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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Bulge formation by the coalescence of giant clumps in primordial disk galaxies
TL;DR: In this article, the observations and evolution of clumpy, high-redshift galaxies are reviewed and models suggest that the clumps form by gravitational instabilities in a gas-rich disk, interact with each other gravitationally, and then merge in the center where they form a bulge.
Journal ArticleDOI
RED NUGGETS AT z ∼ 1.5: COMPACT PASSIVE GALAXIES AND THE FORMATION OF THE KORMENDY RELATION
Ivana Damjanov,Patrick J. McCarthy,Roberto Abraham,Karl Glazebrook,Haojing Yan,Erin Mentuch,Damien Le Borgne,Sandra Savaglio,David Crampton,Richard Murowinski,Stéphanie Juneau,Raymond G. Carlberg,Inger Jorgensen,Kathy Roth,Hsiao-Wen Chen,Ronald O. Marzke +15 more
TL;DR: In this article, the authors presented the results of Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) imaging of a sample of 19 high-mass passively evolving galaxies with 1.2 < z < 2, taken primarily from the Gemini Deep Deep Survey (GDDS).
Journal ArticleDOI
A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation
Tomas Dahlen,Bahram Mobasher,Sandra M. Faber,Henry C. Ferguson,Guillermo Barro,Steven L. Finkelstein,Kristian Finlator,Adriano Fontana,Ruth Gruetzbauch,Seth Johnson,Janine Pforr,Mara Salvato,Tommy Wiklind,Stijn Wuyts,Viviana Acquaviva,Mark Dickinson,Yicheng Guo,Jiasheng Huang,Jiasheng Huang,Kuang-Han Huang,Jeffrey A. Newman,Eric F. Bell,Christopher J. Conselice,Audrey Galametz,Eric Gawiser,Mauro Giavalisco,Norman A. Grogin,Nimish P. Hathi,Dale D. Kocevski,Anton M. Koekemoer,David C. Koo,Kyoung-Soo Lee,Elizabeth J. McGrath,Casey Papovich,Michael Peth,Russell E. Ryan,Rachel S. Somerville,Benjamin J. Weiner,Grant W. Wilson +38 more
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Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies
Stijn Wuyts,Natascha M. Förster Schreiber,Reinhard Genzel,Yicheng Guo,Guillermo Barro,Eric F. Bell,Avishai Dekel,Sandra M. Faber,Henry C. Ferguson,Mauro Giavalisco,Norman A. Grogin,Nimish P. Hathi,Kuang-Han Huang,Dale D. Kocevski,Anton M. Koekemoer,David C. Koo,Jennifer M. Lotz,Dieter Lutz,Elizabeth J. McGrath,Jeffrey A. Newman,David J. Rosario,Amélie Saintonge,Linda J. Tacconi,Benjamin J. Weiner,Arjen van der Wel +24 more
TL;DR: In this article, the resolved colors and stellar populations of a complete sample of 323 star-forming galaxies (SFGs) at 0.5 < z < 1.5 and 326 SFGs at 1.1 < 2.5 in the ERS and CANDELS-Deep region of GOODS-South.
Journal ArticleDOI
The number density and mass density of star-forming and quiescent galaxies at 0.4 < z < 2.2
Gabriel B. Brammer,Katherine E. Whitaker,Pieter van Dokkum,Danilo Marchesini,Marijn Franx,Mariska Kriek,Ivo Labbé,Kyoung-Soo Lee,Adam Muzzin,Ryan Quadri,Gregory Rudnick,Rik J. Williams +11 more
TL;DR: In this paper, the build-up of the bimodal galaxy population using the NEWFIRM Medium-Band Survey was studied, which provides excellent redshifts and well-sampled spectral energy distributions of ~27,000 galaxies with K 3 10^11 solar masses.
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