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.

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

References in corpus (333)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Gaia mission
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Advanced LIGO
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• In the Realm of the Hubble tension $-$ a Review of Solutions
• The James Webb Space Telescope
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
• Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
• Some Aspects of Measurement Error in Linear Regression of Astronomical Data
• A gravitational-wave standard siren measurement of the Hubble constant
• COSMOS Photometric Redshifts with 30-bands for 2-deg2
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• Dark Energy after GW170817: dead ends and the road ahead
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• The Physics of Gamma-Ray Bursts and Relativistic Jets
• Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
• Strong constraints on cosmological gravity from GW170817 and GRB 170817A
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
• The trouble with $H_0$
• A distance to the Large Magellanic Cloud that is precise to one per cent
• Calculating black hole shadows: Review of analytical studies
• A Bayesian approach to strong lensing modelling of galaxy clusters
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• UV-extended E-MILES stellar population models: young components in massive early-type galaxies
• H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: $H_0$ to 3.8% precision from strong lensing in a flat $\Lambda$CDM model
• The Atlas3D Project - XXX. Star formation histories and stellar population scaling relations of early-type galaxies
• The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• On the Hubble constant tension in the SNe Ia Pantheon sample
• The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
• Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
• Evolutionary stellar population synthesis with MILES - II. Scaled-solar and α-enhanced models
• ZOBOV: a parameter-free void-finding algorithm
• Extended Gravity Cosmography
• Measuring primordial non-gaussianity without cosmic variance
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
• Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
• Late-time cosmology with 21cm intensity mapping experiments
• Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
• 4MOST: Project overview and information for the First Call for Proposals
• Space Telescope and Optical Reverberation Mapping Project. II. Swift and HST Reverberation Mapping of the Accretion Disk of NGC 5548
• The third realization of the International Celestial Reference Frame by very long baseline interferometry
• Weighing the Giants IV: Cosmology and Neutrino Mass
• Post-correlation radio frequency interference classification methods
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• How accurately can 21 cm tomography constrain cosmology?
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• To H0 or not to H0?
• The first ultraviolet quasar stacked spectrum at z=2.4 from WFC3
• Recovering galaxy star formation and metallicity histories from spectra using VESPA
• Cosmic dynamics in the era of Extremely Large Telescopes
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• A time - luminosity correlation for Gamma Ray Bursts in the X - rays
• Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7
• Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
• Multi-scale cluster lens mass mapping I. Strong Lensing modelling
• On the galaxy stellar mass function, the mass-metallicity relation, and the implied baryonic mass function
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
• The Aspen--Amsterdam Void Finder Comparison Project
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• Where are LIGO's Big Black Holes?
• Firefly (Fitting IteRativEly For Likelihood analYsis): a full spectral fitting code
• Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• Charting the evolution of the ages and metallicities of massive galaxies since z=0.7
• CLASH-VLT: Insights on the mass substructures in the Frontier Fields Cluster MACS J0416.1-2403 through accurate strong lens modeling
• Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
• A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
• A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
• The evolution of star formation histories of quiescent galaxies
• Quasars as standard candles III. Validation of a new sample for cosmological studies
• The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
• HIRAX: A Probe of Dark Energy and Radio Transients
• The Neutral Hydrogen Cosmological Mass Density at z=5
• Running Hubble Tension and a H0 Diagnostic
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• Testing General Relativity with 21 cm intensity mapping
• The Sloan Digital Sky Survey Quasar Lens Search. I. Candidate Selection Algorithm
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• The darkness that shaped the void: dark energy and cosmic voids
• A Comprehensive Analysis of Fermi Gamma-ray Burst Data: II. $E_{\mathrm{p}}$-Evolution Patterns and Implications for the Observed Spectrum-Luminosity Relations
• Observational constraints on cosmological solutions of $f(Q)$ theories
• Blind foreground subtraction for intensity mapping experiments
• The Assembly Histories of Quiescent Galaxies Since z=0.7 from Absorption Line Spectroscopy
• 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
• Characterization of systematic error in Advanced LIGO calibration
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• A measurement of the Hubble constant from Type II supernovae
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• KiDS-1000 Cosmology: constraints beyond flat $\Lambda$CDM
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• The Scale of the Problem : Recovering Images of Reionization with GMCA
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• The Properties of Galaxies in Voids
• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
• The Epeak-Eiso plane of long Gamma Ray Bursts and selection effects
• Gamma-ray Burst Cosmology
• Discovery of a tight correlation among the prompt emission properties of long Gamma Ray Bursts
• A Population of Massive and Evolved Galaxies at z$\ga$5
• Using H(z) data as a probe of the concordance model
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• Simulating nonlinear cosmological structure formation with massive neutrinos
• 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
• H0LiCOW III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435-1223 through weighted galaxy counts
• COSMOGRAIL XVI: Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry
• A New Survey for Giant Arcs
• 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
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• 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 MIXR sample: AGN activity versus star formation across the cross-correlation of WISE, 3XMM, and FIRST/NVSS
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• A measurement of the Alcock-Paczynski effect using cosmic voids in the SDSS
• Gamma-Ray Bursts in $1.8<z<5.6$ Suggest that the Time Variation of the Dark Energy is Small
• A marked correlation function for constraining modified gravity models
• Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• SuperRAENN: A Semi-supervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium Deep Survey Supernovae
• Over-constrained Gravitational Lens Models and the Hubble Constant
• Fast Radio Bursts and cosmological tests
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• Precision cosmology with voids in the final BOSS data
• Large-Scale Clustering of Cosmic Voids
• 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
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• When are LIGO/Virgo's Big Black-Hole Mergers?
• HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations
• Mass distribution in the core of MACS J1206: robust modeling from an exceptionally large sample of central multiple images
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• MultiDark-Galaxies: data release and first results
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• 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
• Modeling the neutral hydrogen distribution in the post-reionization Universe: intensity mapping
• Cosmic voids in modified gravity models with massive neutrinos
• Fast simulations for intensity mapping experiments
• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• The GIGANTES dataset: precision cosmology from voids in the machine learning era
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• Jumping the gap: searching for LIGO's biggest black holes
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• The star formation activity in cosmic voids
• The trouble beyond $H_0$ and the new cosmic triangles
• The local and distant Universe: stellar ages and $H_0$
• 21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• The Optical Luminosity-Time Correlation for More Than 100 Gamma-Ray Burst Afterglows
• We do not live in the R_h = c t universe
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• The Redshift Space Momentum Power Spectrum II: measuring the growth rate from the combined 2MTF and 6dFGSv surveys
• Standardized long gamma-ray bursts as a cosmic distance indicator
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Soundness of Dark Energy properties
• Quasar standardization: Overcoming Selection Biases and Redshift Evolution
• A Pixelated Approach to Galaxy Catalogue Incompleteness: Improving the Dark Siren Measurement of the Hubble Constant
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• The lensing and temperature imprints of voids on the Cosmic Microwave Background
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts
• The most luminous blue quasars at $3.0<z<3.3$. I. A tale of two X-ray populations
• A new cosmological distance measure using AGN X-ray variability
• Recovery of 21 cm intensity maps with sparse component separation
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• Gravitational lensing model degeneracies: Is steepness all-important?
• 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
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses V. The time delay in SDSS J1650+4251
• Data Mining for Gravitationally Lensed Quasars
• Redshift-space distortions with split densities
• Connecting early and late epochs by f(z)CDM cosmography
• Comparing Foreground Removal Techniques for Recovery of the LOFAR-EoR 21cm Power Spectrum
• A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403
• The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• Measuring the growth rate of structure with Type IA Supernovae from LSST
• Impact of Foregrounds on HI Intensity Mapping Cross-Correlations with Optical Surveys
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• Massive and old quiescent galaxies at high redshift
• Properties of simulated galaxies and supermassive black holes in cosmic voids
• 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
• SRG/eROSITA uncovers the most X-ray luminous quasar at z>6
• The resilience of the Etherington-Hubble relation
• 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
• Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
• The Age of the Universe with Globular Clusters: Reducing Systematic Uncertainties
• Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS
• Tracing dark energy history with gamma ray bursts
• Hubble diagram at higher redshifts: Model independent calibration of quasars
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Cosmography by orthogonalized logarithmic polynomials
• Joint Analysis of near-infrared properties and surface brightness fluctuations of LMC star clusters
• Assessment of the cosmic distance duality relation using Gaussian Process
• The Accuracy of the Hubble Constant Measurement Verified through Cepheid Amplitudes
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Cosmological Information in the Marked Power Spectrum of the Galaxy Field
• Testing cosmic geometry without dynamic distortions using voids
• Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• Line-of-sight effects in strong gravitational lensing
• Cosmology with Standard Sirens at Cosmic Noon
• A Two-Year Time Delay for the Lensed Quasar SDSS J1029+2623
• A Study of Massive and Evolved Galaxies at High Redshift
• Clues on void evolution III: Structure and dynamics in void shells
• Measuring the Hubble constant with black sirens
• What does the Marked Power Spectrum Measure? Insights from Perturbation Theory
• The Tianlai Cylinder Pathfinder Array: System Functions and Basic Performance Analysis
• Dark matter voids in the SDSS galaxy survey
• Gaia GraL: Gaia DR2 Gravitational Lens Systems. VI. Spectroscopic Confirmation and Modeling of Quadruply-Imaged Lensed Quasars
• Shot noise and biased tracers: a new look at the halo model
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Searching for signals of inhomogeneity using multiple probes of the cosmic expansion rate H(z)
