The Second Data Release of the Sloan Digital Sky Survey

Abstract

The Sloan Digital Sky Survey has validated and made publicly available its Second Data Release. This data release consists of 3324 square degrees of five-band (u g r i z) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars and calibrating blank sky patches selected over 2627 degrees of this area, and tables of measured parameters from these data. The imaging data reach a depth of r ~ 22.2 (95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 milli-arcsec rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point spread function (PSF) magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 A to 9200 A at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars, and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines, and included in the Second Data Release. The data are publically available as of 2004 March 15 via the web sites http://www.sdss.org/dr2 and http://skyserver.sdss.org .

24 pages, submitted to AJ. See ftp://ftp.astro.princeton.edu/strauss/sdss/dr2.ps for high-resolution figures

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• One thousand cataclysmic variables from the Catalina Real-time Transient Survey
• The Intrinsic Shape of Galaxies in SDSS/Galaxy Zoo
• Discovery of a Fifth Image of the Large Separation Gravitationally Lensed Quasar SDSS J1004+4112
• Pilgrim Dark Energy in $f(T,T_G)$ cosmology
• The baryonic mass function of galaxies
• Compact Symmetric Objects and Supermassive Binary Black Holes in the VLBA Imaging and Polarimetry Survey
• Testing adiabatic contraction with SDSS elliptical galaxies
• Gemini Deep Deep Survey VI: Massive Hdelta-strong galaxies at z=1
• The Post-Starburst Evolution of Tidal Disruption Event Host Galaxies
• Connecting Transitions in Galaxy Properties to Refueling
• Topology of structure in the Sloan Digital Sky Survey: model testing
• The distribution of AGN in a large sample of galaxy clusters
• Low Surface Brightness Galaxies in the SDSS: the link between environment, star-forming properties and AGN
• New Close Binary Systems from the SDSS-I (Data Release Five) and the Search for Magnetic White Dwarfs in Cataclysmic Variable Progenitor Systems
• Characterizing Inflationary Perturbations: The Uniform Approximation
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• Reconstruction of f(T) gravity from the Holographic dark energy
• Discovery of New Ultracool White Dwarfs in the Sloan Digital Sky Survey
• The Bright End of the Luminosity Function of Red Sequence Galaxies
• Boötes IV: A New Milky Way Satellite Discovered in the Subaru Hyper Suprime-Cam Survey and Implications for the Missing Satellite Problem
• Type 1 AGN at low z. III. The optical narrow line ratios
• The kinematics of late type stars in the solar cylinder studied with SDSS data
• Luminous Infrared Galaxies in the Local Universe
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Cylindrical Solutions in Modified f(T) Gravity
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• The SDSS Galaxy Angular Two-Point Correlation Function
• The kinematics and spatial distribution of stellar populations in E+A galaxies
• The SDSS u-band Galaxy Survey: Luminosity functions and evolution
• Host galaxy-active galactic nucleus alignments in the SDSS-DR7
• The Atacama Cosmology Telescope: Detection of Sunyaev-Zel'dovich Decrement in Groups and Clusters Associated with Luminous Red Galaxies
• Star Models with Dark Energy
• Optical Properties of 4248 IRAS Galaxies
• The Spatial Clustering of Low Luminosity AGN
• The radial profiles of the different mass components in galaxy clusters
• Supersymmetric Theories of Neutrino Dark Energy
• Morphological Classification of Galaxies using Photometric Parameters: the Concentration index versus the Coarseness parameter
• Anomalously low PAH emission from low-luminosity galaxies
• A New Approach to Quintessence and a Solution of Multiple Attractors
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• The large-scale environment of low surface brightness galaxies
• Using M Dwarf Spectra to Map Extinction in the Local Galaxy
• Black Hole Formation from Collapsing Dust Fluid in a Background of Dark Energy
• What triggers galaxy transformations? The environments of post-starburst galaxies
• Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry
• Near-infrared imaging of 222 nearby Hdelta-strong galaxies from the SDSS
• Introducing piXedfit -- a Spectral Energy Distribution Fitting Code Designed for Resolved Sources
