The DESI Experiment Part I: Science,Targeting, and Survey Design

Abstract

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($2.1<z<3.5$), for the Ly-$\alpha$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.

Cited by in corpus (835)

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• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Removing Imaging Systematics from Galaxy Clustering Measurements with Obiwan : Application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey Emission Line Galaxy Sample
• Wavelet Moments for Cosmological Parameter Estimation
• Parametrising non-linear dark energy perturbations
• The PAU Survey: Spectral features and galaxy clustering using simulated narrow band photometry
• Non-linear general relativistic effects in the observed redshift
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• Tests of Neutrino and Dark Radiation Models from Galaxy and CMB surveys
• The 3D Lyman-$\alpha$ Forest Power Spectrum from eBOSS DR16
• Computational Tools for the Spectroscopic Analysis of White Dwarfs
• Probing a Steep EoS for Dark Energy with latest observations
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Cylinders out of a top hat: counts-in-cells for projected densities
• Impact of inhomogeneous reionization on the Lyman-α forest
• Large-scale density and velocity field reconstructions with neural networks
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Enabling matter power spectrum emulation in beyond-$\Lambda$CDM cosmologies with COLA
• Reconstructing the baryon acoustic oscillations using biased tracers
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• Light Fields during Inflation from BOSS and Future Galaxy Surveys
• Joint velocity and density reconstruction of the Universe with nonlinear differentiable forward modeling
• Generating Synthetic Cosmological Data with GalSampler
• The HI intensity mapping bispectrum including observational effects
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Analytical and EZmock covariance validation for the DESI 2024 results
• Accurately Weighing Neutrinos with Cosmological Surveys
• DAHe white dwarfs from the DESI survey
• Identifying Tidal Disruption Events via Prior Photometric Selection of Their Preferred Hosts
• Constraints on Steep Equation of State for the Dark Energy using BAO
• Cresting the wave: Proper motions of the Eastern Banded Structure
• Barry and the BAO Model Comparison
• Data-Driven Selection and Spectral Classification of White Dwarf Stars
• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
• The universal multiplicity function: counting halos and voids
• BCS in the Sky: Signatures of Inflationary Fermion Condensation
• Non-linearities in the Lyman-$\alpha$ forest and in its cross-correlation with dark matter halos
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• Measuring the integrated Sachs-Wolfe effect from the low-density regions of the universe
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• Neutrino effects on the morphology of cosmic large-scale structure
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Cross-correlating 21 cm and galaxy surveys: implications for cosmology and astrophysics
• Cosmological lensing ratios with DES Y1, SPT and Planck
• Relation between the Turnaround radius and virial mass in $f(R)$ model
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• Clustering dark energy imprints on cosmological observables of the gravitational field
• The LSST DESC Data Challenge 1: Generation and Analysis of Synthetic Images for Next Generation Surveys
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis
• Cosmological Inference from Galaxy-Clustering Power Spectrum: Gaussianization and Covariance Decomposition
• Taming assembly bias for primordial non-Gaussianity
• Multi-tracer power spectra and bispectra: Formalism
• Cosmological Perturbations and Invariant Observables in Geodesic Lightcone Coordinates
• The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions
• The scale of cosmic homogeneity as a standard ruler
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• The miniJPAS survey: Identification and characterization of the emission line galaxies down to $z<0.35$ in the AEGIS field
• Density reconstruction from biased tracers and its application to primordial non-Gaussianity
• Cross-correlating 2D and 3D galaxy surveys
• Oxygen-enhanced extremely metal-poor DLAs: A signpost of the first stars?
