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.
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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
SIZES AND SURFACE BRIGHTNESS PROFILES OF QUIESCENT GALAXIES AT z ∼ 2
TL;DR: In this paper, a stellar mass-limited sample of quiescent galaxies at 1.5 < z < 2.5 was used to measure surface brightness profiles for these galaxies using a method that properly measures low surface brightness flux at large radii.
Journal ArticleDOI
Dependence of galaxy quenching on halo mass and distance from its centre
Joanna Woo,Avishai Dekel,S. M. Faber,Kai G. Noeske,David C. Koo,Brian F. Gerke,Michael C. Cooper,Samir Salim,Aaron A. Dutton,Jeffrey A. Newman,Benjamin J. Weiner,Kevin Bundy,Christopher N. A. Willmer,Marc Davis,Renbin Yan +14 more
TL;DR: In this article, the dependence of star-formation quenching on galaxy mass and environment, in the SDSS (z~0.1) and the AEGIS (z-1) was studied.
Journal ArticleDOI
The dependence of quenching upon the inner structure of galaxies at 0.5 ≤ $z$ < 0.8 in the DEEP2/AEGIS survey
Edmond Cheung,S. M. Faber,David C. Koo,Aaron A. Dutton,Luc Simard,Elizabeth J. McGrath,J.-S. Huang,Eric F. Bell,Avishai Dekel,Jerome J. Fang,Samir Salim,Guillermo Barro,Kevin Bundy,Alison L. Coil,Michael C. Cooper,C. J. Conselice,Michael Davis,Aaron Dominguez,Susan A. Kassin,Dale D. Kocevski,Anton M. Koekemoer,Lihwai Lin,Jennifer M. Lotz,Jeffrey A. Newman,Andrew C. Phillips,David J. Rosario,Benjamin J. Weiner,Christopher N. A. Willmer +27 more
TL;DR: In this paper, the authors analyze the rest-frame U -B color correlations versus these structural parameters using a sample of galaxies in the redshift range 0.5 − 2.3.
Journal ArticleDOI
Radiative feedback and the low efficiency of galaxy formation in low-mass haloes at high redshift
Daniel Ceverino,Anatoly Klypin,Elizabeth S. Klimek,Sebastian Trujillo-Gomez,Christopher W. Churchill,Joel R. Primack,Avishai Dekel +6 more
TL;DR: In this article, the effect of radiation pressure in cosmological, zoom-in galaxy formation simulations is modeled as a non-thermal pressure that acts only in dense and optically thick star-forming regions.
Journal ArticleDOI
The Rise and Fall of Passive Disk Galaxies: Morphological Evolution Along the Red Sequence Revealed by COSMOS
Kevin Bundy,Claudia Scarlata,C. M. Carollo,Richard S. Ellis,Niv Drory,Philip F. Hopkins,Mara Salvato,Alexie Leauthaud,Alexie Leauthaud,Anton M. Koekemoer,Norman Murray,O. Ilbert,Pascal Oesch,Chung-Pei Ma,Peter Capak,Lucia Pozzetti,N. Z. Scoville +16 more
TL;DR: In this paper, the authors show that the correspondence between galaxy morphology and color is not perfect, providing insight into the physical origin of this evolution, and they estimate that as much as 60% of galaxies transitioning onto the red sequence evolve through a passive disk phase.
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