• Galaxy interactions II: High density environments
• Hyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE
• Robust Machine Learning Applied to Astronomical Datasets II: Quantifying Photometric Redshifts for Quasars Using Instance-Based Learning
• Chandra and XMM Observations of Type II Quasars from the SDSS
• The Gaia-ESO Survey and CSI 2264: Substructures, disks, and sequential star formation in the young open cluster NGC 2264
• Interacting Ricci Dark Energy with Logarithmic Correction
• A wide angle tail radio galaxy in the COSMOS field: evidence for cluster formation
• Variable Faint Optical Sources Discovered by Comparing POSS and SDSS Catalogs
• Precision cluster mass determination from weak lensing
• A Survey of CN and CH Variations in Galactic Globular Clusters from SDSS Spectroscopy
• Phantom phase power-law solution in $f(G)$ gravity
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey
• A MMT/Hectospec Redshift Survey of 24 Micron Sources in the Spitzer First Look Survey
• Bivariate Galaxy Luminosity Functions in the Sloan Digital Sky Survey
• The Colours of Elliptical galaxies
• A large sample of low surface brightness disk galaxies from the SDSS. I: The sample and the stellar populations
• Virial Masses of Black Holes from Single Epoch Spectra of AGN
• New Approaches To Photometric Redshift Prediction Via Gaussian Process Regression In The Sloan Digital Sky Survey
• A Hubble Space Telescope Snapshot Survey of Dynamically Close Galaxy Pairs in the CNOC2 Redshift Survey
• On structure formation from a small-scales-interacting dark sector
• Ultraviolet, Optical, and Infrared Constraints on Models of Stellar Populations and Dust Attenuation
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Origin of holographic dark energy models
• Mergers in Galaxy Groups - I. Structure and Properties of Elliptical Remnants
• The Mass Function of Void Galaxies in the SDSS Data Release 2
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
• SDSS J0246-0825: A New Gravitationally Lensed Quasar from the Sloan Digital Sky Survey
• The MOND Fundamental Plane
• Accelerating Universe scenario in anisotropic $f\left(Q\right)$ cosmology
• Improved optical mass tracer for galaxy clusters calibrated using weak lensing measurements
• The mass-metallicity relation of Lyman-break analogues and its dependence on galaxy properties
• Post-starburst--AGN Connection: Spatially Resolved Spectroscopy of Hdelta-Strong AGNs
• A Census of Object Types and Redshift Estimates in the SDSS Photometric Catalog from a Trained Decision-Tree Classifier
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• The Small-scale Clustering of Luminous Red Galaxies via Cross-Correlation Techniques
• New Interaction between Dark Energy and Dark Matter Changes Sign during Cosmological Evolution
• Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• To use or not to use synthetic stellar spectra in population synthesis models?
• Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
• Realizing Scale-invariant Density Perturbations in Low-energy Effective String Theory
• Deep 21-cm HI Observations at z~0.1: The Precursor to the Arecibo Ultra Deep Survey
• The Luminosity, Colour and Morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
• Radial and 2D Colour Properties of E+A Galaxies
• Statistical Properties of Multi-epoch Spectral Variability of SDSS Stripe82 Quasars
• Cosmic age problem revisited in the holographic dark energy model
• A highly unequal-mass eclipsing M-dwarf binary in the WFCAM Transit Survey
• Consequences of energy conservation violation: Late time solutions of $\Lambda (T)CDM$ subclass of $f(R,T)$ gravity using dynamical system approach
• Galaxy properties from Voids to Clusters in the SDSS-DR4
• VLBI observations of bright AGN jets with KVN and VERA Array (KaVA): Evaluation of Imaging Capability
• FRII radio galaxies in the SDSS: Observational facts
• Properties of satellite galaxies in the SDSS photometric survey: luminosities, colours and projected number density profiles
• Inflationary Perturbations and Precision Cosmology
• Stellar tidal disruption candidates found by cross-correlating the ROSAT Bright Source Catalogue and XMM-Newton observations
• SDSS J0806+2006 and SDSS J1353+1138: Two New Gravitationally Lensed Quasars from the Sloan Digital Sky Survey
• Satellite Luminosities in Galaxy Groups
• The Sloan Digital Sky Survey Reverberation Mapping Project: Post-Starburst Signatures in Quasar Host Galaxies at z < 1
