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A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy
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October 2019 |
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SciPy 1.0: fundamental algorithms for scientific computing in Python
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February 2020 |
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Astropy: A community Python package for astronomy
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September 2013 |
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A large sample of Kohonen selected E+A (post-starburst) galaxies from the Sloan Digital Sky Survey
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January 2017 |
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Planck 2018 results: VI. Cosmological parameters
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September 2020 |
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The first catalogue of spectroscopically confirmed red nuggets at z ∼ 0.7 from the VIPERS survey
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January 2023 |
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From VIPERS to SDSS: Unveiling galaxy spectra evolution over 9 Gyr through unsupervised machine learning
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June 2024 |
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SExtractor: Software for source extraction
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Spectroscopy of galaxies in distant clusters. II - The population of the 3C 295 cluster
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The Environment of ``E+A'' Galaxies
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Differential Galaxy Evolution in Cluster and Field Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z\approx 0.3$ \end{document}
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December 1999 |
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Galactic Stellar and Substellar Initial Mass Function
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July 2003 |
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Black Holes in Galaxy Mergers: Evolution of Quasars
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September 2005 |
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The Discovery of 1000 km s[FORMULA][F][SUP]-1[/SUP][/F][/FORMULA] Outflows in Massive Poststarburst Galaxies at [FORMULA][F]z=0.6[/F][/FORMULA]
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June 2007 |
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A Cosmological Framework for the Co‐evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. I. Galaxy Mergers and Quasar Activity
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April 2008 |
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Structure and Star Formation in Galaxies out to z = 3: Evidence for Surface Density Dependent Evolution and Upsizing
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December 2008 |
emcee : The MCMC Hammer
- Foreman-Mackey, Daniel; Hogg, David W.; Lang, Dustin
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Publications of the Astronomical Society of the Pacific, Vol. 125, Issue 925
https://doi.org/10.1086/670067
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March 2013 |
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Detailed Decomposition of Galaxy Images. ii. Beyond Axisymmetric Models
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April 2010 |
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The Relation Between Compact, Quiescent High-Redshift Galaxies and Massive Nearby Elliptical Galaxies: Evidence for Hierarchical, Inside-Out Growth
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May 2009 |
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Morphological Quenching of star Formation: Making Early-Type Galaxies red
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November 2009 |
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THE GROWTH OF MASSIVE GALAXIES SINCE z = 2
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January 2010 |
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The two Phases of Galaxy Formation
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December 2010 |
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GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR-MASS PLANE FROM z ∼ 2.5 TO z ∼ 0.1
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November 2011 |
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A LARGE POPULATION OF MASSIVE COMPACT POST-STARBURST GALAXIES AT z > 1: IMPLICATIONS FOR THE SIZE EVOLUTION AND QUENCHING MECHANISM OF QUIESCENT GALAXIES
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January 2012 |
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Can Minor Merging Account for the size Growth of Quiescent Galaxies? new Results from the Candels Survey
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February 2012 |
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SIZES AND SURFACE BRIGHTNESS PROFILES OF QUIESCENT GALAXIES AT z ∼ 2
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March 2012 |
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CANDELS: THE PROGENITORS OF COMPACT QUIESCENT GALAXIES AT z ∼ 2
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February 2013 |
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A link Between star Formation Quenching and Inner Stellar mass Density in Sloan Digital sky Survey Central Galaxies
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September 2013 |
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December 2013 |
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May 2014 |
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July 2014 |
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October 2014 |
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Discovery of Large Molecular gas Reservoirs in Post-Starburst Galaxies
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February 2015 |
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Forming Compact Massive Galaxies
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October 2015 |
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3D-HST: A WIDE-FIELD GRISM SPECTROSCOPIC SURVEY WITH THE HUBBLE SPACE TELESCOPE
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May 2012 |
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3d-Hst Wfc3-Selected Photometric Catalogs in the five Candels/3d-Hst Fields: Photometry, Photometric Redshifts, and Stellar Masses
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October 2014 |
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Project Overview of the Beijing–Arizona Sky Survey
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April 2017 |
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Evolution Through the Post-starburst Phase: Using Post-starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution
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July 2021 |
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THE STAR FORMATION MASS SEQUENCE OUT TO z = 2.5
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July 2012 |
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August 2012 |
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Geometry of Star-Forming Galaxies from Sdss, 3d-Hst, and Candels
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August 2014 |
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THE SIZES OF MASSIVE QUIESCENT AND STAR-FORMING GALAXIES AT z ∼ 4 WITH ZFOURGE AND CANDELS
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July 2015 |
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Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
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July 2020 |
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Comparison of stellar populations in simulated and real post-starburst galaxies in MaNGA
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August 2020 |
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From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
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April 2021 |
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October 2023 |
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INSPIRE: INvestigating Stellar Population In RElics – V. A catalogue of ultra-compact massive galaxies outside the local Universe and their degree of relicness
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November 2023 |
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Age and metal gradients in massive quiescent galaxies at 0.6 ≲ z ≲ 1.0: implications for quenching and assembly histories
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July 2024 |
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Wet disc contraction to galactic blue nuggets and quenching to red nuggets
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December 2013 |
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A new method for classifying galaxy SEDs from multiwavelength photometry
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March 2014 |
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Massive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activity
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June 2014 |
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The formation of massive, compact galaxies at z = 2 in the Illustris simulation
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March 2015 |
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Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets
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May 2015 |
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The evolution of post-starburst galaxies from z=2 to 0.5
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August 2016 |
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Evolution of density profiles in high- z galaxies: compaction and quenching inside-out
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February 2016 |
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Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at z < 1
