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The environmental dependence of the chemical properties of star-forming galaxies
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The Luminosity Dependence of the Galaxy Merger Rate
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Unravelling the cosmic web: an analysis of the Sloan Digital Sky Survey Data Release 14 with the local dimension
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March 2019 |
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Sloan Digital Sky Survey: Early Data Release
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January 2002 |
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Galaxy assembly bias on the red sequence
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March 2010 |
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The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters
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August 2002 |
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Formation of Massive Galaxies at high Redshift: cold Streams, Clumpy Disks, and Compact Spheroids
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September 2009 |
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Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
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September 2002 |
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Galaxy Correlations as a Function of Morphological Type
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August 1976 |
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Properties of gas phases around cosmic filaments atz= 0 in the IllustrisTNG simulation
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May 2021 |
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Impact of Cosmic Filaments on the Gas Accretion Rate of Dark Matter Halos
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January 2022 |
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Galaxy Zoo: the dependence of morphology and colour on environment
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March 2009 |
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Effects of galaxy interactions in different environments
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April 2006 |
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Can a conditioning on stellar mass explain the mutual information between morphology and environment?
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September 2020 |
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Tidally Triggered Star Formation in Close Pairs of Galaxies: Major and Minor Interactions
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June 2006 |
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TRIGGERED STAR FORMATION IN GALAXY PAIRS AT z = 0.08-0.38
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April 2010 |
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Galaxy Pairs in the Sloan Digital sky Survey. i. star Formation, Active Galactic Nucleus Fraction, and the Luminosity/Mass-Metallicity Relation
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April 2008 |
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Generating Hot Gas in Simulations of Disk-Galaxy Major Mergers
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April 2004 |
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Modelling feedback from stars and black holes in galaxy mergers
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Formation and rotation of disc galaxies with haloes
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November 1980 |
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An analytic model for the evolution of the stellar, gas and metal content of galaxies: An analytic model for galaxy evolution
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December 2011 |
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Quantifying the Bimodal Color‐Magnitude Distribution of Galaxies
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January 2004 |
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The Local Dimension: a method to quantify the Cosmic Web
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March 2009 |
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An EAGLE view of the missing baryons
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February 2021 |
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Interacting Galaxies in the A901/902 Supercluster with Stages
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October 2009 |
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Virial shocks in galactic haloes?
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October 2003 |
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Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
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October 2001 |
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The orientation of galaxy pairs with filamentary structures: dependence on morphology
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October 2018 |
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How filaments of galaxies are woven into the cosmic web
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April 1996 |
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Galaxy Star Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey
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February 2003 |
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Exploring galaxy colour in different environments of the cosmic web with SDSS
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September 2020 |
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Galaxy pairs in the 2dF survey - II. Effects of interactions on star formation in groups and clusters
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August 2004 |
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Galaxy pairs in the Sloan Digital Sky Survey - V. Tracing changes in star formation rate and metallicity out to separations of 80 kpc: Galaxy pairs in the Sloan Digital Sky Survey - V
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September 2012 |
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Galaxy Zoo: passive red spirals
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March 2010 |
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Strangulation in Galaxy Groups
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December 2007 |
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Galaxy pairs in the 2dF survey - I. Effects of interactions on star formation in the field
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December 2003 |
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Gas Regulation of Galaxies: the Evolution of the Cosmic Specific star Formation Rate, the Metallicity-Mass-Star-Formation rate Relation, and the Stellar Content of Halos
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July 2013 |
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Structure of superclusters and supercluster formation - III. Quantitative study of the Local Supercluster
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The evolution of disk galaxies and the origin of S0 galaxies
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Morphological Transformation from Galaxy Harassment
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Are cosmological gas accretion streams multiphase and turbulent?