• Reconstruction of f(T) gravity according to holographic dark energy
• The clustering of barred galaxies in the local Universe
• Stability of Anisotropic Stellar Filaments
• Colours of Bulges and Discs within Galaxy Clusters and the Signature of Disc Fading on Infall
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• Infrared-Faint Radio Sources: A New Population of High-redshift Radio Galaxies
• On Anisotropic Dark Energy
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• A tale of two galaxies: light and mass in NGC891 and NGC7814
• X-ray Insights Into Interpreting CIV Blueshifts and Optical/UV Continua
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Barred Galaxies in the Abell 901/2 Supercluster with STAGES
• Spatially Resolved Spectroscopy of the E+A Galaxies in the z=0.32 Cluster AC114
• HI Selected Galaxies in the Sloan Digital Sky Survey I: Optical Data
• Five New High-Redshift Quasar Lenses from the Sloan Digital Sky Survey
• Do star formation rates of galaxy clusters depend on mass?: blue/late-type fractions, total star formation rates of 115 galaxy clusters as a function of cluster virial mass
• Can $f(T)$ gravity theories mimic $\Lambda$CDM cosmic history
• IC 225: a dwarf elliptical galaxy with a peculiar blue core
• Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology
• HST Grism Confirmation of Two $z\sim 2$ Structures from the Clusters Around Radio-Loud AGN (CARLA) Survey
• $\gamma$ Parameter and Solar System constraint in Chameleon Brans Dick Theory
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Phantom cosmology in an Extended Theory of Gravity
• Ultraluminous Infrared Galaxies in the AKARI All Sky Survey
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Search for high-amplitude Delta Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis
• Bouncing Universe and Reconstructing Vector Field
• Statefinder Parameters for Interacting Phantom Energy with Dark Matter
• Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE
• Constraints on the End of Reionization from the Density Fields Surrounding Two Highly Opaque Quasar Sightlines
• Chandra Observations of 12 Luminous Red Quasars
• Dark and Baryonic Matter in Bright Spiral Galaxies: I.Near-infrared and Optical Broadband Surface Photometry of 30 Galaxies
• ROXA: a new multi-frequency selected large sample of blazars with SDSS and 2dF optical spectroscopy
• The Environment of Active Galaxies in the SDSS-DR4
• Cosmic Behavior, Statefinder Diagnostic and $w-w^{\prime }$ Analysis for Interacting NADE model in Non-flat Universe
• Metal Abundances of KISS Galaxies. VI. New Metallicity Relations for the KISS Sample of Star-Forming Galaxies
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Discovery of Four Gravitationally Lensed Quasars from the Sloan Digital Sky Survey
• D-term chaotic inflation in supergravity
• Dynamics of holographic vacuum energy in the DGP model
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• A Photometric Metallicity Estimate of the Virgo Stellar Overdensity
• Velocities from Cross-Correlation: A Guide for Self-Improvement
• SDSSJ102111.02+491330.4: A Newly Discovered Gravitationally Lensed Quasar
• Couplings between holographic dark energy and dark matter
• Broadband Optical Properties of Massive Galaxies: the Dispersion Around the Field Galaxy Color-Magnitude Relation Out to z~0.4
• Chaotic universe model: Lotka-Volterra dynamics of the universe evolution
• J-PLUS: On the identification of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs
• Background-Source Separation in astronomical images with Bayesian probability theory (I): the method
• Spectrophotometric properties of galaxies at intermediate redshifts (z ~ 0.2--1.0) I. Sample description, photometric properties and spectral measurements
• The effect of FIR emission from SDSS galaxies on the SFD Galactic extinction map
• Merging Galaxy Cluster Abell 2255 in Mid-Infrared
• Revisiting the role of bars in AGN fuelling with propensity score sample matching
• Enhanced X-ray Emission from the Most Radio-Powerful Quasar in the Universe's First Billion Years
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. II. Faint end color-magnitude diagrams and radial profiles of red and blue galaxies at $0.1<z<1.1$
• The amazing diversity in the hot gas content of an X-ray unbiased massive galaxy clusters sample
• Spectrophotometric properties of galaxies at intermediate redshifts (z ~ 0.2--1.0) II. The Luminosity -- Metallicity relation
