Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies
Guillermo Barro,Guillermo Barro,S. M. Faber,David C. Koo,Avishai Dekel,Jerome J. Fang,Jonathan R. Trump,Pablo G. Pérez-González,Camilla Pacifici,Joel R. Primack,Rachel S. Somerville,Haojing Yan,Yicheng Guo,F. S. Liu,Daniel Ceverino,Dale D. Kocevski,Elizabeth J. McGrath +16 more
TLDR
In this article, the authors study the evolution of scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.Abstract:
We study the evolution of the scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.read more
Citations
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Improving galaxy morphologies for SDSS with Deep Learning
H. Domínguez Sánchez,H. Domínguez Sánchez,Marc Huertas-Company,Marc Huertas-Company,Marc Huertas-Company,Mariangela Bernardi,D Tuccillo,D Tuccillo,J. L. Fischer +8 more
TL;DR: A morphological catalogue for 670,000 galaxies in the Sloan Digital Sky Survey in two flavours: T-Type, related to the Hubble sequence, and Galaxy Zoo 2 (GZ2 hereafter) classification scheme, provided by combining accurate existing visual classification catalogues with machine learning.
Journal ArticleDOI
Star formation is boosted (and quenched) from the inside-out: radial star formation profiles from MaNGA
Sara L. Ellison,Sebastián F. Sánchez,Hector Ibarra-Medel,Braulio Antonio,Braulio Antonio,J. Trevor Mendel,Jorge K. Barrera-Ballesteros +6 more
TL;DR: In this paper, the authors investigated the SFR profiles of 864 galaxies as a function of their position relative to the global star forming main sequence (Delta SFR), and found that for quiescent/passive galaxies that lie at least a factor of 10 below the global main sequence, there is an analogous deficit of star formation throughout the galaxy with the lowest values of Delta Sigma_SFR in the central 3 kpc.
Journal ArticleDOI
Effect of local environment and stellar mass on galaxy quenching and morphology at 0.5 < z < 2.0
Lalitwadee Kawinwanichakij,Casey Papovich,Ryan Quadri,Karl Glazebrook,Glenn G. Kacprzak,Rebecca Allen,Eric F. Bell,Darren J. Croton,Avishai Dekel,Henry C. Ferguson,Ben Forrest,Norman A. Grogin,Yicheng Guo,Dale D. Kocevski,Anton M. Koekemoer,Ivo Labbé,Ray A. Lucas,Themiya Nanayakkara,Themiya Nanayakkara,Lee R. Spitler,Lee R. Spitler,Caroline M. S. Straatman,Kim-Vy Tran,Adam Tomczak,Pieter G. van Dokkum +24 more
TL;DR: In this paper, the authors studied galactic star-formation activity as a function of environment and stellar mass over 0.5 9 (9.5) and showed that the effects of quenching related to stellar mass and environment are not separable.
Journal ArticleDOI
Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
Sandro Tacchella,Benedikt Diemer,Lars Hernquist,Shy Genel,Shy Genel,Federico Marinacci,Dylan Nelson,Annalisa Pillepich,Vicente Rodriguez-Gomez,Laura V. Sales,Volker Springel,Mark Vogelsberger +11 more
TL;DR: In this paper, a kinematical decomposition of the stellar component into a spheroidal and a disc component (spheroid-to-total ratio, S/T) and the concentration of stellar mass density profile (C_{82}$) was proposed to quantify the relationship between galaxy morphology and star formation.
Journal ArticleDOI
Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ∼ 2
References
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Journal ArticleDOI
A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
Joshua S. Speagle,Joshua S. Speagle,Charles L. Steinhardt,Charles L. Steinhardt,Peter Capak,John D. Silverman +5 more
TL;DR: In this article, the authors investigate the evolution of the star-forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out to z ~ 6.4 Gyr.