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October 2017 |
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Massive post-starburst galaxies at z > 1 are compact proto-spheroids
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August 2017 |
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July 2018 |
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September 2019 |
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February 2014 |
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March 2005 |
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Physical Properties and Environments of Nearby Galaxies
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September 2009 |
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SEP: Source Extractor as a library
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October 2016 |
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pysersic: A Python package for determining galaxy structural properties via Bayesian inference, accelerated with jax
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September 2023 |
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LOW GAS FRACTIONS CONNECT COMPACT STAR-FORMING GALAXIES TO THEIR z ∼ 2 QUIESCENT DESCENDANTS
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November 2016 |
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December 2016 |
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The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package
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August 2018 |
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Overview of the DESI Legacy Imaging Surveys
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April 2019 |
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Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
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October 2022 |
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December 2022 |
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Target Selection and Validation of DESI Luminous Red Galaxies
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January 2023 |
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The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
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March 2023 |
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Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument
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July 2023 |
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Survey Operations for the Dark Energy Spectroscopic Instrument
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November 2023 |
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Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument
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January 2024 |
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The Early Data Release of the Dark Energy Spectroscopic Instrument
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July 2024 |
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The Optical Corrector for the Dark Energy Spectroscopic Instrument
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July 2024 |
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MOSFIRE SPECTROSCOPY OF QUIESCENT GALAXIES AT 1.5 < z < 2.5. I. EVOLUTION OF STRUCTURAL AND DYNAMICAL PROPERTIES
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December 2016 |
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Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2
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February 2017 |
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Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
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March 2017 |
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Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5
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March 2017 |
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Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
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May 2017 |
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Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs
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May 2018 |
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Fast and Slow Paths to Quiescence: Ages and Sizes of 400 Quiescent Galaxies from the LEGA-C Survey
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November 2018 |
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MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching
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March 2019 |
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Half-mass Radii for ∼7000 Galaxies at 1.0 ≤ z ≤ 2.5: Most of the Evolution in the Mass–Size Relation Is Due to Color Gradients
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May 2019 |
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An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D- HST Survey
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June 2019 |
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COSMOS-DASH: The Evolution of the Galaxy Size–Mass Relation since z ∼ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D- HST
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July 2019 |
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Evidence for Inside-out Galaxy Growth and Quenching of a z ∼ 2 Compact Galaxy From High-resolution Molecular Gas Imaging
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September 2019 |
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The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching
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January 2020 |
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SQuIGG E Survey: Massive z ∼ 0.6 Post-starburst Galaxies Exhibit Flat Age Gradients
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December 2020 |
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Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies
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December 2020 |
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April 2021 |
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Dissecting the Size–Mass and Σ 1 –Mass Relations at 1.0 < z < 2.5: Galaxy Mass Profiles and Color Gradients as a Function of Spectral Shape
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July 2021 |
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Searching for Local Counterparts of High-redshift Poststarburst Galaxies in Integral Field Unit Spectroscopic Surveys of Nearby Galaxies
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May 2021 |
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October 2021 |
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SQuIGGL⃗E : Studying Quenching in Intermediate-z Galaxies—Gas, AnguL⃗ar Momentum, and Evolution
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The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample
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The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package*
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August 2022 |
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Color Gradients and Half-mass Radii of Galaxies Out to z = 2 in the CANDELS/3D-HST Fields: Further Evidence for Important Differences in the Evolution of Mass-weighted and Light-weighted Sizes
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March 2023 |
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Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
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May 2023 |
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Extending the Dynamic Range of Galaxy Outflow Scaling Relations: Massive Compact Galaxies with Extreme Outflows
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July 2023 |
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August 2024 |
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The Size–Mass Relation at Rest-frame 1.5 μm from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS Fields
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Stellar Population Inference with Prospector
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May 2021 |
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Siena Galaxy Atlas 2020
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October 2023 |
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THE RELATION BETWEEN GALAXY STRUCTURE AND SPECTRAL TYPE: IMPLICATIONS FOR THE BUILDUP OF THE QUIESCENT GALAXY POPULATION AT 0.5 < z < 2.0
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January 2016 |
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Massive Quenched Galaxies at z ∼ 0.7 Retain Large Molecular Gas Reservoirs
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September 2017 |
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Stellar Metallicities and Elemental Abundance Ratios of z ∼ 1.4 Massive Quiescent Galaxies
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August 2019 |
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Half-mass Radii of Quiescent and Star-forming Galaxies Evolve Slowly from 0 ≲ z ≤ 2.5: Implications for Galaxy Assembly Histories
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October 2019 |
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Color Gradients along the Quiescent Galaxy Sequence: Clues to Quenching and Structural Growth
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August 2020 |
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DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at z ∼ 1
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April 2023 |
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Preliminary Target Selection for the DESI Luminous Red Galaxy (LRG) Sample
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October 2020 |
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astropy/photutils: 1.8.0
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software
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May 2023 |