• Maximum Likelihood Fitting of Tidal Streams With Application to the Sagittarius Dwarf Tidal Tails
• Constraining the Galactic structure parameters with the XSTPS-GAC and SDSS photometric surveys
• Photometric properties and luminosity function of nearby massive early-type galaxies
• The close pair fraction of BCGs since $z=0.5$: major mergers dominate recent BCG stellar mass growth
• Precision Spectrophotometry at the Level of 0.1%
• Reconstruction of modified gravity with ghost dark energy models
• Optical imaging for the Spitzer Survey of Stellar Structure in Galaxies. Data release and notes on interacting galaxies
• Two New Gravitationally Lensed Double Quasars from the Sloan Digital Sky Survey
• VLBA Imaging Polarimetry of Active Galactic Nuclei - An Automated Approach
• Spectroscopic Survey of 1.4 GHz and 24 Micron Sources in the Spitzer First Look Survey with WIYN/Hydra
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Toward Understanding Environmental Effects in SDSS Clusters
• The Optical and Near-Infrared Properties of 2837 Quasars in the UKIRT Infrared Deep Sky Survey (UKIDSS)
• Correlations among the properties of galaxies found in a blind HI survey, which also have SDSS optical data
• SEGUE-2 Limits on Metal-Rich Old-Population Hypervelocity Stars In the Galactic Halo
• The stellar halo of the Milky Way traced by blue horizontal-branch stars in the Subaru Hyper Suprime-Cam Survey
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• SDSS J1130+0058 an X-shaped Radio Source With Double-Peaked Low-Ionization Emission Lines: A binary Black Hole System?
• Reconstructing the potentials for the quintessence and tachyon dark energy, from the holographic principle
• Small- and Large-Scale Galactic Conformity in SDSS DR7
• A Nearby Old Halo White Dwarf Candidate from the Sloan Digital Sky Survey
• The gas-phase metallicities of star-forming galaxies in aperture-matched SDSS samples follow potential rather than mass or average surface density
• Discovery of a Gravitationally Lensed Quasar from the Sloan Digital Sky Survey: SDSS J133222.62+034739.9
• Tolman IV fluid sphere in f(R, T) gravity
• Properties of Disks and Bulges of Spiral and Lenticular Galaxies in the Sloan Digital Sky Survey
• The RASS--6dFGS catalogue: a sample of X-ray selected AGN from the 6dF Galaxy Survey
• Characterisation of Sloan Digital Sky Survey Stellar Photometry
• Brane inflation driven by noncanonical scalar field
• Variegate galaxy cluster gas content: Mean fraction, scatter, selection effects and covariance with X-ray luminosity
• EMPRESS. VII. Ionizing Spectrum Shapes of Extremely Metal-Poor Galaxies: Uncovering the Origins of Strong HeII and the Impact on Cosmic Reionization
• Dependence of Galaxy Shape on Environment in the Sloan Digital Sky Survey
• Polarimetry of optically selected BL Lac candidates from the SDSS
• Optical properties of infrared-bright dust-obscured galaxies viewed with Subaru Hyper Suprime-Cam
• Fourier Phase Analysis of SDSS Galaxies
• Luminous Red Galaxy Population in Clusters at $0.2\le z\le 0.6$
• A map-based method for eliminating systematic modes from galaxy clustering power spectra with application to BOSS
• E+A and Companion Galaxies - I : A Catalogue and Statistics
• Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z=2.26 Galaxy SDSS J0901+1814
• Automated Morphological Classification of SDSS Red Sequence Galaxies
• Inflation from D3-brane motion in the background of D5-branes
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Ultracompact Blue Dwarf Galaxies: Hubble Space Telescope Imaging and Stellar Population Analysis
• Molecular gas filaments and star-forming knots beneath an X-ray cavity in RXC J1504-0248
• Interacting Dark Energy in Hořava-Lifshitz Cosmology
• Reconstructing a String-Inspired Non-minimally Coupled Quintom Model
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Spatial Variations of Galaxy Number Counts in the Sloan Digital Sky Survey. II. Test of Galactic Extinction in High Extinction Regions
• From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
• The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies
• A Chandra observation of the z=2.285 galaxy FSC10214+4724: Evidence for a Compton-thick quasar?
• Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
• The importance of interloper removal in galaxy clusters: saving more objects for the Jeans analysis
• Wide-Field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-ray Observations
• The Milky Way's stellar halo - lumpy or triaxial?
