The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set

Abstract

We present distance measurements to 71 high redshift type Ia supernovae discovered during the first year of the 5-year Supernova Legacy Survey (SNLS). These events were detected and their multi-color light-curves measured using the MegaPrime/MegaCam instrument at the Canada-France-Hawaii Telescope (CFHT), by repeatedly imaging four one-square degree fields in four bands. Follow-up spectroscopy was performed at the VLT, Gemini and Keck telescopes to confirm the nature of the supernovae and to measure their redshift. With this data set, we have built a Hubble diagram extending to z=1, with all distance measurements involving at least two bands. Systematic uncertainties are evaluated making use of the multi-band photometry obtained at CFHT. Cosmological fits to this first year SNLS Hubble diagram give the following results : Omega_M = 0.263 +/- 0.042(stat) +/- 0.032(sys) for a flat LambdaCDM model; and w = -1.023 +/- 0.090(stat) +/- 0.054(sys) for a flat cosmology with constant equation of state w when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.

(The SNLS Collaboration) 24 pages, 13 figures, Accepted in A&A. Computer readable tables at http://snls.in2p3.fr/conf/papers/cosmo1/

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• Neutrino Dark Energy -- Revisiting the Stability Issue
• The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release
• Measuring cosmological parameters with Gamma-Ray Bursts
• Constraints on dark energy with the LOSS SN Ia sample
• Finite-time singularities in f(R, T) gravity and the effect of conformal anomaly
• On the onset of cosmological backreaction
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Dynamic vacuum variable and equilibrium approach in cosmology
• Testing Screened Modified Gravity
• The phenomenological approach to modeling the dark energy
• Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• The Ages of Type Ia Supernova Progenitors
• Anisotropic Universe Models with Perfect Fluid and Scalar Field in f(R,T) Gravity
• SNLS Spectroscopy: Testing for Evolution in Type Ia Supernovae
• Supernova limits on brane world cosmology
• Thermal history of the plasma and high-frequency gravitons
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• If Gauss-Bonnet interaction plays the role of dark energy
• Dark Energy Constraints from Galaxy Cluster Peculiar Velocities
• Weak lensing survey of galaxy clusters in the CFHTLS Deep
• Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters
• Some aspects of generalized modified gravity models
• The Art of Lattice and Gravity Waves from Preheating
• Constraining dark matter halo properties using lensed SNLS supernovae
• The growth of matter perturbations in some scalar-tensor DE models
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Evolution in the Volumetric Type Ia Supernova Rate from the Supernova Legacy Survey
• Estimation of cosmological parameters using adaptive importance sampling
• OzDES multi-object fibre spectroscopy for the Dark Energy Survey: Results and second data release
• The LSST DESC DC2 Simulated Sky Survey
• Supernovae in the Subaru Deep Field: An Initial Sample, and Type Ia Rate, out to Redshift 1.6
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• The Abell Cluster A586 and the Detection of the Equivalence Principle
• Dynamics in Nonlocal Cosmological Models Derived from String Field Theory
• Cosmic Acceleration, Dark Energy and Fundamental Physics
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Carbon Detection in Early-Time Optical Spectra of Type Ia Supernovae
• Reconstruction of cosmic history from a simple parametrization of H
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Properties of the ultraviolet flux of type Ia supernovae: an analysis with synthetic spectra of SN 2001ep and SN 2001eh
• Bayesian Estimation Applied to Multiple Species: Towards cosmology with a million supernovae
• The Effect of Environment on Type Ia Supernovae in the Dark Energy Survey Three-Year Cosmological Sample
• Dynamics of f(R)-cosmologies containing Einstein static models
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Type II-P Supernovae from the SDSS-II Supernova Survey and the Standardized Candle Method
• Scaling relations and mass calibration of the X-ray luminous galaxy clusters at z~0.2: XMM-Newton observations
• Observational Evidence of the Accelerated Expansion of the Universe
• Reconstruction of the Scalar-Tensor Lagrangian from a LCDM Background and Noether Symmetry
• On using the CMB shift parameter in tests of models of dark energy
• Constraints on f(R) Cosmology in the Palatini Formalism
• Evaluating backreaction with the peak model of structure formation
• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• How flat can you get? A model comparison perspective on the curvature of the Universe
• Testing GRBs as Standard Candles
• Dark energy equation of state parameter and its variation at low redshifts
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• Evidence for short-lived SN Ia progenitors
• A Hierarchical Bayesian SED Model for Type Ia Supernovae in the Optical to Near-Infrared
• Phantom Dark Energy Models with a Nearly Flat Potential
• Curvature singularities, tidal forces and the viability of Palatini f(R) gravity
• The Luminosity Function of the Hot and Cold Kuiper belt Populations
• CfAIR2: Near Infrared Light Curves of 94 Type Ia Supernovae
• Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
• Determination of the Hubble constant, the intrinsic scatter of luminosities of Type Ia SNe, and evidence for non-standard dust in other galaxies
• Constraining Type Ia Supernovae progenitors from three years of SNLS data
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• On the curvature of the present-day Universe
• Searching for a Companion Star of Tycho's Type Ia Supernova with Optical Spectroscopic Observations
• A new null diagnostic customized for reconstructing the properties of dark energy from BAO data
• Bayesian optimisation for likelihood-free cosmological inference
• Gaussian Process Estimation of Transition Redshift
• Fermion Masses and Flavor Mixings in a Model with $S_4$ Flavor Symmetry
• Thermodynamics in $f(R)$ gravity in the Palatini formalism
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• The past and future dynamics of quintom dark energy models
• Cosmological dynamics with non-linear interactions
• How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Measurement of Ω_m, Ω_Λ from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe
• Analysis of the Yukawa gravitational potential in $f(R)$ gravity II: relativistic periastron advance
• Falsifying Paradigms for Cosmic Acceleration
• A 5% measurement of the Hubble constant from Type II supernovae
• SPACE: the SPectroscopic All-sky Cosmic Explorer
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• A unified explanation for the supernova rate-galaxy mass dependency based on supernovae discovered in Sloan galaxy spectra
• Axion isocurvature fluctuations with extremely blue spectrum
• Magnetized CMB observables: a dedicated numerical approach
• Do spectra improve distance measurements of Type Ia supernovae?
• Growth Index of DGP Model and Current Growth Rate Data
• Nonlinear growth in modified gravity theories of dark energy
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101
• An improved cosmological bound on the thermal axion mass
• Constraining $f(R)$ gravity by the Large Scale Structure
• Probing the Cosmic Distance Duality Relation with the Sunyaev-Zeldovich Effect, X-rays Observations and Supernovae Ia
• Large Einstein Radii: A Problem for LambdaCDM
• Anisotropic Fluid and Bianchi Type III Model in f(R) Gravity
• An Intensive HST Survey for z>1 Supernovae by Targeting Galaxy Clusters
• De Sitter Universe in Nonlocal Gravity
• The interior spacetimes of stars in Palatini f(R) gravity
• Interacting holographic dark energy with logarithmic correction
• ESC observations of SN 2005cf: II. Optical Spectroscopy and the high velocity features
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• How to Find More Supernovae with Less Work: Object Classification Techniques for Difference Imaging
• Analytical Approach to Subhaloes Population in Dark Matter Haloes
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Constraining the range of Yukawa gravity interaction from S2 star orbits II: Bounds on graviton mass
• New agegraphic dark energy model with generalized uncertainty principle
• A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
• The Type Ia Supernova Color-Magnitude Relation and Host Galaxy Dust: A Simple Hierarchical Bayesian Model
• The reliability of the AIC method in Cosmological Model Selection
• Energy conditions and current acceleration of the universe
• Constraining Cosmic Evolution of Type Ia Supernovae
• The Rate of Supernovae at Redshift 0.1-1.0 - the Stockholm VIMOS Supernova Survey IV
• Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
• On the progenitors of super-Chandrasekhar mass type Ia supernovae
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Energy Conditions and Supernovae Observations
• Cosmic transparency: A test with the baryon acoustic feature and type Ia supernovae
• Cosmological scaling solutions in generalised Gauss-Bonnet gravity theories
• Observational constraints on late-time Lambda(t) cosmology
• Conserved Quantities in $f(R)$ Gravity via Noether Symmetry
• Kernel PCA for type Ia supernovae photometric classification
• Genetic Algorithms and Supernovae Type Ia Analysis
• BAHAMAS: new SNIa analysis reveals inconsistencies with standard cosmology
• Dark matter halo properties from galaxy-galaxy lensing
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Neutrino masses and cosmic radiation density: Combined analysis
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• The Limits of Extended Quintessence
• The Weak Energy Condition and the Expansion History of the Universe
• Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• PTF10nvg: An Outbursting Class I Protostar in the Pelican/North American Nebula
• Spectrophotometric templates for core collapse supernovae and their application in simulations of time-domain surveys
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Cosmology of neutrinos and extra light particles after WMAP3
• Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data
• Quintessence reconstructed: new constraints and tracker viability
• Redshift evolution of the underlying type Ia supernova stretch distribution
• Phenomenology of dark energy: exploring the space of theories with future redshift surveys
• Off-center explosions of Chandrasekhar-mass white dwarfs: an explanation of super-bright type Ia supernovae?