• Spectral classification and composites of galaxies in LAMOST DR4
• The life and death of cosmic voids
• Radial density profiles of time-delay lensing galaxies
• HI intensity mapping with MeerKAT: 1/f noise analysis
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• The Chandra view of the relation between X-ray and UV emission in quasars
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Probing the primordial Universe with MeerKAT and DES
• Statistical study of gamma-ray bursts with jet break feature in multi-wavelength afterglow emissions
• Cosmic Growth and Expansion Conjoined
• 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
• 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 test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
• HOLISMOKES -- III. Achromatic Phase of Strongly Lensed Type Ia Supernovae
• Redshift-space effects in voids and their impact on cosmological tests. Part II: the void-galaxy cross-correlation function
• Gravitational lensing formalism in a curved arc basis: A continuous description of observables and degeneracies from the weak to the strong lensing regime
• Forecasts of redshift drift constraints on cosmological parameters
• Optical Surface Brightness Fluctuations of shell galaxies towards 100 Mpc
• Influence of the Bounds of the Hyperparameters on the Reconstruction of Hubble Constant with Gaussian Process
• The Impact of Observing Strategy on Cosmological Constraints with LSST
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• 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
• Measuring the growth of structure with intensity mapping surveys
• The MASSIVE Survey -- XV. A Stellar Dynamical Mass Measurement of the Supermassive Black Hole in Massive Elliptical Galaxy NGC 1453
• The search for galaxy cluster members with deep learning of panchromatic HST imaging and extensive spectroscopy
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• Quasars as high-redshift standard candles
• VLT/MUSE observations of SDSS J1029+2623: towards a high-precision strong lensing model
• The VIMOS Public Extragalactic Redshift Survey - Searching for Cosmic Voids
• Observational constraints on Starobinsky $f(R)$ cosmology from cosmic expansion and structure growth data
• 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
• Void profile from Planck lensing potential map
• Redshift drift as a model independent probe of dark energy
• The ACCELERATION programme: I. Cosmology with the redshift drift
• 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)
• HIDE & SEEK: End-to-End Packages to Simulate and Process Radio Survey Data
• 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
• Detection of Surface Brightness Fluctuations in Elliptical Galaxies imaged with the Advanced Camera for Surveys. B- and I-band measurements
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
• The HI intensity mapping bispectrum including observational effects
• How to Build a Catalogue of Linearly-Evolving Cosmic Voids
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• Extracting HI Astrophysics from Interferometric Intensity Mapping
• The PDF perspective on the tracer-matter connection: Lagrangian bias and non-Poissonian shot noise
• Age, metallicity and star formation history of spheroidal galaxies in cluster at z~1.2
• Constraining the growth rate by combining multiple future surveys
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• Cosmological impact of redshift drift measurements
• The effects of velocities and lensing on moments of the Hubble diagram
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Constraining the anisotropy of the Universe with the X-ray and UV fluxes of quasars
• Measuring weak lensing correlations of Type Ia Supernovae
• Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
• Identification of Cosmic Voids as Massive Cluster Counterparts
• On surface brightness fluctuations: probabilistic and statistical bases I: Stellar population and theoretical SBF
• A Quasar microlensing event towards J1249+3449?
• The 6x2pt method: supernova velocities meet multiple tracers
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Volume Statistics as a Probe of Large-Scale Structure
• Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423
• Gamma-ray burst cosmology: Hubble diagram and star formation history
• Gravitational lenses in arbitrary space-times
• Extragalactic HI 21-cm absorption line observations with the Five-hundred-meter Aperture Spherical radio Telescope
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• Voids and Superstructures: correlations and induced large-scale velocity flows
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• How do galaxy properties affect void statistics?
• False outliers of the Ep,i - Eiso correlation?
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• The failure of testing for cosmic opacity via the distance-duality relation
• Weak Lensing of Type Ia Supernovae from the Dark Energy Survey
• The large-scale environment of thermonuclear and core-collapse supernovae
• 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

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