• A Catalog of Luminous Infrared Galaxies in the IRAS Survey and the Second Data Release of the SDSS
• Black-hole mass estimates for a homogeneous sample of bright flat-spectrum radio quasars
• A Realistic Particle Physics Dark Energy Model
• Galactic conformity measured in semi-analytic models
• Black hole and holographic dark energy
• Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields
• Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
• Optical and Infrared Diagnostics of SDSS galaxies in the SWIRE Survey
• Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
• Candidate spectroscopic binaries in the Sloan Digital Sky Survey
• Carbon-enhanced Metal-poor Stars in SDSS/SEGUE. II. Comparison of CEMP Star Frequencies with Binary Population Synthesis Models
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Noether Gauge Symmetry of Modified Teleparallel Gravity Minimally Coupled with a Canonical Scalar Field
• The Snapshot Hubble U-Band Cluster Survey (SHUCS). I. Survey Description and First Application to the Mixed Star Cluster Population of NGC 4041
• A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• The Sloan Nearby Cluster Weak Lensing Survey
• The white dwarf luminosity function. I. Statistical errors and alternatives
• New holographic dark energy model with non-linear interaction
• Statefinder Analysis of Symmetric Teleparallel Cosmology
• Intracluster Light Properties in a Fossil Cluster at z=0.47
• Cosmic Dynamics in $F(R,\varphi )$ Gravity
• Measurement of the integrated Sachs-Wolfe effect using the AllWISE data release
• The Century Survey Galactic Halo Project II: Global Properties and the Luminosity Function of Field Blue Horizontal Branch Stars
• The Combined NVSS-FIRST Galaxies (CoNFIG) Sample - I. Sample Definition, Classification and Evolution
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Estimation of Absolute Magnitude-dependent Galactic Model Parameters In Intermediate Latitude With SDSS and SCUSS
• Automated Classification of Sloan Digital Sky Survey (SDSS) Stellar Spectra using Artificial Neural Networks
• XMM-Newton Observations of the Extremely Low Accretion Rate Polars SDSSJ15531.12+551614.5 and SDSSJ132411.57+032050.5
• Two novel approaches for photometric redshift estimation based on SDSS and 2MASS databases
• Kernel Regression For Determining Photometric Redshifts From Sloan Broadband Photometry
• Identifying Tidal Disruption Events via Prior Photometric Selection of Their Preferred Hosts
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Distant Field BHB Stars III: Identification of a probable outer halo stream at Galactocentric distance r = 70 kpc
• Fixed points and FLRW cosmologies: Flat case
• The Transparency of Galaxy Clusters
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• Fossil Group Origins VII. Galaxy substructures in fossil systems
• Seeing in the dark -- I. Multi-epoch alchemy
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• HI Selected Galaxies in the Sloan Digital Sky Survey II: The Colors of Gas-Rich Galaxies
• The faint-end of the galaxy luminosity function in groups
• Statefinder and Om Diagnostics for Interacting New Holographic Dark Energy Model and Generalized Second Law of Thermodynamics
• Towards a fully consistent Milky Way disc model - II. The local disc model and SDSS data of the NGP region
• A Dyson Sphere around a black hole
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Variability of Moderate Luminosity Active Galactic Nuclei at z=0.36
• A Massive Field-Theoretic Model for Hodge Theory
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Dynamics of an Anisotropic Universe in $f(R,T)$ Theory
• The 3-D clustering of radio galaxies in the TONS survey
• Bianchi type-I Dust Filled Accelerating Brans- Dicke Cosmology
• Learning from the machine: interpreting machine learning algorithms for point- and extended- source classification
• Young stellar populations in type II quasars: timing the onset of star formation and nuclear activity
• Optical multiband surface photometry of a sample of Seyfert galaxies. I. Large-scale morphology and local environment analysis of matched Seyfert and inactive galaxy samples
• GMOS Integral Field Spectroscopy of a Merging System with Enhanced Balmer Absorption
• The Circumnuclear Star-forming Activities along the Hubble Sequence
• Abell 2111: An Optical and Radio Study of the Richest Butcher-Oemler Cluster
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• Holographic interacting dark energy in the braneworld cosmology
• The Power of Simultaneous Multi-frequency Observations for mm-VLBI: Beyond Frequency Phase Transfer
• Deep GALEX Observations of the Coma Cluster: Source Catalog and Galaxy Counts
• A New Type of Dark Energy Model
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Discovery of Four Doubly Imaged Quasar Lenses from the Sloan Digital Sky Survey
• The Faint End Slopes Of Galaxy Luminosity Functions In The COSMOS 2-Square Degree Field
• 4C02.27: a quasar with episodic activity?