• Kinetic k-essence ghost dark energy model
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Model selection as a science driver for dark energy surveys
• Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study
• Radiation-hydrodynamical modelling of Core-Collapse Supernovae: light curves and the evolution of photospheric velocity and temperature
• The Fundamental Metallicity Relation Reduces Type Ia SN Hubble Residuals More Than Host Mass Alone
• The Standardizability of Type Ia Supernovae in the Near-Infrared: Evidence for a Peak Luminosity-Decline Rate Relation in the Near-Infrared
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Faraday rotation, stochastic magnetic fields and CMB maps
• The Impact of Cosmic Dust on Supernova Cosmology
• Constraining Modified Gravity and Growth with Weak Lensing
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Gravastars in $f(\mathbb{T},\mathcal{T})$ gravity
• Evaluating Systematic Dependencies of Type Ia Supernovae: The Influence of Progenitor Ne22 Content on Dynamics
• Can Dark Matter Decay in Dark Energy?
• Constraining Lorentz violation with cosmology
• Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• A review of type Ia supernova spectra
• Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
• First-Year Spectroscopy for the SDSS-II Supernova Survey
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• 6+1 lessons from f(R) gravity
• The cosmic snap parameter in f(R) gravity
• Supernova constraints on decaying vacuum cosmology
• Reconciling the local void with the CMB
• Redshift-Independent Distances in the NASA/IPAC Extragalactic Database: Methodology, Content and Use of NED-D
• Observational constraint on generalized Chaplygin gas model
• Bayesian analysis of Friedmannless cosmologies
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Spectral modelling of the "Super-Chandra" Type Ia SN 2009dc - testing a 2 M_sun white dwarf explosion model and alternatives
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Determining the Neutrino Mass Hierarchy with Cosmology
• Berkeley Supernova Ia Program V: Late-Time Spectra of Type Ia Supernovae
• Supernova ejecta with a relativistic wind from a central compact object: a unified picture for extraordinary supernovae
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• Photometric selection of Type Ia supernovae in the Supernova Legacy Survey
• The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology
• Tight coupling expansion and fully inhomogeneous magnetic fields
• Accelerating dark energy models in bianchi Type-V space-time
• Latest supernovae constraints on f(R) cosmologies
• The imprint of the interaction between dark sectors in galaxy clusters
• On Phantom Thermodynamics
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• Cylindrical Solutions in Modified f(T) Gravity
• Stability analysis for cosmological models in $f(R)$ gravity using dynamical system analysis
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
• How clustering dark energy affects matter perturbations
• Real-time Analysis and Selection Biases in the Supernova Legacy Survey
• Cosmological consequences of a possible $\Lambda$-dark matter interaction
• Anisotropic perturbations due to dark energy
• Primordial Black Holes, Eternal Inflation, and the Inflationary Parameter Space after WMAP5
• Supernova Host Galaxies in the Dark Energy Survey: I. Deep Coadds, Photometry, and Stellar Masses
• Early massive clusters and the bouncing coupled dark energy
• Bayesian Single-Epoch Photometric Classification of Supernovae
• Stellar configurations in f(R) theories of gravity
• Cosmology with moving dark energy and the CMB quadrupole
• Star Models with Dark Energy
• Can a galaxy redshift survey measure dark energy clustering?
• Berkeley Supernova Ia Program III: Spectra Near Maximum Brightness Improve the Accuracy of Derived Distances to Type Ia Supernovae
• Exact dark energy star solutions
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Comments on scalar-tensor representation of nonlocally corrected gravity
• Cosmological constraints on neutrino plus axion hot dark matter
• The ESO/VLT 3rd year Type Ia supernova data set from the Supernova Legacy Survey
• Testing dark energy paradigms with weak gravitational lensing
• Cosmological model with interactions in the dark sector
• Learning from the Scatter in Type Ia Supernovae
• Remarks on the formulation of the cosmological constant/dark energy problems
• Dark Energy Evolution and the Curvature of the Universe from Recent Observations
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Dirac Neutrinos with $S_4$ Flavor Symmetry in Warped Extra Dimensions
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Time-Dependent Wormhole Solutions of $f(R)$ Theory of Gravity and Energy Conditions
• Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
• Extended Quintessence with non-minimally coupled phantom scalar field
• Supernova Legacy Survey: Using Spectral Signatures To Improve Type Ia Supernovae As Distance Indicators
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Accelerating cosmologies tested by distance measures
• On the Past Asymptotic Dynamics of Non-minimally Coupled Dark Energy
• DASH: Deep Learning for the Automated Spectral Classification of Supernovae and their Hosts
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• Testing the Consistency of Dust Laws in SN Ia Host Galaxies: A BayeSN Examination of Foundation DR1
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Spectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First Four Years
• Measuring deviations from a cosmological constant: a field-space parameterization
• SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features
• How to Distinguish Dark Energy and Modified Gravity?
• Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
• Voids of dark energy
• How far is it to a sudden future singularity of pressure?
• Photometric Estimates of Redshifts and Distance Moduli for Type Ia Supernovae
• Interacting Ricci Dark Energy with Logarithmic Correction
• High redshift cosmography: new results and implication for dark energy
• Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
• Determining Cosmological Parameters with Latest Observational Data
• Evolution of density perturbations in decaying vacuum cosmology
• Cheng-Weyl Vector Field and its Cosmological Application
• Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
• Bayesian Analysis and Constraints on Kinematic Models from Union SNIa
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Reconstruction of the Primordial Power Spectrum by Direct Inversion
• The XMM Cluster Survey: The Dynamical State of XMMXCS J2215.9-1738 at z=1.457
• Dissipative or Conservative cosmology with dark energy ?
• Swiss Cheese and a Cheesy CMB
• Phantom phase power-law solution in $f(G)$ gravity
• Designing Future Dark Energy Space Mission: I. Building Realistic Galaxy Spectro-Photometric Catalogs and their first applications
• Transient cosmic acceleration from interacting fluids
• The Hubble diagram extended to z>>1: the gamma-ray properties of GRBs confirm the Lambda-CDM model
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Growth factor parametrization in curved space
• Origin of holographic dark energy models
• Interacting Energy Components and Observational $H(z)$ Data
• Clustering properties of a type-selected volume-limited sample of galaxies in the CFHTLS
• Cosmological constraints combining H(z), CMB shift and SNIa observational data
• Cosmological Constraints from Galaxy Cluster Velocity Statistics
• A test of the CPL parameterization for rapid dark energy equation of state transitions
• New coupled quintessence cosmology
• Subluminous Type Ia Supernovae at High Redshift from the Supernova Legacy Survey
• Constraining dark matter properties with Cosmic Microwave Background observations
• Cosmological constraints on a light non-thermal sterile neutrino
• Yang-Mills condensate dark energy coupled with matter and radiation
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• Oscillations in the dark energy EoS: new MCMC lessons
• Dynamical Dark Energy simulations: high accuracy Power Spectra at high redshift
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Cosmological perturbations in Palatini modified gravity
• Is cosmology compatible with sterile neutrinos?
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• UV stable, Lorentz-violating dark energy with transient phantom era
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• CFHTLS weak-lensing constraints on the neutrino masses
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• $\Lambda (t)$ cosmology induced by a slowly varying Elko field
• Cosmological Constraints on Invisible Decay of Dark Matter
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• Dark energy: investigation and modeling
• Non-universal scalar-tensor theories and big bang nucleosynthesis
• The cosmic jerk parameter in f(R) gravity
• Supernovae in Low-Redshift Galaxy Clusters: Observations by the Wise Observatory Optical Transient Search (WOOTS)
• Hubble parameter reconstruction from a principal component analysis: minimizing the bias
• Classification of dark energy models in the (w_0,w_a) plane
• Photometry of supernovae in an image series : methods and application to the Supernova Legacy Survey (SNLS)
• Scalar Field Dark Energy Perturbations and their Scale Dependence
• GHOST: Using Only Host Galaxy Information to Accurately Associate and Distinguish Supernovae
• Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey
• Lightcurves of Type Ia Supernovae from Near the Time of Explosion
• Errors in Estimating Omega_Lambda due to the Fluid Approximation
• Is the evidence for dark energy secure?
• The Effect of Weak Lensing on Distance Estimates from Supernovae
• How robust are inflation model and dark matter constraints from cosmological data?