• Evidence for baryon acoustic oscillations from galaxy-ellipticity correlations
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- II. A case study for magnification bias and radio continuum surveys
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Nonlinear Redshift-Space Distortions in the Harmonic-space Galaxy Power Spectrum
• The assembly bias of emission line galaxies
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Assessing the accuracy of cosmological parameters estimated from velocity -- density comparisons via simulations
• Modelling Non-Linear Effects of Dark Energy
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue
• Modeling the Lyman-$\alpha$ forest with Eulerian and SPH hydrodynamical methods
• Multi-wavelength spectroscopic probes: biases from neglecting light-cone effects
• Renormalization of Lagrangian bias via spectral parameters
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Compact Groups of Galaxies in Sloan Digital Sky Survey and LAMOST Spectral Survey. II. Dynamical Properties of Isolated and Embedded Groups
• Measuring ISW with next-generation radio surveys
• A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• Second-order gauge-invariant formalism for the cosmological observables: Complete verification of their gauge-invariance
• Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Constraining planet formation around 6$M_{\odot }$-8$M_{\odot }$ stars
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• The Cosmological Perturbation Theory on the Geodesic Light-Cone background
• Local Primordial Non-Gaussianities and Super-Sample Variance
• A neural network emulator for the Lyman-$\alpha$ 1D flux power spectrum
• Estimating redshift distributions using Hierarchical Logistic Gaussian processes
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• A cosmic glitch in gravity
• UV Background Fluctuations and Three-Point Correlations in the Large Scale Clustering of the Lyman-alpha Forest
• The PAU survey: Ly$\alpha$ intensity mapping forecast
• Large-scale structure in mimetic Horndeski gravity
• The position-dependent matter density probability distribution function
• ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
• Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• The impact of relativistic effects on the 3D Quasar-Lyman-$\alpha$ cross-correlation
• Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
• Mitigating the noise of DESI mocks using analytic control variates
• RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
• Impact of survey geometry and super-sample covariance on future photometric galaxy surveys
• Neutrino masses from large-scale structures: future sensitivity and theory dependence
• Synthetic spectra for Lyman-$\alpha$ forest analysis in the Dark Energy Spectroscopic Instrument
• Mass Functions, Luminosity Functions, and Completeness Measurements from Clustering Redshifts
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• Cosmological Probes of Structure Growth and Tests of Gravity
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses
• Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
• HI gas content of SDSS galaxies revealed by ALFALFA: implications for the mass-metallicity relation and the environmental dependence of HI in the local Universe
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Testing Quintessence Axion Dark Energy with Recent Cosmological Results
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• Application of the iterative reconstruction to simulated galaxy fields
• Forward Modeling of Spectroscopic Galaxy Surveys: Application to SDSS
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• White dwarfs identified in LAMOST Data Release 5
• Cosmology before noon with multiple galaxy populations
• The Lyman-$\alpha$ power spectrum - CMB lensing convergence cross-correlation
• Jupyter-Enabled Astrophysical Analysis for Researchers and Students
• Improving estimates of the growth rate using galaxy-velocity correlations: a simulation study
• DIGS: Deep Inference of Galaxy Spectra with Neural Posterior Estimation
• Measuring the scale dependence of intrinsic alignments using multiple shear estimates
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic measurement of structure growth and expansion rate from anisotropic galaxy clustering in Fourier space
• Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Iterative removal of redshift space distortions from galaxy clustering
• Spherical collapse in Generalized Dark Matter models
• Leptogenesis from the Asymmetric Texture
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Using Action Space Clustering to Constrain the Accretion History of Milky Way like Galaxies
• Confronting missing observations with probability weights: Fourier space and generalised formalism
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Modelling the next-to-leading order matter three-point correlation function using FFTLog
• Cosmology from the kinetic polarized Sunyaev Zel'dovich effect
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• A single parameterization for dark energy and modified gravity models
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• Correlated orientations of the axes of large quasar groups on Gpc scales
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Tribimaximal Mixing in the $SU(5)\times {\mathcal{T}}_{13}$ Texture
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Quasars at intermediate redshift are not special; but they are often satellites
• Null tests of the concordance model in the era of Euclid and the SKA
• Survey Operations for the Dark Energy Spectroscopic Instrument
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Ly$\alpha$ forest power spectrum as an emerging window into the epoch of reionization and cosmic dawn
• Measurement of the small-scale 3D Lyman-$\alpha$ forest power spectrum
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• Spectroscopic QUasar Extractor and redshift (z) EstimatorSQUEzE I: Methodology
• Impact of Massive Neutrinos and Dark Radiation on the High-redshift Cosmic Web. I. Lyman-Alpha Forest Observables
• Testing General Relativity with the Doppler magnification effect
• Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Deep Drilling in the Time Domain with DECam: Survey Characterization
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• Non-thermal Hot Dark Matter from Inflaton/Moduli Decay: The Momentum Distribution and Relaxing the Cosmological Mass Bound
• $\alpha$-attractor dark energy in view of next-generation cosmological surveys
• Quenching, bursting and galaxy shapes: colour transformation as a function of morphology
• Robustness of the pairwise kinematic Sunyaev-Zeldovich power spectrum shape as a cosmological gravity probe
• The incidence of AGN in galaxies with different stellar population ages
• Super-sample tidal modes on the celestial sphere
• Redshift-space distortions from vector perturbations
• An Inventory of Bispectrum Estimators for Redshift Space Distortions
• Weak lensing of the Lyman-alpha forest
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
• Halo Occupation Distribution of Emission Line Galaxies: fitting method with Gaussian Processes
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Constraining cluster masses from the stacked phase space distribution at large radii
• Intrinsic Alignment as an RSD Contaminant in the DESI Survey
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• On The Distribution of Bayesian Evidences
• De-noising of galaxy optical spectra with autoencoders
• Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR $Cosmo$ Simulations
• Identifying anomalous radio sources in the EMU Pilot Survey using a complexity-based approach
• How does the radio enhancement of broad absorption line quasars relate to colour and accretion rate?