• Morphology of Mock SDSS Catalogues
• Atomic and Molecular Absorption in Redshifted Radio Sources
• Effects of galaxy environment on merger fraction
• Perturbations for transient acceleration
• Large-scale anomalies of the CMB in the curvaton scenario
• Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). III. Discovery of a z = 4.72 Radio Galaxy with Lyman Break Technique
• The orientation of the nuclear obscurer of the AGNs
• On a phenomenology of the accelerated expansion with a varying ghost dark energy
• Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture
• Bouncing Universe with Non-minimally Coupled Quintom Matter
• Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems
• Improved photometry of SDSS crowded field images: Structure and dark matter content in the dwarf spheroidal galaxy Leo I
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• Nuclear vs. Integrated Spectroscopy of Galaxies in the Herschel Reference Survey
• Bianchi Type-I Universe Models with Nonlinear Viscosity
• Four Faint T Dwarfs from the UKIRT Infrared Deep Sky Survey (UKIDSS) Southern Stripe
• Nature and completeness of galaxies detected in the Two Micron All Sky Survey
• The interacting galaxy pair KPG 390: H$\alpha$ kinematics
• Color, Structure, and Star Formation History of Dwarf Galaxies over the last ~3 Gyr with GEMS and SDSS
• The Color Selection of Quasars from Redshifts 5 to 10: Cloning and Discovery
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• Morphological Dependence of Star Formation Properties for the Galaxies in the Merging Galaxy Cluster A2255
• Spatially resolved emission lines in galaxies at $4\le z<10$ from the JADES survey: evidence for enhanced central star formation
• Photometric Metallicity Calibration with SDSS and SCUSS and its Application to distant stars in the South Galactic Cap
• Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
• Logarithmic entropy corrected holographic dark energy with $F(R,T)$ gravity
• Photometric Biases in Modern Surveys
• Pulling out Threads from the Cosmic Tapestry: Defining Filaments of Galaxies
• Deep Extragalactic VLBI-Optical Survey (DEVOS): I. Pilot MERLIN and VLBI observations
• A Dynamical Analysis of the Corona Borealis Supercluster
• Continuum optical-UV and X-ray variability of AGN: current results and future challenges
• Magnitude and size evolution of bulgeless galaxies
• Asteroid Distributions in the Ecliptic
• New active galactic nuclei detected in ROSAT All Sky Survey galaxies - The complete dataset
• Early Science Result from the Japanese Virtual Observatory: AGN and Galaxy Clustering at z = 0.3 to 3.0
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Ionized Gas Outflows in Low Excitation Radio Galaxies Are Radiation Driven
• Looking at quasars through galaxies
• The luminosity bias relation from filaments in the Sloan Digital Sky Survey Data Release Four
• Interacting Ghost Dark Energy in Complex Quintessence Theory
• How accurate is our knowledge of galaxy bias?
• Revealing strong bias in common measures of galaxy properties using new inclination-independent structures
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Stable Large-Scale Perturbations in Interacting Dark-Energy Model
• Compact groups from semi-analytical models of galaxy formation -- I: a comparative study of frequency and nature
• Dynamical analysis of strong-lensing galaxy groups at intermediate redshift
• XMM-Newton and optical follow-up observations of three new polars from the Sloan Digital Sky Survey
• Inverse-Scattering Theory and the Density Perturbations from Inflation
• Spectral analyses of DO white dwarfs and PG1159 stars from the Sloan Digital Sky Survey
• Dynamical systems of cosmological models for different possibilities of $G$ and ${\rho }_{\Lambda }$
• Strong CaII absorption lines in the reddened quasar SDSS J2339$-$0912: Evidence of the collision/merger in the host galaxy?
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
• The Aromatic Features in Very Faint Dwarf Galaxies
• SDSS J210014.12+004446.0: A New Dwarf Nova with Quiescent Superhumps?