Journal ArticleDOI
Galactic star formation and accretion histories from matching galaxies to dark matter haloes
TL;DR: In this article, a multi-epoch abundance matching (MEAM) model was proposed to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z � 4 to the present.
Journal ArticleDOI
Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust-enshrouded Star Formation Rate
Ranga-Ram Chary,David Elbaz +1 more
TL;DR: In this article, the evolution of the mid-infrared local luminosity function with redshift to the spectrum of the cosmic infrared background (CIRB) at j[ 5 km and the galaxy counts from various surveys at midinfrared, far infrared, and submillimeter wavelengths was investigated.
Journal ArticleDOI
GOODS–Herschel: an infrared main sequence for star-forming galaxies
David Elbaz,Mark Dickinson,Ho Seong Hwang,Tanio Díaz-Santos,Georgios E. Magdis,Benjamin Magnelli,D. Le Borgne,Frédéric Galliano,Maurilio Pannella,P. Chanial,Lee Armus,Vassilis Charmandaris,Vassilis Charmandaris,Emanuele Daddi,Herve Aussel,P. Popesso,Jeyhan S. Kartaltepe,Bruno Altieri,Ivan Valtchanov,D. Coia,Helmut Dannerbauer,Kalliopi Dasyra,Roger Leiton,Roger Leiton,Joseph M. Mazzarella,David M. Alexander,V. Buat,Denis Burgarella,R.-R. Chary,Roberto Gilli,Rob Ivison,Rob Ivison,Stéphanie Juneau,E. Le Floc'h,Dieter Lutz,G. E. Morrison,James Mullaney,Eric J. Murphy,Alexandra Pope,Douglas Scott,Mark Brodwin,Daniela Calzetti,C. Cesarsky,Stéphane Charlot,Herve Dole,Peter Eisenhardt,Henry C. Ferguson,N. M. Förster Schreiber,Dave Frayer,Mauro Giavalisco,Minh Huynh,Anton M. Koekemoer,Casey Papovich,Naveen A. Reddy,Christian Surace,Harry I. Teplitz,Min S. Yun,G. W. Wilson +57 more
TL;DR: In this paper, the authors examined the infrared (IR) 3-500μm spectral energy distributions (SEDs) of galaxies at 0 < z < 2.5, supplemented by a local reference sample from IRAS, ISO, Spitzer, and AKARI data.
Journal ArticleDOI
GOODS-Herschel: an infrared main sequence for star-forming galaxies
David Elbaz,Mark Dickinson,Ho Seong Hwang,Tanio Díaz-Santos,Georgios E. Magdis,Benjamin Magnelli,D. Le Borgne,Frédéric Galliano,Maurilio Pannella,P. Chanial,Lee Armus,Vassilis Charmandaris,Emanuele Daddi,Herve Aussel,P. Popesso,Jeyhan S. Kartaltepe,Bruno Altieri,Ivan Valtchanov,D. Coia,Helmut Dannerbauer,Kalliopi Dasyra,Roger Leiton,Joseph M. Mazzarella,V. Buat,Denis Burgarella,Roberto Gilli,Rob Ivison,Stéphanie Juneau,E. LeFloch,Dieter Lutz,G. E. Morrison,James Mullaney,Eric J. Murphy,Alexandra Pope,Douglas Scott,David M. Alexander,Mark Brodwin,Daniela Calzetti,C. J. Cesarsky,Stéphane Charlot,H. Dole,Peter Eisenhardt,Henry C. Ferguson,N. Foerster-Schreiber,Dave Frayer,Mauro Giavalisco,Minh Huynh,Anton M. Koekemoer,Casey Papovich,Naveen A. Reddy,Christian Surace,Harry Teplitz,Min S. Yun,G. W. Wilson +53 more
TL;DR: In this article, deep far-IR observations obtained with Herschel and examined the 3-500um SEDs of galaxies at 0 3x10^10 Lsun kpc^-2 and a high specific SFR (i.e., SBs).
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