• Constraints on Galileon-induced precessions from solar system orbital motions
• The Mean Type Ia Supernova Spectrum Over the Past 9 Gigayears
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• The Multi-Epoch Nearby Cluster Survey: type Ia supernova rate measurement in z~0.1 clusters and the late-time delay time distribution
• Spectral analysis of the 91bg-like Type Ia SN 2005bl: Low luminosity, low velocities, incomplete burning
• A new approach on the stability analysis in ELKO cosmology
• Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
• Probing bulk flow with nearby SNe Ia data
• On the determination of curvature and dynamical Dark Energy
• Model independent constraints on the cosmological expansion rate
• The growth of linear perturbations in the DGP model
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Age constraints on the cosmic equation of state
• Accelerating universe in scalar tensor models - confrontation of theoretical predictions with observations
• Testing Cosmology with Cosmic Sound Waves
• Supernova Discoveries 2010-2011: Statistics and Trends
• Consequences of energy conservation violation: Late time solutions of $\Lambda (T)CDM$ subclass of $f(R,T)$ gravity using dynamical system approach
• How well will ton-scale dark matter direct detection experiments constrain minimal supersymmetry?
• Consistency tests in cosmology using relative entropy
• Near-Horizon Solution for DGP Perturbations
• The need for accurate redshifts in supernova cosmology
• Reconstruction Procedure in Nonlocal Cosmological Models
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Light curves for off-centre ignition models of type Ia supernovae
• Time drift of cosmological redshifts and its variance
• Constraints on growth index parameters from current and future observations
• The Relation Between Ejecta Velocity, Intrinsic Color, and Host-Galaxy Mass for High-Redshift Type Ia Supernovae
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• Type Ia Supernovae are Excellent Standard Candles in the Near-Infrared
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• $\text{simsurvey}$: Estimating Transient Discovery Rates for the Zwicky Transient Facility
• Phantom-Like Behavior in $f(R)$-Gravity
• Concerning Colour: The Effect of Environment on Type Ia Supernova Colour in the Dark Energy Survey
• Stable Models of superacceleration
• Parameterized Post-Newtonian Cosmology
• SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements
• Anomaly Detection in the Open Supernova Catalog
• Lensing and Supernovae: Quantifying The Bias on the Dark Energy Equation of State
• Model independent constraints on transition redshift
• Reconstruction of f(T) gravity according to holographic dark energy
• Berkeley Supernova Ia Program: Data Release of 637 Spectra from 247 Type Ia Supernovae
• The Hubble Space Telescope Cluster Supernova Survey: II. The Type Ia Supernova Rate in High-Redshift Galaxy Clusters
• Testing the DGP model with ESSENCE
• Brane assisted quintessential inflation with transient acceleration
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Cosmological dynamics of fourth order gravity: A compact view
• Estimating relic magnetic fields from CMB temperature correlations
• Tension in the Recent Type Ia Supernovae Datasets
• Testing the Distance-Duality Relation with a Combination of Cosmological Distance Observations
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae Data
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• Global and Local Effects of Rotation: Observational Aspects
• An Improved Treatment of Optics in the Lindquist-Wheeler Models
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• The Dark Energy Survey Supernova Program: Modelling selection efficiency and observed core collapse supernova contamination
• The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
• Measuring dark energy spatial inhomogeneity with supernova data
• The influence of Host Galaxies in Type Ia Supernova Cosmology
• Helium star evolutionary channel to super-Chandrasekhar mass type Ia supernovae
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• Low redshift observational constraints on tachyon models of dark energy
• A Probabilistic Approach to Classifying Supernovae Using Photometric Information
• Connecting LHC, ILC, and Quintessence
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• On Anisotropic Dark Energy
• Chemical Potential and the Nature of the Dark Energy: The case of phantom
• Single-field inflation constraints from CMB and SDSS data
• Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant
• Luminosity Functions of Type Ia Supernovae and their Host Galaxies from the Sloan Digital Sky Survey
• Dynamics in nonlocal linear models in the Friedmann-Robertson-Walker metric
• Fuzzy Supernova Templates I: Classification
• Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity
• When Did Cosmic Acceleration Start ?
• A parametrization for the growth index of linear matter perturbations
• Reconstructing the interaction rate in holographic models of dark energy
• What the small angle CMB really tells us about the curvature of the Universe
• Cosmological Perturbations in Elastic Dark Energy Models
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
• Possible extensions of the standard cosmological model: anisotropy, rotation, and magnetic field
• The Relative Specific Type Ia Supernovae Rate From Three Years of ASAS-SN
• Type Ia Supernova Colors and Ejecta Velocities: Hierarchical Bayesian Regression with Non-Gaussian Distributions
• Using a phenomenological model to test the coincidence problem of dark energy
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• The signature of dark energy perturbations in galaxy cluster surveys
• Cosmic distance duality and cosmic transparency
• Type Ia Supernovae Rates and Galaxy Clustering from the CFHT Supernova Legacy Survey
• Galaxy Zoo Supernovae
• New Constraints on Macroscopic Compact Objects as a Dark Matter Candidate from Gravitational Lensing of Type Ia Supernovae
• Perturbations of SNe Ia lightcurves, colors and spectral features by circumstellar dust
• Properties of Type II Plateau Supernova SNLS-04D2dc: Multicolor Light Curves of Shock Breakout and Plateau
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• New Parametrization for the Scale Dependent Growth Function in General Relativity
• Adjoint SUSY $SU(5)$ Grand Unified Model with $S_4$ Flavor Symmetry
• The Dark Energy Survey 5-year photometrically identified Type Ia Supernovae
• Near-IR Search for Lensed Supernovae Behind Galaxy Clusters - II. First Detection and Future Prospects
• Probing the extragalactic fast transient sky at minute timescales with DECam
• Exploring scalar field dynamics with Gaussian processes
• Can $f(T)$ gravity theories mimic $\Lambda$CDM cosmic history
• The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate
• Cosmic Behavior, Statefinder Diagnostic and $w-w^{\prime }$ Analysis for Interacting NADE model in Non-flat Universe
• Construction of Exact Solutions in Two-Fields Models and the Crossing of the Cosmological Constant Barrier
• High-redshift supernova rates measured with the gravitational telescope A1689
• Gauss-Bonnet Chameleon Mechanism of Dark Energy
• Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions
• Cosmic Core-Collapse Supernovae from Upcoming Sky Surveys
• Bouncing Universe and Reconstructing Vector Field
• Internal Robustness: systematic search for systematic bias in SN Ia data
• Probing non-standard gravity with the growth index: a background independent analysis
• Cosmic Constraint on Ricci Dark Energy Model
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Do supernovae indicate an accelerating universe?
• Hubble Space Telescope Studies of Nearby Type Ia Supernovae: The Mean Maximum Light Ultraviolet Spectrum and its Dispersion
• Cosmological dynamics of brane f(R) gravity
• Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
• Core-collapse supernovae in low-metallicity environments and future all-sky transient surveys
• $\Lambda$-CDM Universe: A Phenomenological Approach With Many Possibilities
• Supernovae as seen by off-center observers in a local void
• A See-Saw $S_4$ model for fermion masses and mixings
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• Confronting pNGB quintessence with data
• Comparison of Recent SnIa datasets
• Beyond Two Dark Energy Parameters
• The Tsinghua University-Ma Huateng Telescopes for Survey: Overview and Performance of the System
• Cosmological perturbations in SFT inspired non-local scalar field models
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• A Type II Supernova Hubble diagram from the CSP-I, SDSS-II, and SNLS surveys
• New Constraints On The Dark Energy Equation of State
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Dynamics of holographic vacuum energy in the DGP model
• Type II-P supernovae as standardised candles: improvements using near infrared data
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• Super-sample covariance approximations and partial sky coverage
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• Reconstruction of k-essence model
• Dark viscous fluid described by a unified equation of state in cosmology
• Coupled quintessence and vacuum decay
• Couplings between holographic dark energy and dark matter
• Residual Hubble-bubble effects on supernova cosmology
• Variable Radio Sources in the Galactic Plane
• Hybrid natural inflation from non Abelian discrete symmetry
• Gravitational lensing in the Supernova Legacy Survey (SNLS)
• Standardizing the GRBs with the Amati Ep,i - Eiso relation: the updated Hubble diagram and implications for cosmography
• Asymmetric Gravitational Lenses in TeVeS and Application to the Bullet Cluster
• Legacy data and cosmological constraints from the angular-size/redshift relation for ultra-compact radio sources
• Natural Phantom Dark Energy, Wiggling Hubble Parameter $H(z)$ and Direct $H(z)$ Data
• Effects of f(R) Dark Energy on Dissipative Anisotropic Collapsing Fluid
• Revisiting f(R) gravity models that reproduce $\Lambda$CDM expansion
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• A Model for Dark Energy decay
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Bright High z SnIa: A Challenge for LCDM?
• UV surface brightness of galaxies from the local Universe to z ~ 5
• The growth factor of matter perturbations in an f(R) gravity
• Study Of Tachyon Dynamics For Broad Classes of Potentials
• Observational tests for Λ(t)CDM cosmology
• How strong is the evidence for accelerated expansion?
