuring the mass profile and shape of a lens
• The void halo mass function: a promising probe of neutrino mass
• Redshift drift as a model independent probe of dark energy
• The ACCELERATION programme: I. Cosmology with the redshift drift
• Multipole expansion for HI intensity mapping experiments: simulations and modelling
• Void profile from Planck lensing potential map
• Improving sampling and calibration of GRBs as distance indicators
• A successful search for intervening 21 cm HI absorption in galaxies at 0.4 < z <1.0 with the Australian Square Kilometre Array Pathfinder (ASKAP)
• The Halo Void (Dust) Model of Large Scale Structure
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Are long gamma-ray bursts standard candles?
• HIDE & SEEK: End-to-End Packages to Simulate and Process Radio Survey Data
• Concordance Cosmology?
• The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): the Evolution of Dusty and Non-Dusty Galaxies with Stellar Mass at z=2-6
• H0LiCOW XI. A weak lensing measurement of the external convergence in the field of the lensed quasar B1608+656 using HST and Subaru deep imaging
• Turning noise into signal: learning from the scatter in the Hubble diagram
• The HI intensity mapping bispectrum including observational effects
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• Weak lensing with 21cm intensity mapping at $z\sim 2-3$
• Detection of Surface Brightness Fluctuations in Elliptical Galaxies imaged with the Advanced Camera for Surveys. B- and I-band measurements
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• How to Build a Catalogue of Linearly-Evolving Cosmic Voids
• Cluster-Void Degeneracy Breaking: Modified Gravity in the Balance
• STRIDES: Spectroscopic and photometric characterization of the environment and effects of mass along the line of sight to the gravitational lenses DES J0408-5354 and WGD 2038-4008
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• Impact of astrophysics on cosmology forecasts for 21 cm surveys
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• Improving Fisher matrix forecasts for galaxy surveys: window function, bin cross-correlation, and bin redshift uncertainty
• General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
• Age, metallicity and star formation history of spheroidal galaxies in cluster at z~1.2
• Measuring the Hubble function with standard candle clustering
• Pulse-wise Amati correlation in Fermi GRBs
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Matched filtering with interferometric 21cm experiments
• Cosmological impact of redshift drift measurements
• Beyond $\Lambda$CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
• Constraining the growth rate by combining multiple future surveys
• Toward a direct measurement of the cosmic acceleration: roadmap and forecast on FAST
• The effects of velocities and lensing on moments of the Hubble diagram
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Constraining coupled quintessence with the 21cm signal
• Measuring weak lensing correlations of Type Ia Supernovae
• Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
• A Method to Measure the Mass of Damped Ly-alpha Absorber Host Galaxies Using Fluctuations in 21cm Emission
• Identification of Cosmic Voids as Massive Cluster Counterparts
• On surface brightness fluctuations: probabilistic and statistical bases I: Stellar population and theoretical SBF
• ADEMIS: A Library of Evolutionary Models for Emission-Line Galaxies: I- Dustfree Models
• The Void Galaxy Survey
• A Quasar microlensing event towards J1249+3449?
• The 6x2pt method: supernova velocities meet multiple tracers
• Gamma-ray burst cosmology: Hubble diagram and star formation history
• Volume Statistics as a Probe of Large-Scale Structure
• Intensity mapping of the 21cm emission: lensing
• The sparkling Universe: a scenario for cosmic void motions
• Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423
• On the amount of peculiar velocity field information in supernovae from LSST and beyond
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Gravitational lenses in arbitrary space-times
• Extragalactic HI 21-cm absorption line observations with the Five-hundred-meter Aperture Spherical radio Telescope
• The sparkling Universe: Clustering of voids and void clumps
• A methodology to select galaxies just after the quenching of star formation
• VLT Optical BVR observations of two bright Supernova Ia hosts in the Virgo cluster
• The age of extremely red and massive galaxies at very high redshift
• Constraining properties of neutron star merger outflows with radio observations
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• The ages of (the oldest) stars
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• How do galaxy properties affect void statistics?
• Voids and Superstructures: correlations and induced large-scale velocity flows
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• On the cosmological performance of photometrically classified supernovae with machine learning
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• Effect of GRB spectra on the empirical luminosity correlations and the GRB Hubble diagram
• The failure of testing for cosmic opacity via the distance-duality relation
• False outliers of the Ep,i - Eiso correlation?
• The large-scale environment of thermonuclear and core-collapse supernovae
• Weak Lensing of Type Ia Supernovae from the Dark Energy Survey
• Ages of globular clusters: breaking the age-distance degeneracy with the luminosity function
• The non-linear X-ray/UV relation in active galactic nuclei: contribution of instrumental effects on the X-ray variability
• The Alcock Paczynski test with 21cm intensity field
• Consistent use of Type Ia supernovae highly magnified by galaxy clusters to constrain the cosmological parameters
• Variability in Quasar Light Curves: using quasars as standard candles
• Climbing out of the shadows: building the distance ladder with black hole images
• Cluster Strong Lensing with Hierarchical Inference
• Surface Brightness Fluctuations: A Case for Extremely Large Telescopes

Cited by in corpus (1)

• Multi-messenger Gravitational Lensing