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Tomographic redshift dipole: Testing the cosmological principle
• Cosmological Tests of Gravity: A Future Perspective
• Revisiting Vainshtein Screening for fast N-body simulations
• Accurate Model of the Projected Velocity Distribution of Galaxies in Dark Matter Halos
• Relativistic Effects on Galaxy Redshift Samples due to Target Selection
• Modeling iterative reconstruction and displacement field in the large scale structure
• Assessing non-linear models for galaxy clustering III: Theoretical accuracy for Stage IV surveys
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
• How dark are filaments in the cosmic web?
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• High redshift LBGs from deep broadband imaging for future spectroscopic surveys
• Impact of tidal environment on galaxy clustering in GAMA
• asevolution: a relativistic N-body implementation of the (a)symmetron
• Cosmic Filaments from Cosmic Strings
• Extracting the astrophysics of reionization from the Ly$\alpha$ forest power spectrum: a first forecast
• The alignment of galaxies at the Baryon Acoustic Oscillation scale
• Forecasts for interacting dark energy with time-dependent momentum exchange
• Subpercent Accurate Fitting of Modified Gravity Growth
• On the Fast Random Sampling and Other Properties of the Three Point Correlation Function in Galaxy Surveys
• Reconstruction with velocities
• The Jiao Tong University Spectroscopic Telescope Project
• Theoretical and Experimental Challenges in the Measurement of Neutrino Mass
• HIR4: Cosmological signatures imprinted on the cross correlation between 21-cm map and galaxy clustering
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• Using peculiar velocity surveys to constrain neutrino masses
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• The skewness of the distance-redshift relation in $\Lambda$CDM
• A machine learning approach to infer the accreted stellar mass fractions of central galaxies in the TNG100 simulation
• Accuracy of power spectra in dissipationless cosmological simulations
• The role of $T_0$ in CMB anisotropy measurements
• Cosmological Fisher forecasts for next-generation spectroscopic surveys
• Reconstructing CMB fluctuations and the mean reionization optical depth
• Mitigating the impact of fiber assignment on clustering measurements from deep galaxy redshift surveys
• A model independent constraint on the temporal evolution of the speed of light
• Towards unveiling the large-scale nature of gravity with the wavelet scattering transform
• Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and ${\sigma }_8$
• Measuring the BAO peak position with different galaxy selections
• Dynamically generated inflationary two-field potential via non-Riemannian volume forms
• Constraining neutrino mass and dark energy with peculiar velocities and lensing dispersions of Type Ia supernovae
• Skewing the CMB$\times$LSS: a Fast Method for Bispectrum Analysis
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
• Detecting neutral hydrogen at z > 3 in large spectroscopic surveys of quasars
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Searching for dark energy in the matter-dominated era
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• The two-loop power spectrum in redshift space
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations
• The effects of peculiar velocities on the morphological properties of large-scale structure
• Supervisory Coordination of Robotic Fiber Positioners in Multi-Object Spectrographs
• Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
• Measuring Cosmological Distances Using Cluster Edges as a Standard Ruler
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Resolving XENON Excess With Decaying Cold Dark Matter
• A Minimal Model for Massive Neutrinos in Newtonian N-body Simulations
• Multiplicity functions of quasars: Predictions from the MassiveBlackII simulation
• Euclid: Testing the Copernican principle with next-generation surveys
• Mitigating baryonic effects with a theoretical error covariance
• de Sitter duality and logarithmic decay of dark energy
• The central dark matter fraction of massive early-type galaxies
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• High-redshift cosmology with oxygen lines from H$\alpha$ surveys
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Improving initialization and evolution accuracy of cosmological neutrino simulations
• The flat-sky approximation to galaxy number counts -- redshift space correlation function
• Mass classification of dark matter perturbers of stellar tidal streams
• Cosmology with the MaunaKea Spectroscopic Explorer
• Selecting samples of galaxies with fewer Fingers-of-God
• Constraining galaxy-halo connection with high-order statistics
• The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
• Cosmological test of local position invariance from the asymmetric galaxy clustering
• Stellar atmospheric parameters and chemical abundances of about 5 million stars from S-PLUS multi-band photometry
• The halo 3-point correlation function: a methodological analysis
• A model-independent tripartite test of cosmic distance relations
• Litmus tests of the flat $\Lambda$CDM model and model-independent measurement of $H_0{r}_{\mathrm{d}}$ with LSST and DESI
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• Connecting Primordial Gravitational Waves and Dark Energy
• Impact of photometric redshifts on the galaxy power spectrum and BAO scale in the LSST survey