• Dark energy, gravitation and supernovae
• Multiple kinetic k-essence, phantom barrier crossing and stability
• Bianchi Type $I$ Cosmology in $f(R,T)$ Gravity
• The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates
• The most general fourth order theory of Gravity at low energy
• EmpiriciSN: Re-sampling Observed Supernova/Host Galaxy Populations using an XD Gaussian Mixture Model
• Observational constraints on varying neutrino-mass cosmology
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Reconstruction of modified gravity with ghost dark energy models
• Clustering, Angular Size and Dark Energy
• Diversity of supernovae Ia determined using equivalent widths of Si II 4000
• Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
• Exploring Parameter Constraints on Quintessential Dark Energy: the Inverse Power Law Model
• Unified model of baryonic matter and dark components
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Anisotropic universe with anisotropic sources
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• The solution of the cosmological constant problem from the inhomogeneous equation of state - a hint from modified gravity?
• Phenomenology of $\Lambda$-CDM model: a possibility of accelerating Universe with positive pressure
• Evolution of density perturbations in decaying vacuum cosmology: The case of non-zero perturbations in the cosmological term
• Characterisation of the non-Gaussianity of radio and IR point-sources at CMB frequencies
• Supernovae data and perturbative deviation from homogeneity
• Cosmography: Extracting the Hubble series from the supernova data
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Cosmological Studies with Radio Galaxies and Supernovae
• Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in $f(R,T)$ gravity
• Semi-analytical approach to magnetized temperature autocorrelations
• Dark Energy as a Born-Infeld Gauge Interaction Violating the Equivalence Principle
• Measuring Cosmological Parameters with Type Ia Supernovae in redMaGiC galaxies
• A Geometrical Approach to Strong Gravitational Lensing in f(R) Gravity
• Brans-Dicke Scalar Field Cosmological Model in Lyra's Geometry
• The Cosmic Neutrino Background and the Age of the Universe
• The Hyper Suprime-Cam SSP Transient Survey in COSMOS: Overview
• Quantifying systematic uncertainties in supernova cosmology
• Parameter dependence of magnetized CMB observables
• Photometric redshifts for supernovae Ia in the Supernova Legacy Survey
• Magnetized Bianchi Type $V{I}_0$ Barotropic Massive String Universe with Decaying Vacuum Energy Density $\Lambda$
• Inhomogeneous viscous fluids in FRW universe and finite-future time singularities
• Cosmological Implications of the Effective Field Theory of Cosmic Acceleration
• Analysis of scalar perturbations in cosmological models with a non-local scalar field
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Shedding light on the Type Ia supernova extinction puzzle: dust location found
• Constraints on Energy Momentum Squared Gravity from cosmic chronometers and Supernovae Type Ia data
• The Subaru/XMM-Newton Deep Survey (SXDS) - V. Optically Faint Variable Object Survey
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Constraining the Schwarzschild-de Sitter Solution in Models of Modified Gravity
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Reconstructing the potentials for the quintessence and tachyon dark energy, from the holographic principle
• Signatures of clumpy dark matter in the global 21 cm background signal
• Direct evidence of acceleration from distance modulus redshift graph
• What Can Gamma Ray Bursts Teach Us About Dark Energy?
• Including Absorption in Gordon's Optical Metric
• Cosmological constant and late transient acceleration of the universe in the Horava-Witten Heterotic M-Theory on S^{1}/Z_{2}
• Two Component Model of Dark Energy
• Reconstructing the history of dark energy using maximum entropy
• Is the Dynamics of Tracking Dark Energy Detectable?
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• Color Me Intrigued: the Discovery of iPTF 16fnm, a Supernova 2002cx-like Object
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Cosmology with Ricci dark energy
• Cosmology with interaction in the dark sector
• Hybrid Natural Low Scale Inflation
• Type Ia Supernovae: Colors, Rates, and Progenitors
• Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses
• Energy conditions bounds and their confrontation with supernovae data
• Light curves of five type Ia supernovae at intermediate redshift
• Strange stars in $f(\mathcal{R})$ gravity Palatini formalism and gravitational wave echoes from them
• Tri-Bimaximal Neutrino Mixing and the $T_{13}$ Flavor Symmetry
• Galactic rotation curves and brane world models
• Steve: A hierarchical Bayesian model for Supernova Cosmology
• A $f(R)$-gravity model of the Sunyaev-Zeldovich profile of the Coma cluster compatible with {\it Planck} data
• Perturbative approach for mass varying neutrinos coupled to the dark sector in the generalized Chaplygin gas scenario
• Basics of inflationary cosmology
• First experimental constraints on the disformally coupled Galileon model
• Reconstruction of interacting dark energy models from parameterizations
• SweetSpot: Near-Infrared Observations of Thirteen Type Ia Supernovae from a New NOAO Survey Probing the Nearby Smooth Hubble Flow
• Spectroscopic and Photometric Redshift Estimation by Neural Networks For the China Space Station Optical Survey (CSS-OS)
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• The Post-Newtonian Limit of f(R)-gravity in the Harmonic Gauge
• The Crossing Statistic: Dealing with Unknown Errors in the Dispersion of Type Ia Supernovae
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• L.R.S. Bianchi type II Stiff Fluid cosmological model with Decaying Vacuum Energy Density $\Lambda$ in general relativity
• Dynamics of Chiral Cosmology
• Interacting Dark Energy in Hořava-Lifshitz Cosmology
• Statistical Classification Techniques for Photometric Supernova Typing
• Testing nonstandard cosmological models with SNLS3 supernova data and other cosmological probes
• Generalized CMB initial conditions with pre-equality magnetic fields
• Some remarks on the attractor behaviour in ELKO cosmology
• Composition of Low Redshift Halo Gas
• Exact cosmological solution of a Scalar-Tensor Gravity theory compatible with the $\Lambda CDM$ model
• Assisted dark energy
• Supernovae and Cosmology
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Sky Surveys
• WMAP5 and the Cluster Mass Function
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Coupling between cold dark matter and dark energy from neutrino mass experiments
• Dark Viscous Fluid coupled with Dark Matter and future singularity
• Moduli Fields as Quintessence and the Chameleon
• Expansion history and f(R) modified gravity
• Reconstructing a String-Inspired Non-minimally Coupled Quintom Model
• Cosmology with Photometric Surveys of Type Ia Supernovae
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Static Cylindrically Symmetric Interior Solutions in f(R) Gravity
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Mirror World and Superstring-Inspired Hidden Sector of the Universe, Dark Matter and Dark Energy
• South Galactic Cap u-band Sky Survey (SCUSS): Data Reduction
• Structure formation on the brane: A mimicry
• Black hole and holographic dark energy
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Cosmological constant dominated transit universe from early deceleration to current acceleration phase in Bianchi-V space-time
• Some FRW Models of Accelerating Universe with Dark Energy
• Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
• Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Direct Reconstruction of the Dark Energy Scalar-Field Potential
• The thermal Sunyaev-Zel'dovich Signature of Baryons in the Local Universe
• Probing the physical and mathematical structure of $f(R)$ gravity by PSR $J0348+0432$
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• Holographic Dark Energy from a Modified GBIG Scenario
• Clarifying Forecasts of Dark Energy Constraints from Baryon Acoustic Oscillations
• Quasinormal modes of black holes absorbing dark energy
• Spectral properties of Type Ia supernovae up to z~0.3
• Revised Supernova Rates from the IfA Deep Survey
• Model-Independent Reconstruction of the Expansion History of the Universe from Type Ia Supernovae
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Constraining the SN Ia Host Galaxy Dust Law Distribution and Mass Step: Hierarchical BayeSN Analysis of Optical and Near-Infrared Light Curves
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• A model independent approach to the study of $f(R)$ cosmologies with expansion histories close to $\Lambda$CDM
• SDSS-II Supernova Survey: An Analysis of the Largest Sample of Type Ia Supernovae and Correlations with Host-Galaxy Spectral Properties
• Quantum backreaction in evolving FLRW spacetimes
• The dynamical viability of scalar-tensor gravity theories
• SNLS data are consistent with acceleration at z=3
• Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
• Noether symmetry for Gauss-Bonnet dilatonic gravity
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• The Deformable Universe
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
• Dark energy parameterizations and their effect on dark halos
• Observational Constraints on Interacting Dark Matter Model Without Dark Energy
• The Dark Energy Survey Supernova Program: Cosmological biases from supernova photometric classification
• Dark matter, and its darkness
• Observational Constraints on Dynamical Dark Energy Models
• Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
• Dark Energy and the MSSM
• Extensive search for bias in SNIa data
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Neutrino masses and mixings in the baryon triality constrained minimal supersymmetric standard model
• Estimating dust distances to Type Ia supernovae from colour excess time-evolution
• Cosmodynamics: Energy conditions, Hubble bounds, density bounds, time and distance bounds
• Cosmology of non-minimal derivative coupling to gravity in Palatini formalism and its chaotic inflation
• Dark Energy: A Unifying View
• New holographic dark energy model with non-linear interaction
• Transit String Dark Energy Models in $f(Q)$ Gravity
• Holographic dark energy and late cosmic acceleration
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Does fractal Universe describe a complete cosmic scenario?
