3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE–MASS DISTRIBUTION SINCE z = 3
A. van der Wel,Marijn Franx,P. G. van Dokkum,Rosalind E. Skelton,Ivelina Momcheva,Katherine E. Whitaker,Gabriel B. Brammer,Eric F. Bell,Hans-Walter Rix,Stijn Wuyts,Henry C. Ferguson,Bradford P. Holden,Guillermo Barro,Anton M. Koekemoer,Yu-Yen Chang,Elizabeth J. McGrath,B. Haussler,B. Haussler,Avishai Dekel,Peter Behroozi,Michele Fumagalli,Joel Leja,Britt Lundgren,Michael V. Maseda,Erica J. Nelson,David A. Wake,David A. Wake,Shannon G. Patel,Ivo Labbé,Sandra M. Faber,Norman A. Grogin,Dale D. Kocevski +31 more
TLDR
In this paper, the galaxy size-mass distribution over the redshift range 0 3 × 10{sup 9} M {sub ☉}, and steep, R{sub eff}∝M{sub ∗}{sup 0.75}, for early-type galaxies with stellar mass > 2 × 10,sup 10} M{sub ǫ, and the intrinsic scattermore is ≲0.2 dex for all galaxy types and redshifts.Abstract:
Spectroscopic+photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging to determine the galaxy size-mass distribution over the redshift range 0 3 × 10{sup 9} M {sub ☉}, and steep, R{sub eff}∝M{sub ∗}{sup 0.75}, for early-type galaxies with stellar mass >2 × 10{sup 10} M {sub ☉}. The intrinsic scattermore » is ≲0.2 dex for all galaxy types and redshifts. For late-type galaxies, the logarithmic size distribution is not symmetric but is skewed toward small sizes: at all redshifts and masses, a tail of small late-type galaxies exists that overlaps in size with the early-type galaxy population. The number density of massive (∼10{sup 11} M {sub ☉}), compact (R {sub eff} < 2 kpc) early-type galaxies increases from z = 3 to z = 1.5-2 and then strongly decreases at later cosmic times.« lessread more
Citations
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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
Katherine E. Whitaker,Katherine E. Whitaker,Rachel Bezanson,Rachel Bezanson,Pieter G. van Dokkum,Marijn Franx,Arjen van der Wel,Gabriel B. Brammer,Natascha M. Förster-Schreiber,Mauro Giavalisco,Ivo Labbe,Ivelina Momcheva,Erica J. Nelson,Rosalind E. Skelton +13 more
TL;DR: In this paper, the authors investigated the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at $0.5 $ 0.5 dex in the central density threshold correlated with quiescence from 0.7-2.0.
Journal ArticleDOI
GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
M. Franco,M. Franco,David Elbaz,L. Zhou,L. Zhou,Benjamin Magnelli,Corentin Schreiber,Laure Ciesla,Laure Ciesla,Mark Dickinson,Neil M. Nagar,Georgios E. Magdis,David M. Alexander,Matthieu Béthermin,Ricardo Demarco,E. Daddi,Tao Wang,Tao Wang,James Mullaney,Hanae Inami,Hanae Inami,Xinwen Shu,Frédéric Bournaud,Ranga-Ram Chary,R. T. Coogan,Henry C. Ferguson,Steven L. Finkelstein,Mauro Giavalisco,C. Gómez-Guijarro,Daisuke Iono,Daisuke Iono,Stéphanie Juneau,Guilaine Lagache,Lihwai Lin,Kentaro Motohara,Koryo Okumura,Maurilio Pannella,Maurilio Pannella,Casey Papovich,Alexandra Pope,Wiphu Rujopakarn,Wiphu Rujopakarn,Wiphu Rujopakarn,John D. Silverman,Mengyuan Xiao,Mengyuan Xiao +45 more
TL;DR: In this article, the presence of galaxies detected at 1.1 mm with ALMA below the original blind detection limit of 4.8-$\sigma was explored, where the number of spurious sources starts to dominate over that of real sources.
Journal ArticleDOI
Dust Temperature of Compact Star-forming Galaxies at $ z \sim 1-3$ in 3D-{\it HST}/CANDELS
TL;DR: In this article, the authors investigated the dependence of dust temperature on the size and star formation activity of compact star-forming galaxies (SFGs) and found that both extended and compact SFGs generally follow a similar dust-z$ evolutionary track as that of the main-sequence galaxies.
Journal ArticleDOI
An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
Caitlin M. Casey,Jacqueline Hodge,Jorge A. Zavala,Justin Spilker,Elisabete da Cunha,Johannes Staguhn,Steven L. Finkelstein,Patrick Drew +7 more
TL;DR: In this paper, the authors extend the backward evolution galaxy model described by Casey et al. to the ALMA regime (in depth and area) and determine that the measured number counts and redshift distributions from ALMA deep field surveys are fully consistent with constraints of the infrared luminosity function (IRLF) at $z 4 ).
Journal ArticleDOI
SQuIGG$\vec{L}$E Survey: Massive z$\sim$0.6 Post-Starburst Galaxies Exhibit Flat Age Gradients
David Setton,Rachel Bezanson,Katherine A. Suess,Qiana Hunt,Jenny E. Greene,Mariska Kriek,Justin Spilker,Robert Feldmann,Desika Narayanan +8 more
TL;DR: In this paper, the authors present Gemini GMOS IFU observations of six massive A-star dominated post-starburst galaxies at $z\sim 0.6$, which are a subsample of the SQuIGG$\vec{L}$E Survey.
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