• Galaxy growth by merging in the nearby universe
• VLT/UVES Observation of the Outflow in Quasar SDSS J1439-0106
• Interacting holographic dark energy in the scalar-Gauss-Bonnet gravity
• A Search for Planetary Nebulae With the SDSS: the outer regions of M31
• A sample of metal-poor galaxies identified from the LAMOST spectral survey
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• Charged gravastar model in $f(T)$ gravity admitting conformal motion
• Observational constraints on the fractal cosmology
• Source Matching in the SDSS and RASS: Which Galaxies are Really X-ray Sources?
• Non-flat universe and interacting dark energy model
• A Systematic Survey for z < 0.04 Changing-Look AGNs
• Entropy and statefinder diagnosis in chameleon cosmology
• Generalized second law of thermodynamics in QCD ghost f(G) gravity
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z=0.3-1.4
• The color gradients of spiral disks in the Sloan Digital Sky Survey
• Determining the fraction of reddened quasars in COSMOS with multiple selection techniques from X-ray to radio wavelengths
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Understanding the chemical evolution of blue Edge-on Low Surface Brightness Galaxies
• SDSS J133401.39+331534.3: A New Subarcsecond Gravitationally Lensed Quasar
• Comparing the Host Galaxies of Type Ia, Type II and Type Ibc Supernovae
• Modeling and Analyzing Stability of Hybrid Stars within $f(Q)$ Gravity
• Edge-on disk galaxies in the SDSS DR6: Fractions of bulgeless and other disk galaxies
• Tachyon model of Tsallis holographic dark energy
• How to Detect Inclined Water Maser Disks (and Possibly Measure Black Hole Masses)
• On the holographic dark energy in chameleon scalar-tensor cosmology
• Interacting agegraphic dark energy models in phase space
• Stability analysis in Modified Non-Local Gravity
• Proper motion measurements for stars up to $100$ kpc with Subaru HSC and SDSS Stripe 82
• Disentangling the role of environmental processes in galaxy clusters
• The quasar-galaxy cross SDSS J1320+1644: A probable large-separation lensed quasar
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Particle creation in the framework of f(G) gravity
• First-order formalism for the quintom model of dark energy
• The metallicity evolution of blue compact dwarf galaxies from the intermediate redshift to the local Universe
• Bouncing cosmological models in a functional form of F(R) gravity
• SDSS J1553+0056: A BALQSO mimicking a Lyman-break galaxy
• On the stability of the dark energy based on generalized uncertainty principle
• Hα Dots: Direct-Method Metal Abundances of Low-Luminosity Star-Forming Systems
• Searches for Population III Pair-Instability Supernovae: Impact of Gravitational Lensing Magnification
• Star formation histories and evolution of 35 brightest E+A galaxies from SDSS DR5
• Inflation and New Agegraphic Dark Energy
• Current star formation in early-type galaxies and the K+A phenomenon
• Mapping the Milky Way with Gaia Bp/Rp spectra I: Systematic flux corrections and atmospheric parameters for 68 million stars
• Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ~ 4
• Age problem in holographic dark energy
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• UV to FIR catalogue of a galaxy sample in nearby clusters: SEDs and environmental trends
• Reconstruction of $f(R)$, $f(T)$ and $f(\mathcal{G})$ models inspired by variable deceleration parameter
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
• Compact radio emission from z~0.2 X-ray bright AGN
• Non-minimal coupling of the phantom field and cosmic acceleration
• On the limitations of statistical absorption studies with the Sloan Digital Sky Surveys I--III
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Bayesian bulge-disc decomposition of galaxy images
• Searching in HI for Massive Low Surface Brightness Galaxies: Samples from HyperLeda and the UGC
• The Way We Measure: Comparison of Methods to Derive Radial Surface Brightness Profiles
• Late cosmic acceleration in a vector--Gauss-Bonnet gravity model
• Particle creation in flat FRW Universe in the framework of $f(T)$ gravity
• Phase space analysis of some interacting Chaplygin gas models
• Effect of bulk viscosity in cosmic acceleration
• Predicting spectral features in galaxy spectra from broad-band photometry
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IX. The Most Overdense Region at z~5 Inhabited by a Massive Radio Galaxy
• The white dwarf luminosity function --II. The effect of the measurement errors and other biases
• Transformations between 2MASS, SDSS and BVI photometric systems for late-type giants
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• New holographic Chaplygin gas model of dark energy