• Constraints on oscillating dark energy models
• Compact stellar models in modified gravity
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model
• Modified GBIG Scenario as an Alternative for Dark Energy
• Gravitational Lensing with Three-Dimensional Ray Tracing
• A Model-Independent Photometric Redshift Estimator for Type Ia Supernovae
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Viscous Generalized Chaplygin Gas as a Unified Dark Fluid: Including Perturbation of Bulk Viscosity
• A comparison of perturbations in fluid and scalar field models of dark energy
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Gauge Formulation for Higher Order Gravity
• Bayesian Model Averaging in Astrophysics: A Review
• Holographic kinetic k-essence model
• Using the Topology of Large Scale Structure to constrain Dark Energy
• Single-Field Inflation After WMAP5
• Growth of structure in interacting vacuum cosmologies
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• Scalar-multi-tensorial equivalence for higher order $f\left(R,{\nabla }_{\mu }R,{\nabla }_{{\mu }_1}{\nabla }_{{\mu }_2}R,...,{\nabla }_{{\mu }_1}...{\nabla }_{{\mu }_n}R\right)$ theories of gravity
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Statistical coverage for supersymmetric parameter estimation: a case study with direct detection of dark matter
• Crossing of Phantom Divide in $F(R)$ Gravity
• Dark Energy, A Cosmological Constant, and Type Ia Supernovae
• Cosmography and large scale structure by f(R) gravity: new results
• Quintessential power-law cosmology: dark energy equation of state
• Oscillating universe in the DGP braneworld
• SNIa Host Galaxy Properties and the Dust Extinction Distribution
• Topological Static Spherically Symmetric vacuum Solutions in $\mathcal{F}(R,G)$ Gravity
• Vacuum Energy as the Origin of the Gravitational Constant
• Phantom solution in a non-linear Israel-Stewart theory
• First-order formalism for dark energy and dust
• A conventional approach to the dark-energy concept
• Interacting New Agegraphic Dark Energy in a Cyclic Universe
• The GRBs Hubble diagram in quintessential cosmological models
• Graviton corrections to the Newtonian potential using invariant observables
• Bouncing models with a cosmological constant
• First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters
• Precision Cosmology: Successes and Challenges
• Testing $f(R)$ dark energy model with the large scale structure
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• On the growth of perturbations in interacting dark energy and dark matter fluids
• Quasars as probes of cosmological reionization
• High-resolution imaging of the cosmic mass distribution from gravitational lensing of pregalactic HI
• Extinction properties of lensing galaxies
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• Light Curves of 213 Type Ia Supernovae from the ESSENCE Survey
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• Geometrical Diagnostics for Generalized Chaplygin Gas
• Application of Bayesian graphs to SN Ia data analysis and compression
• A model-independent dark energy reconstruction scheme using the geometrical form of the luminosity-distance relation
• Disorder on the landscape
• Exponential Cardassian Universe
• Topology of large scale structure as test of modified gravity
• The unification of inflation and late-time acceleration in the frame of $k$-essence
• Testing the interaction model with cosmological data and gamma-ray bursts
• The birth rate of supernovae from double-degenerate and core-degenerate systems
• Light curve studies of nearby Type Ia Supernovae with a Multi-band Stretch method
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Near-IR search for lensed supernovae behind galaxy clusters: I. Observations and transient detection efficiency
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• Gravitational Dust Collapse in $f(R)$ Gravity
• Constraining the dark energy and smoothness-parameter with supernovae
• Consistency of LCDM with Geometric and Dynamical Probes
• A Critique of Supernova Data Analysis in Cosmology
• Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions
• An Unbiased Method of Modeling the Local Peculiar Velocity Field with Type Ia Supernovae
• Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda$CDM model
• A Redshift Dependent Color-Luminosity Relation in Type 1a Supernovae
• The impact of neutrino masses on the determination of dark energy properties
• Testing Cosmological General Relativity against high redshift observations
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Realistic Cyclic Magnetic Universe
• The birth rate of subluminous and overluminous type Ia supernovae
• Bayesian constraints on dark matter halo properties using gravitationally-lensed supernovae
• Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• Viscous Fluids and Gauss-Bonnet Modified Gravity
• Consistency Test of Dark Energy Models
• Inflationary susceptibilities, duality and large-scale magnetic fields generation
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological bounds on oscillating dark energy models
• Tension between SN and BAO: current status and future forecasts
• Conformal Hamiltonian Dynamics of General Relativity
• Cosmological acceleration
• The Abnormally Weighting Energy Hypothesis: the Missing Link between Dark Matter and Dark Energy
• Linear Perturbation constraints on Multi-coupled Dark Energy
• Linear perturbations in K-mouflage cosmologies with massive neutrinos
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• The luminosity-redshift relation in brane-worlds: II. Confrontation with experimental data
• Constraints on the DGP Universe Using Observational Hubble parameter
• Be It Unresolved: Measuring Time Delays from Lensed Supernovae
• Testing the mutual consistency of different supernovae surveys
• Testing Lambda and the Limits of Cosmography with the Union2.1 Supernova Compilation
• Cosmological Parameters From Supernovae Associated With Gamma-ray Bursts
• Confronting Tracker Field Quintessence with Data
• Constraints on Quintessence From Using Cosmological Data
• Integrated Cosmological Probes: Extended Analysis
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Dynamical Background
• Holographic interacting dark energy in the braneworld cosmology
• Probing the isotropy of cosmic acceleration using different supernova samples
• Constraining the dark energy and smoothness parameter with type Ia Supernovae and Gamma-Ray Bursts
• The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties
• Dark Matter Halos from the Inside Out
• Host Galaxy Extinction of SNIa: Co-evolution of ISM Structure and Extinction Law with Star-Formation
• Cosmological Implications of 5-dimensional Brans-Dicke Theory
• On the Emergence of Accelerating Cosmic Expansion in f(R) Theories of Gravity
• Extended Cosmology in Palatini f(R)-theories
• A Complete Cosmological Scenario in Teleparallel Gravity
• Reconstructing the properties of dark energy from recent observations
• Cosmological Parameter Estimation from SN Ia data: a Model-Independent Approach
• Survey Requirements for Accurate and Precise Photometric Redshifts for Type Ia Supernovae
• More Evidence for the Redshift Dependence of Color from the JLA Supernova Sample Using Redshift Tomography
• Utilizing Type Ia Supernovae in a Large, Fast, Imaging Survey to Constrain Dark Energy
• Raytracing simulations of coupled dark energy models
• Perturbations for transient acceleration
• Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process
• The Type Ia supernovae rate with Subaru/XMM-Newton Deep Survey
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Distance-redshift from an optical metric that includes absorption
• Detecting z > 2 Type IIn Supernovae
• On the Rates of Type Ia Supernovae in Dwarf and Giant Hosts with ROTSE-IIIb
• Revisiting the matter power spectra in $f(R)$ gravity
• Probing Dark Energy Inhomogeneities with Supernovae
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• Prospects and pitfalls of gravitational lensing in large supernova surveys
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• Anisotropy in Pantheon+ supernovae
• Bouncing Universe with Non-minimally Coupled Quintom Matter
• Self accelerating solutions in a DGP brane with a scalar field trapped on it: the dynamical systems perspective
• Weak Gravitational Lensing in Fourth Order Gravity
• Inhomogeneous viscous fluids in FRW universe
• Averaging in cosmological models using scalars
• CCDM model from quantum particle creation: constraints on dark matter mass
• Deviation from $\Lambda$CDM: Pressure Parametrization
• Constraints on the physical properties of Type Ia supernovae from photometry
• Type Ia supernova parameter estimation: a comparison of two approaches using current datasets
• Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• Dark matter interacts with variable vacuum energy
• The First Data Release from SweetSpot: 74 Supernovae in 36 Nights on WIYN+WHIRC
• Cosmological constraint on Brans-Dicke Model
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• $\Lambda$CDM-type cosmological model and observational constraints
• Dark Energy-Dark Matter Interaction from the Abell Cluster A586
• Limitations of Bayesian Evidence Applied to Cosmology
• Gravity and Mirror Gravity in Plebanski Formulation
• PHotometry Assisted Spectral Extraction (PHASE) and identification of SNLS supernovae
• Dark Matter from the Inflaton Field
• Possible dark energy imprints in gravitational wave spectrum of mixed neutron-dark-energy stars
• Linking Extragalactic Transients and their Host Galaxy Properties: Transient Sample, Multi-Wavelength Host Identification, and Database Construction
• A 5D noncompact Kaluza -Klein cosmology in the presence of Null perfect fluid
• Non-parametric reconstruction of cosmological observables using Gaussian Processes Regression
• Thermodynamical Behaviour of Inhomogeneous Universe with Varying $\Lambda$ in Presence of Electromagnetic Field
• Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
• A new class of holographic dark energy models in LRS Bianchi Type-I
• On Bianchi type III Cosmological Model with Quadratic EoS in Lyra Geometry
• Cosmological constraints in the presence of ionizing and resonance radiation at recombination
• Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Supernovae and Gaia
• Interacting entropy-corrected holographic Chaplygin gas model
• The zenithal 4-m International Liquid Mirror Telescope: a unique facility for supernova studies
• Is Thick Brane Model Consistent with the Recent Observations?
• Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
• Constraining a double component dark energy model using type Ia supernovae data
• Precision measurements of large scale structure with future type Ia supernova surveys
• A simplified approach for Chaplygin-type cosmologies
• Quantum corrections for spinning particles in de Sitter
• Inhomogeneous Bulk Viscous Fluid Universe with Electromagnetic Field and Variable $\Lambda$-Term
• Liverpool Telescope 2: a new robotic facility for rapid transient follow-up
• Can galaxy clusters, type Ia supernovae and cosmic microwave background rule out a class of modified gravity theories?
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Dark energy constraints from a space-based supernova survey
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• Axially magnetized Dark Energy cosmological model
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Revisiting the screening mechanism in $f(R)$ gravity
• Testing and selection of cosmological models with $(1+z{)}^6$ corrections
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• Rest-Frame R-band Lightcurve of a z~1.3 Supernova Obtained with Keck Laser Adaptive Optics
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• FLRW accelerating universe with interactive dark energy
• Unification of cosmological scalar fields
• An optimal basis system for cosmology: data analysis and new parameterisation
• Data analysis methods for the cosmic microwave background
• Is dark energy evolving?
• Observations of the High Redshift Universe
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• Acceleration of the Universe driven by the Casimir force
• Multi-dimensional numerical simulations of type Ia supernova explosions
• Weighing neutrinos in the presence of a running primordial spectral index
• New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity
• Hybrid dark energy
• Constraints on Dark Energy Models Using Late Universe Probes
• Implications of Two Type Ia Supernova Populations for Cosmological Measurements
• Smooth deformations and cosmic statefinders
• Is there a standard measuring rod in the Universe?
• iPTF Survey for Cool Transients
• Cosmic Type Ia SN rate and constraints on SN Ia progenitors
• Interacting Ghost Dark Energy in Complex Quintessence Theory
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Observational Evidence for Negative-Energy Dust in Late-Times Cosmology
• Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxies
• Observational constraints on a cosmological model with Lagrange multipliers
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Measuring Baryon Acoustic Oscillations with Millions of Supernovae
• Weighing dark matter haloes with gravitationally lensed supernovae
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Probing the course of cosmic expansion with a combination of observational data
• An FLRW interacting dark energy model of the Universe
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Dark Energy From Vacuum Fluctuations
• Coupled quintessence with a possible transient accelerating phase
• Properties of type Ia supernovae inside rich galaxy clusters
• High Redshift Investigation On The Dark Energy Equation of State
• Second-order matter fluctuations via higher-order galaxy correlators
• Extending the redshift-distance relation in Cosmological General Relativity to higher redshifts
• Scalar field dark energy perturbations and the Integrated Sachs Wolfe effect
• Cosmology With A Dark Refraction Index
• Current lookback time-redshift bounds on dark energy
• Symmetric-Bounce Quantum State of the Universe
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Constraints on Cubic and $f(P)$ Gravity from the Cosmic Chronometers, BAO & CMB datasets : Use of Machine Learning Algorithms
• Simulations of structure formation in interacting dark energy cosmologies
• Is a Bose-Einstein Condensate a good candidate for Dark Matter? A test with Galaxy Rotation Curves
• The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS
• Phantom Accretion by Black Holes and the Generalized Second Law of Thermodynamics
• Cosmological Constant in a Model with Superstring-Inspired E_6 Unification and Shadow Theta-Particles
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Power-law solutions and accelerated expansion in scalar-tensor theories
• The Hubble constant and dark energy from cosmological distance measures
• Exploring Plane Symmetric Solutions in $f(R)$ Gravity
• FRW dark energy cosmological model with hybrid expansion law
• Interacting Scalar fields: Dark matter and early dark energy
• Towards observational constraints on negative (1+z)^4 type contribution in the Friedmann equation
• Non-flat universe and interacting dark energy model
• Dark energy and the hierarchy problem
• Interacting holographic dark energy models: A general approach
• The $k$-essence scalar field in the context of Supernova Ia Observations
• Scalar field power-law cosmology with spatial curvature and dark energy-dark matter interaction
• Projected distances to host galaxy reduce SNIa dispersion
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Interacting holographic dark energy in the scalar-Gauss-Bonnet gravity
• Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Distinguishing f(R) theories from general relativity by gravitational lensing effect
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Observational tests of backreaction with recent data
• Reconstructing the interaction between the dark matter and holographic dark energy
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data
• Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method
• Complete density perturbations in the Jordan-Fierz-Brans-Dicke theory
• On the stability of spherically symmetric spacetimes in metric f(R) gravity
• Constraints on the Phase Plane of the Dark Energy Equation of State
• Probing the Progenitors of Type Ia Supernovae using Circumstellar Material Interaction Signatures
• Simplified Quartessence Cosmology
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• Like vs. Like: Strategy and Improvements in Supernova Cosmology Systematics
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• Effective dark matter power spectra in $f(R)$ gravity
• Halting eternal acceleration with an effective negative cosmological constant
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• Testing the consistency between cosmological measurements of distance and age
• Neutrino Dark Energy With More Than One Neutrino Species
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• Constraints on the Transition Redshift using Hubble Phase Space Portrait
• Non-existence of Extended Holographic Dark Energy with Hubble Horizon
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Decaying dark energy in light of the latest cosmological dataset
• Holographic dilatonic model of dark energy
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Classification of Cosmic Scale Factor via Noether Gauge Symmetries
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• UV Properties of Type Ia Supernova and their Host Galaxies
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Near-infrared K corrections of Type Ia Supernovae and their errors
• Extended General Relativity: large-scale antigravity and short-scale gravity with ω=-1 from five dimensional vacuum
• Relaxing neutrino mass bounds by a running cosmological constant
• Testing for redshift evolution of Type Ia supernovae using the strongly lensed PS1-10afx at $z=1.4$
• Reducing the gravitational lensing scatter of Type Ia supernovae without introducing any extra bias
• Probing the Largest Cosmological Scales with the CMB-Velocity Correlation
• Confronting quintessence models with recent high-redshift supernovae data
• Gluon condensate, modified gravity, and the accelerating Universe
• First-order formalism for the quintom model of dark energy
• Tachyon model of Tsallis holographic dark energy
• Spectroscopic observations of eight supernovae at intermediate redshift
• Stability, dark energy parameterization and swampland aspect of Bianchi Type-$V{I}_h$ cosmological models with f(R, T)-gravity
• Time variable $\Lambda$ and the accelerating Universe
• Tsallis holographic dark energy under Complex form of Quintessence model
• Type Ia Supernova Distance Modulus Bias and Dispersion From K-correction Errors: A Direct Measurement Using Lightcurve Fits to Observed Spectral Time Series
• Constraining dust and color variations of high-z SNe using NICMOS on Hubble Space Telescope
• Reducing Zero-point Systematics in Dark Energy Supernova Experiments
• Stability analysis in Modified Non-Local Gravity
• Comparison of cosmological parameter inference methods applied to supernovae lightcurves fitted with SALT2
• Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology
• The cosmological constant in the brane world of string theory on $S^1/Z_2$
• Particle creation in the framework of f(G) gravity
• Hubble Diagram of Gamma-Rays Bursts calibrated with Gurzadyan-Xue Cosmology
• Time-dependent diffusive interactions between dark matter and dark energy in the context of $k-$essence cosmology
• Late-time acceleration driven by shift-symmetric Galileon in the presence of Torsion
• The Incidence of Dwarf Novae in Large Area Transient Searches
• Properties of the Top Quark
• Testing backreaction effects with observational Hubble parameter data
• Satellite-Mounted Light Sources as Photometric Calibration Standards for Ground-Based Telescopes
• Interacting holographic tachyon model of dark energy
• Constraining Perturbative Early Dark Energy with Current Observations
• Going Forward with the Nancy Grace Roman Space Telescope Transient Survey: Validation of Precision Forward-Modeling Photometry for Undersampled Imaging
• Gas mass fraction from XMM-Newton and Chandra high redshift clusters and its use as a cosmological test
• Cosmological constraints on unparticle dark matter
• On the stability of the dark energy based on generalized uncertainty principle
• Impact of Rubin Observatory cadence choices on supernovae photometric classification
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Is Dark Energy Abnormally Weighting?
• Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
• Generalized Model for $\Lambda$-Dark Energy
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• A search for transients in the Reionization Lensing Cluster Survey (RELICS): Three new supernovae
• Tachyonic (phantom) power-law cosmology
• Interacting warm dark matter
• Improved parametrization of the growth index for dark energy and DGP models
• Effect of low anisotropy on cosmological models by using supernova data
• The Science Case for PILOT II: the Distant Universe
• Age problem in holographic dark energy
• Classification of the FRW universe with a cosmological constant and a perfect fluid of the equation of state $p=w\rho$
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• An extension of the cosmological standard model with a bounded Hubble expansion rate
• Model-Independent Plotting of the Cosmological Scale Factor as a Function of Lookback Time
• A way to get rid of cosmological constant and zero point energy problems of quantum fields through metric reversal symmetry
• Qualitative analysis and characterization of two cosmologies including scalar fields
• Diffusive dark matter and dark energy scenario and $k-$essence in the context of Supernova Ia observations
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• Local dark energy: HST evidence from the expansion flow around Cen A/M83 galaxy group
• Non-minimal coupling of the phantom field and cosmic acceleration
• Quantifying parameter errors due to the peculiar velocities of type Ia supernovae
• FM 047-02: a collisional pair of galaxies with a ring
• Towards the European strategy for particle physics: the Briefing Book
• Multicolor light curves simulations of Population III core-collapse supernovae: from shock breakout to ${}^{56}$Co decay
• Cosmology from one galaxy in a void?
• No-Bang Quantum State of the Cosmos
• Ricci curvature non-minimal derivative coupling cosmology with field re-scaling
• $\Lambda$-CDM type Heckmann - Suchuking model and union 2.1 compilation
• Cosmology of fermionic dark matter
• Reconstruction of $f(R)$, $f(T)$ and $f(\mathcal{G})$ models inspired by variable deceleration parameter
• Non-singular inflation with vacuum decay
• Latest Observational Constraints on Cardassian Models
• Dark energy in thermal equilibrium with the cosmological horizon?
• A study of the remarkable galaxy system AM 546-324 (the core of Abell S0546)
• GRBs spectral correlations and their cosmological use
• Understanding Type Ia Supernova Distance Biases by Simulating Spectral Variations
• Scalar - Tensor gravity with scalar -matter direct coupling and its cosmological probe
• Constraints on Dark Energy Models from Weak Gravity Conjecture
• Reconstructing FHDE with Scalar and Gauge Fields
• Integration of the Friedmann equation for universes of arbitrary complexity
• Coupled Quintessence scalar field model in light of observational datasets
• Vacuum properties of nonsymmetric gravity in de Sitter space
• The primordial "f_NL" non-Gaussianity, and perturbations beyond the present horizon
• Modified Bekenstein-Hawking system in $f(R)$ gravity
• A possible interrelation between the estimated luminosity distances and internal extinctions of type Ia supernovae
• The Type Ia Supernova Rate in Radio and Infrared Galaxies from the CFHT Supernova Legacy Survey
• Late transient acceleration of the universe in string theory on $S^1/Z_2$
• Bootstrapping from inflationary magnetogenesis to CMB initial conditions
• The Impact of Resolution on Double-Detonation Models for Type Ia Supernovae
• Clustering of supernova Ia host galaxies
• Fuzzy Supernova Templates II: Parameter Estimation
• The Cosmological Constant Constrained with Union2.1 Supernovae Type Ia Data. Derivation and evaluation of several FRW and Carmeli models presenting underwhelming support for the standard model
• Ellipsoidal universe in the brane world
• Specific Effect of Peculiar Velocities on Dark-Energy Constraints from Type Ia Supernovae
• Brans-Dicke model constrained from Big Bang nucleosynthesis and magnitude redshift relations of Supernovae
• Can Dark Matter be a Scalar Field?
• Optical Cross Correlation Filters: An Economical Approach for Identifying SNe Ia and Estimating their Redshifts
• Observational constraint on dynamical evolution of dark energy
• CCDM Model with Spatial Curvature and The Breaking of "Dark Degeneracy"
• On the Effective Equation of State of Dark Energy
• Constraining Parameters of Generalized Cosmic Chaplygin Gas in Loop Quantum Cosmology
• What can be learned about dark energy evolution?
• "Expansion" around the vacuum: how far can we go from Lambda?
• Unveiling the Universe with Emerging Cosmological Probes
• Towards an Observational Appraisal of String Cosmology
• Concentrating the Dark Matter in Galaxy Clusters through Tidal Stripping of Baryonically-Compressed Galactic Halos
• Particle creation in flat FRW Universe in the framework of $f(T)$ gravity
• Why we need to see the dark matter to understand the dark energy
• Dark energy from topology change induced by microscopic Gauss-Bonnet wormholes
• Unbiased constraints on the clumpiness of universe from standard candles
• Detection efficiency and photometry in supernova surveys - the Stockholm VIMOS Supernova Survey I
• Late cosmic acceleration in a vector--Gauss-Bonnet gravity model
• Cosmological implications of the KATRIN experiment
• Radiative neutrino mass generation and dark energy
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Tachyon field inspired dark energy and supernovae constraints
• Photometric type Ia supernova surveys in narrow band filters
• The Next Generation of Cosmological Measurements with Type Ia Supernovae
• Anisotropies of Diffusive Ultra-high Energy Cosmic Rays in $f(R)$ Gravity Theory
• Do recent supernovae Ia observations tend to rule out all the cosmologies?
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• A Class of Anisotropic Five-Dimensional Solutions for the Early Universe
• A symmetry for vanishing cosmological constant
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• The discovery and classification of 16 supernovae at high redshifts in ELAIS-S1 - the Stockholm VIMOS Supernova Survey II
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Fitting the luminosity data from type Ia supernovae in the frame of the Cosmic Defect theory
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• The Matrix Reloaded - on the Dark Energy Seesaw
• The preliminary statistical analysis of LAMOST DR8 low resolution AFGK stars
• Complementarity of Future Dark Energy Probes
• Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
• Probing the cosmic acceleration from combinations of different data sets
• A Nearly Model-Independent Characterization of Dark Energy Properties as a Function of Redshift
• Constraining some $r^{-n}$ extra-potentials in modified gravity models with LAGEOS-type laser-ranged geodetic satellites
• SNIa detection in the SNLS photometric analysis using Morphological Component Analysis
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• From Barthel Randers Kropina Geometries to the Accelerating Universe: A Brief Review of Recent Advances in Finslerian Cosmology
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Scenarios of cosmic string with variable cosmological constant
• Reconstructing thawing quintessence with multiple datasets
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Constraints on smoothness parameter and dark energy using observational $H(z)$ data
• Probing for cosmological parameters with LAMOST measurement
• The Bianchi type-V Dark Energy Cosmology in Self Interacting Brans Dicke Theory of Gravity
• The Shared Causal Pasts and Futures of Cosmological Events
• Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff
• Cosmic acceleration from second order gauge gravity
• Type Ia SNe along redshift: the R(Si II) ratio and the expansion velocities in intermediate z supernovae
• Equilibrium boundary conditions, dynamic vacuum energy, and the Big Bang
• On the Determination of Neutrino Masses and Dark Energy Evolution from the Cross Correlation of CMB and LSS
• Interacting Kasner-type cosmologies
• Holographic Bound in Quantum Field Energy Density and Cosmological Constant
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Navigability of Random Geometric Graphs in the Universe and Other Spacetimes
• Comparing the light curves of simulated Type Ia Supernovae with observations using data-driven models
• Statefinders and observational measurement of superenergy
• Transient Detection and Classification
• Complementary cosmological tests of RSII brane models
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Spectra of dynamical Dark Energy cosmologies from constant-w models
• Variability and transient search in the SUDARE-VOICE field: a new method to extract the light curves
• The Compilation and Validation of the Spectroscopic Redshift Catalogs for the DESI-COSMOS and DESI-XMMLSS Fields
• Nonlinear Resonance in Hořava-Lifshitz Bouncing Cosmologies
• A comprehensive analysis of the compact phase space for Hu-Sawicki $f(R)$ dark energy models including spatial curvature
• Constraints on the unified dark energy-dark matter model from latest observational data
• Brane cosmology in the Horava-Witten heterotic M-Theory on $S^1/Z_2$
• Hořava-Lifshitz Bouncing Bianchi IX Universes: A Dynamical System Analysis
• The hierarchy problem, radion mass, localization of gravity and 4D effective Newtonian potential in string theory on $S^1/Z_2$
• Search For Type Ia Supernova NUV-Optical Subclasses
• Multipole analysis on gyroscopic precession in $f(R)$ gravity with irreducible Cartesian tensors
• Atmospheric effects in astroparticle physics experiments and the challenge of ever greater precision in measurements
• Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
• Cosmological extrapolation of MOND
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Asymptotically Friedmann self-similar scalar field solutions with potential
• Dynamics of holographic dark energy with apparent-horizon cutoff and non-minimal derivative coupling gravity in non-flat FLRW universe
• Interacting Tsallis agegraphic dark energy in DGP Braneworld Cosmology
• Consistency of $f(R)$ gravity models around solar polytropes
• Analysis of recent type Ia supernova data based on evolving dark energy models
• On the viability of a certain vector-tensor theory of gravitation
• Thick DGP braneworlds
• Observational Constraints on Phantom Crossing DGP Gravity
• SUSY SU(5) $\times S_4$ GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large ${\theta }_{13}^{PMNS}$
• Liverpool Telescope 2: a new robotic facility for time domain astronomy in 2020+
• Primordial black hole detection through diffractive microlensing
• Nonparametric determination of redshift evolution index of Dark Energy
• Gamma Ray Bursts: Cosmic Rulers for the High-Redshift Universe?