• Contribution of Flares from Tidal Disruption of Stars to high-redshift AGN
• Flat-sky Angular Power Spectra Revisited
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Neutrino Observables from a U(2) Flavor Symmetry
• Spectroscopic QUasar Extractor and redshift (z) EstimatorSQUEzE II: Universality of the results
• Halo Growth and Merger Rates as a Cosmological Test
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Tests of Acoustic Scale Shifts in Halo-based Mock Galaxy Catalogues
• Probing Large-scale UV Background Inhomogeneity Associated with Quasars using Metal Absorption
• Screened fifth forces in parity-breaking correlation functions
• Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Modeling the Spectral Diversity of Quasars in the Sixteenth Data Release from the Sloan Digital Sky Survey
• Covariant Decomposition of The Non-Linear Galaxy Number Counts and Their Monopole
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• Beyond the Lognormal Approximation: a General Simulation Scheme
• Validation of Emission-Line Galaxies Target Selection Algorithms for the Dark Energy Spectroscopic Instrument Using the MMT Binospec
• Triumvirate: A Python/C++ package for three-point clustering measurements
• A forecast for the detection of the power asymmetry from galaxy surveys
• Decoupling Local Primordial non-Gaussianity from Relativistic Effects in the Galaxy Bispectrum
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Cosmic Tidal Reconstruction with Halo Fields
• Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
• Improved selection of extremely red quasars with boxy CIV lines in BOSS
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Inpainting hydrodynamical maps with deep learning
• Non-linear Cosmological Perturbations for Coupled Dark Energy
• Euclid preparation. XXXIV. The effect of linear redshift-space distortions in photometric galaxy clustering and its cross-correlation with cosmic shear
• Predictive Dirac and Majorana Neutrino Mass Textures from $SU(6)$ Grand Unified Theories
• Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Euclid preparation. Simulations and nonlinearities beyond $\Lambda$CDM. 1. Numerical methods and validation
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Shape noise and dispersion in precision weak lensing
• Warm Hawking Relics From Primordial Black Hole Domination
• Climbing out of the shadows: building the distance ladder with black hole images
• The Commissioning Instrument for the Dark Energy Spectroscopic Instrument
• Precise self-calibration of interloper bias in spectroscopic surveys
• Performance of the Dark Energy Spectroscopic Instrument(DESI) Fiber System
• Probing cosmology via the clustering of critical points
• Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds
• Constraining the quintessential $\alpha$-attractor inflation through dynamical horizon exit method
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Massive $\nu$s through the CNN lens: interpreting the field-level neutrino mass information in weak lensing
• On the impact of the galaxy window function on cosmological parameter estimation
• Window convolution of the galaxy clustering bispectrum
• Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
• Bispectrum constraints on Primordial non-Gaussianities with the eBOSS DR16 quasars
• Probing the cosmic web in Ly$\alpha$ emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
• Effects of Dark Energy anisotropic stress on the matter power spectrum
• Contributions from primordial non-Gaussianity and General Relativity to the galaxy power spectrum
• Galaxy Spectra neural Networks (GaSNets). I. Searching for strong lens candidates in eBOSS spectra using Deep Learning
• A search for cosmological anisotropy using the Lyman alpha forest from SDSS quasar spectra
• The missing radial velocities of Gaia: a catalogue of Bayesian estimates for DR3
• DESI Commissioning Instrument Metrology
• STRRINGS: STReams in Residual Images of Nearby GalaxieS
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Nearby stellar substructures in the Galactic halo from DESI Milky Way Survey Year 1 Data Release
• Searching for low-redshift faint galaxies with MMT/Hectospec
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• Extended Fast Action Minimisation method: application to SDSS-DR12 Combined Sample
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Super-Eddington accreting massive black holes explore high-$z$ cosmology: Monte-Carlo simulations
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Anisotropic effective redshift and evolving clustering amplitude
• Cross-correlating Planck with VST ATLAS LRGs: a new test for the ISW effect in the Southern Hemisphere
• Cosmological Unification, Dark Energy and the Origin of Neutrino Mass
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• GrGadget: an N-body TreePM relativistic code for cosmological simulations
• A fully Lagrangian, non-parametric bias model for dark-matter halos
• A wide-angle formulation of foreground filters for HI intensity mapping
• Signature of Massive Neutrinos from the Clustering of Critical Points. I. Density-threshold-based Analysis in Configuration Space
• The Maunakea Spectroscopic Explorer: Thousands of Fibers, Infinite Possibilities
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• Abundance of peaks and dips in three-dimensional mass and halo density fields: a test for cosmology
• Misinterpreting Modified Gravity as Dark Energy: a Quantitative Study
• A new instability in clustering dark energy?