• The architecture of Abell 1386 and its relationship to the Sloan Great Wall
• Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
• Stability analysis and observational constraints in scalar tensor theory
• SDSS Pre-Burst Observations of Recent Gamma-Ray Burst Fields
• X-ray Observations of Optically Selected Giant Elliptical-Dominated Galaxy Groups
• A Monte-Carlo Method for Estimating Stellar Photometric Metallicity Distributions
• Assembling a RELIC at Redshift 1: Spectroscopic Observations of Galaxies in the RELICS Cluster SPT-CLJ0615-5746
• The effect of supersymmetry breaking in the Mass Varying Neutrinos
• Search for extended Lyman-$\alpha$ emission around 9k quasars at z=2-3
• Checking the reliability of equivalent width R23 for estimating metallicities of galaxies
• Spatially Resolved Spectroscopic Observations of a Possible E+A Progenitor SDSS J160241.00+521426.9
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
• Phase structure of the $O(2)$ ghost model with higher-order gradient term
• Constraints on Holographic cosmologies from strong lensing systems
• Properties of optically selected BL Lac candidates from the SDSS
• SDSSJ103913.70+533029.7: A Super Star Cluster in the Outskirts of a Galaxy Merger
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Study of Some Cosmological Parameters for Interacting New Holographic Dark Energy Model in f(T) Gravity
• Observational constraints in scalar tensor theory with tachyonic potential
• The Tidal Tails of Globular Cluster Palomar 5 Based on Neural Networks Method
• On the Photometric Redshift Estimates for FR II Radio Galaxies
• The Effects of Tachyonic and Phantom Fields in the Intermediate and Logamediate Scenarios of the Anisotropic Universe
• An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
• Analysis of interacting and isolated quasars
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Stability of curvature perturbation with new covariant form for energy-momentum transfer in dark sector
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
• Inconsistences in Interacting Agegraphic Dark Energy Models
• Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature
• Constraints on scalar-tensor theories from observations
• Keck/Deimos Spectroscopy of a GALEX UV Selecte Sample from the Medium Imaging Survey
• Systematic Study of the Inner Structure of Molecular Tori in Nearby U/LIRGs using Velocity Decomposition of CO Rovibrational Absorption Lines
• Reconstructing f(R) model from Holographic DE: Using the observational evidence
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Theory of Cosmological Perturbations and Applications to Superstring Cosmology
• Where do X-ray low surface brightness clusters sit with respect to filaments?
• Boxy H$\alpha$ Emission Profiles in Star-Forming Galaxies
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• Star formation properties of galaxy cluster A1767
• Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Recalibration of SDSS photometric zero-points based on the InfraRed Flux Method temperature scale
• Semi-holographic model revisited
• Metallicity Dependent Transformations for Red Giants with Synthetic Colours of UBV and ugr
• On observational signatures of multi-fractional theory
• Late time attractors of some varying Chaplygin gas cosmological models
• Using the XMM Optical Monitor to Study Cluster Galaxy Evolution
• A Monte-Carlo Method for Making SDSS $u$-Band Magnitude more accurate
• Geometric and thermodynamic properties in Gauss-Bonnet gravity
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Photometric Selection of a Massive Galaxy Catalog with $z\ge 0.55$
• On Gauge Choice of Spherically Symmetric 3-Branes
• Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off
• HR-pyPopStar II: high spectral resolution evolutionary synthesis models low metallicity expansion and the properties of the stellar populations of dwarf galaxies
• Agegraphic Model based on the Generalized Uncertainty Principle
• High-energy Astrophysics and the Virtual Observatory
• Robust detection of CID double stars in SDSS
• Bouncing Cosmologies in modified gravity with space time torsion
• Galaxy disc central surface brightness distribution in the optical and near-infrared bands
• The cosmic environment overtakes the local density in shaping galaxy star formation
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• Do gas-poor galaxy clusters have different galaxy populations? The positive covariance of hot and cold baryons
• The influence of cosmological constant on light deflection in rotating spacetimes via the generalized Gibbons-Werner method
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data