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February 2018 |
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Morphological Quenching of star Formation: Making Early-Type Galaxies red
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November 2009 |
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On the fragmentation of cosmic gas clouds. I - The formation of galaxies and the first generation of stars
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Environmental Dependence of Properties of Galaxies in the Sloan Digital Sky Survey
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April 2007 |
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Galaxy pairs align with Galactic filaments
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On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback from Momentum‐driven Winds
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January 2005 |
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Star formation in galaxies falling into clusters along supercluster-scale filaments
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June 2008 |
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A method for classification of red, blue, and green galaxies using fuzzy set theory
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September 2020 |
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Clusters and superclusters in the Sloan Digital Sky Survey
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June 2003 |
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The SAURON project--V. Integral-field emission-line kinematics of 48 elliptical and lenticular galaxies
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March 2006 |
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Cooling, dynamics and fragmentation of massive gas clouds: clues to the masses and radii of galaxies and clusters
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August 1977 |
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How much a galaxy knows about its large-scale environment?: An information theoretic perspective
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December 2016 |
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Parametric Recovery of Line‐of‐Sight Velocity Distributions from Absorption‐Line Spectra of Galaxies via Penalized Likelihood
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February 2004 |
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The Propagation of Uncertainties in Stellar Population Synthesis Modeling. i. the Relevance of Uncertain Aspects of Stellar Evolution and the Initial mass Function to the Derived Physical Properties of Galaxies
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June 2009 |
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On the evolution and environmental dependence of the star formation rate versus stellar mass relation since z ∼ 2
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July 2013 |
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Semi-analytic modelling of galaxy formation: the local Universe
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December 1999 |
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Isolating Triggered Star Formation
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December 2007 |
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The Origin of Star Formation Gradients in Rich Galaxy Clusters
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Core radius and density measurements in N-body experiments Connections with theoretical and observational definitions
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The Coma/A1367 supercluster and its environs
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Planck 2018 results: VI. Cosmological parameters
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The hα Galaxy Survey. Viii. Close Companions and Interactions, and the Definition of Starbursts
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June 2009 |
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The Systematic Properties of Clusters of Galaxies. Photometry of 15 Clusters
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Galaxy morphology in rich clusters - Implications for the formation and evolution of galaxies
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March 1980 |
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How is star formation quenched in massive galaxies?: Star formation quenching
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June 2010 |
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Galaxy bimodality due to cold flows and shock heating
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May 2006 |
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The 2dF Galaxy Redshift Survey: spectra and redshifts
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December 2001 |
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Minor Galaxy Interactions: Star Formation Rates and Galaxy Properties
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June 2007 |
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Galaxy pairs in the Sloan Digital Sky Survey - III. Evidence of induced star formation from optical colours: Galaxy pairs in the SDSS - III
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January 2011 |
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Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
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July 1978 |
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Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five
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June 2008 |
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The luminosity, colour and morphology dependence of galaxy filaments in the Sloan Digital Sky Survey Data Release Four
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October 2006 |
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LESS THAN 10 PERCENT OF STAR FORMATION IN z ∼ 0.6 MASSIVE GALAXIES IS TRIGGERED BY MAJOR INTERACTIONS
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September 2009 |
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How do galaxies get their gas?
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October 2005 |
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Redshift‐Space Distortions and the Real‐Space Clustering of Different Galaxy Types
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November 1997 |
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Disc growth and quenching
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October 2019 |
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Galaxy harassment and the evolution of clusters of galaxies
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The Broadband Optical Properties of Galaxies with Redshifts 0.02 < z < 0.22
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September 2003 |
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The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies: Galaxy structure, star formation and nuclear activity
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August 2004 |
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The morphology-density relation in the Sloan Digital Sky Survey: Morphology-density relation in the SDSS
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November 2003 |
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Structure of superclusters and supercluster formation
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November 1980 |
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Galaxy evolution in cosmological simulations with outflows - II. Metallicities and gas fractions: Galaxy evolution in simulations - II
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July 2011 |
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The Overdensities of Galaxy Environments as a Function of Luminosity and Color
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March 2003 |
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Galaxy Clustering in Early Sloan Digital Sky Survey Redshift Data
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May 2002 |
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Star formation in close pairs selected from the Sloan Digital Sky Survey
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December 2004 |
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A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
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August 2020 |
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The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
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June 2020 |
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Galaxy pairs in the Sloan Digital Sky Survey - II. The effect of environment on interactions: Galaxy pairs in the Sloan Digital Sky Survey
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July 2010 |
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Tidally Triggered Star Formation in Close Pairs of Galaxies
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February 2000 |
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On the Infall of Matter Into Clusters of Galaxies and Some Effects on Their Evolution
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August 1972 |