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• Position-dependent Voronoi probability distribution functions for matter and halos
• Conversations in the dark: cross-correlating birefringence and LSS to constrain axions
• Environmental effects on associations of dwarf galaxies
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• Dynamic Zoom Simulations: a fast, adaptive algorithm for simulating lightcones
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• Constraining Scale Dependent Growth with Redshift Surveys
• Including relativistic and primordial Non-Gaussianity contributions in cosmological simulations by modifying the initial condition
• Cosmic distance determination from photometric redshift samples using BAO peaks only
• GLEAM: Galaxy Line Emission & Absorption Modeling
• Measurement of redshift-space two- and three-point correlation of Ly$\alpha$ absorbers at $1.7<z<3.5$: Implications on evolution of the physical properties of IGM
• Forecasts for Broadband Intensity Mapping of the Ultraviolet-Optical Background with CASTOR and SPHEREx
• Prospects for cosmological research with the FAST array: 21-cm intensity mapping survey observation strategies
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Renormalization group computation of likelihood functions for cosmological data sets
• Testing for gravitational preferred directions with galaxy and lensing surveys
• The Gravitational Lensing Imprints of DES Y3 Superstructures on the CMB: A Matched Filtering Approach
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Euclid: Fast two-point correlation function covariance through linear construction
• Measuring lensing ratios with future cosmological surveys
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• Cross-correlating radial peculiar velocities and CMB lensing convergence
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• On the Dark Matter Halos of Optical and IR-selected AGN in the Local Universe
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Clusternets: A deep learning approach to probe clustering dark energy
• Cosmic acceleration in asymptotically Ricci flat Universe
• Convergence of halo statistics: code comparison between Rockstar and CompaSO using scale-free simulations
• Testing the 10 spectrograph units for DESI: approach and results
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Automated Measurement of Quasar Redshift with a Gaussian Process
• Cosmological constraints with the linear point from the BOSS survey
• TensorFlow Hydrodynamics Analysis for Ly-$\alpha$ Simulations
• K-mouflage at high $k$: extending the reach of $\text{Hi-COLA}$
• Doppler bias: impact of peculiar velocities on color selection and the large scale structure of galaxy surveys
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Constraining primordial non-Gaussianity from the large scale structure two-point and three-point correlation functions
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• 3D Correlations in the Lyman-$\alpha$ Forest from Early DESI Data
• Linear and non-linear Modified Gravity forecasts with future surveys
• Cosmology with shear ratios: a joint study of weak lensing and spectroscopic redshift datasets
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Reconstructing redshift distributions with photometric galaxy clustering
• Model-independent constraints on clustering and growth of cosmic structures from BOSS DR12 galaxies in harmonic space
• Cosmology with Cosmic Voids
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• Dark Matter and Fundamental Physics Searches with IACTs
• Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Model Independent Dark Matter Properties from Cosmic Growth
• Focal Plate Structure Alignment of the Dark Energy Spectroscopic Instrument
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Constraining Galaxy-Halo Connection Using Machine Learning
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• A theoretical approach to density-split clustering
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• The Hawking Energy in a Perturbed Friedmann-Lemaître Universe
• Non-parametric Lagrangian biasing from the insights of neural nets
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• The Effect of Interstellar Absorption on Measurements of the Baryon Acoustic Peak in the Lyman-α Forest
• Multipoles of the galaxy bispectrum on a light cone: wide-separation and relativistic corrections
• Super sample covariance and the volume scaling of galaxy survey covariance matrices
• Sub-percentage measure of distances to redshift of 0.1 by a new cosmic ruler
• Towards cosmology with Void Lensing: how to find voids sensitive to weak-lensing and numerically interpret them
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
• An empirical nonlinear power spectrum overdensity-response
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Chronos: A NIR spectroscopic survey to target the most important phases of galaxy evolution across cosmic time
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• Indicator Functions: Distilling the Information from Gaussian Random Fields