• The generalized second law of thermodynamics of the universe bounded by the event horizon and modified gravity theories
• Testing and Combining Transient Spectral Classification Tools on 4MOST-like Blended Spectra
• Constraints on dark energy evolution
• Searching for non-diagonal Mass varying mechanism in the ${\nu }_{\mu }$-${\nu }_{\tau }$ system
• Finite bounded expanding white hole universe without dark matter
• Direct Dark Matter Searches with CDMS and XENON
• Magnetic Suppression of Cosmic Rays' Flux in $\mathbf{f}(\mathbf{R})$ and $\mathbf{f}(\mathbf{Q})$ Theories of Gravity
• Slow-roll, acceleration, the Big Rip and WKB approximation in NLS-type formulation of scalar field cosmology
• Small cosmological constant in seesaw mechanism with breaking down SUSY
• MUSUBI (MegaCam Ultra-deep Survey: $u^{\ast }$-Band Imaging)-Data for the COSMOS and SXDS Fields
• Constraints on Holographic cosmologies from strong lensing systems
• Constraining the runaway dilaton and quintessential dark energy
• On rates of supernovae strongly lensed by galactic haloes in Millennium Simulation
• Accelerating Universe: Observational Status and Theoretical Implications
• The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
• An Information Theory Approach on Deciding Spectroscopic Follow Ups
• Entropy of cosmological black holes and generalized second law in phantom energy-dominated universe
• The establishment of the Standard Cosmological Model through observations
• Anisotropy in the cosmic acceleration inferred from supernovae
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• Analytical considerations about the cosmological constant and dark energy
• Geometrical constraints on dark energy models
• Generalized particle dynamics in anti de Sitter spaces: A source for dark energy
• Propagating Uncertainties in the SALT3 Model Training Process to Cosmological Constraints
• Observational constraints on a Yang-Mills condensate dark energy model
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Effect of lensing magnification on type Ia supernova cosmology
• Molecular content of a type-Ia SN host galaxy at z=0.6
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• APSIS - an Artificial Planetary System in Space to probe extra-dimensional gravity and MOND
• Data compression of measurements of peculiar velocities of Supernovae Ia
• Mass Varying Neutrinos in Supernovae
• Is scalar-tensor gravity consistent with polytropic stellar models?
• Gravitational Waves Emission in Quadratic Gravity: longitudinal modes, angular momentum emission, and positivity of the radiated power
• Hubble Expansion as an Einstein Curvature
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• Anisotropic cosmological solutions to the $Y(R)F^2$ gravity
• Constraining modified growth patterns with tomographic surveys
• An Exploration of Heterogeneity in Supernova Type Ia Samples
• Constraining Inflationary Scenarios with Braneworld Models and Second Order Cosmological Perturbations
• Photometric properties of intermediate redshift Type Ia Supernovae observed by SDSS-II Supernova Survey
• Constraining the Nonextensive Mass Function of Halos from BAO, CMB and X-ray data
• Multipole analysis in the radiation field for linearized $f(R)$ gravity with irreducible Cartesian tensors
• Non-linear Phenomenology of Disformally Coupled Quintessence
• The Djorgovski-Gurzadyan dark energy integral equation and the Hubble diagram
• A New Insight into the Classification of Type Ia Supernovae
• Cosmology in holographic non-minimal derivative coupling theory: constraints from inflation and variation of gravitational constant
• Cosmology with type-Ia supernovae
• A New Approach to Testing Dark Energy Models by Observations
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Power-law solutions for TeVeS
• Can MONDian vector theories explain the cosmic speed up ?
• Holographic de Sitter Spacetime and Quantum Corrections to The Cosmological Constant
• Dark energy from quantum wave function collapse of dark matter
• Shadow Fermions, Messenger Scalars and Leptogenesis
• Two c's in a pod: Cosmology independent measurement of the Type Ia supernova colour-luminosity relation with a sibling pair
• Constraining spacetime variations of nuclear decay rates from light curves of type Ia supernovae
• Gravitational collapse of spherical shells of fluid in the isotropic homogeneous universe
• ZTF SN Ia DR2: Improved SN Ia colors through expanded dimensionality with SALT3+
• Natures of Statefinder Parameters and Om Diagnostic for Cardassian Universe in Horava-Lifshitz Gravity
• Bayesian analysis of the backreaction models
• A modification of Einstein-Schrodinger theory that contains Einstein-Maxwell-Yang-Mills theory
• Red-shift parametrizations of dark energy and observational constraint on their parameters: Galileon gravity as background
• Cosmic Acceleration Data and Bulk-Brane Energy Exchange
• Reconstructing the weak lensing magnification distribution of Type Ia supernovae
• Eternally inflating cosmologies from intersecting spacelike branes
• The Self-Calibrating Hubble Diagram
• Emergent Universe as an interaction in the dark sector
• Considerations for optimizing photometric classification of supernovae from the Rubin Observatory
• A new mechanism for dark energy: the adaptive screening
• Instruments on large optical telescopes -- A case study
• Some remarks on the observational constraints on the self-interacting scalar field model for dark energy
• Photometric observations of the supernova 2009nr
• Dark matter: A phenomenological existence proof
• Hubble Diagrams in the Jordan and Einstein Frames
• Supernova environments in J-PLUS. Normalized Cumulative Rank distributions and stellar population synthesis, combining narrow- and broad-band filters
• Decoupling of Higgs boson from the inflationary stage of Universe evolution
• Cosmological constraints from supernova data set with corrected redshift
• Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario
• Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
• Probing Systematic Bias in Low-Redshift Type Ia Supernova Measurements by Cross Analyzing Surface Brightness and Hubble Residuals
• Constraints on dark energy and cosmic topology
• Modeling Gravastar Structure admitting Kuchowicz Spacetime in Rastall Gravity Theory
• A Null Test of the Metric Nature of the Cosmic Acceleration
• Cosmological dynamics of holographic dark energy with non-minimally coupled scalar field
• Constraining bouncing cosmology caused by Casimir effect
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5
• Massive neutrinos and dark energy
• f(R) cosmological solutions with varying speed of light
• Cosmological General Relativity With Scale Factor and Dark Energy
• Generalized Second Law of Thermodynamics on the Event Horizon for Interacting Dark Energy
• Cosmological bootstrap
• The Geometry of the Universe
• Role of Resonances in Heavy Meson Processes within Standard Model and Beyond
• Non-perturbative scalar gauge-invariant metric fluctuations from the Ponce de Leon metric in the STM theory of gravity
• Microlensing in phase space II: Correlations analysis
• Angular Power Spectrum in Modular Invariant Inflation Model
• Long-wavelength gravitational waves and cosmic acceleration
• Observations of General Relativity at strong and weak limits
• Remote quantum states in curved spacetime
• Cylindrically Symmetric Scalar Field and its Lyapunov stability in General Relativity
• Lower bounds on photometric redshift errors from Type Ia supernovae templates
• Measuring Type Ia Supernova Distances and Redshifts From Their Multi-band Light Curves
• Dynamical analysis of $k$-essence cosmology in the light of Supernova Ia observations
• Energy conditions and entropy density of the universe
• Propagation of gravitational waves in a universe with slowly-changing equation of state
• A note on vacuum energy from the de Sitter spectrum
• Fluctuation of the Hubble parameter
• Modelling Cosmic Rays Flux with Pierre Auger and Telescope Array Data in $\mathbf{f}(\mathbf{R})$ and $\mathbf{f}(\mathbf{Q})$ Theories of Gravity
• Agegraphic Model based on the Generalized Uncertainty Principle
• Unified Model for Inflation and the Dark Side of the Universe
• Addressing the Crisis in Fundamental Physics
• Yano-Schrödinger Hyperfluid: Cosmological Implications
• Ultra-high energy cosmic rays with UFA-15 source model in Bumblebee gravity theory
• Genetic algorithm demystified for cosmological parameter estimation
• Machine learning analysis of Photometric data from the Dark Energy Survey
• Elliptic solutions of generalized Brans-Dicke gravity with a non-universal coupling
• Using the large scale quasar clustering to constrain flat quintessential universes
• Training Custom Light Curve Models of SN Ia Sub-Populations Selected According to Host Galaxy Properties
• PISCOLA: a data-driven transient light-curve fitter
• Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
• The Wide-field High-resolution Infrared TElescope (WHITE)
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• The creation of radiation and the relic of inflaton potential
• Accidental deep field bias in CMB T and SNe $z$ correlation