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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LOW GAS FRACTIONS CONNECT COMPACT STAR-FORMING GALAXIES TO THEIR z ∼ 2 QUIESCENT DESCENDANTS
Justin Spilker,Rachel Bezanson,Daniel P. Marrone,Benjamin J. Weiner,Katherine E. Whitaker,Christina C. Williams +5 more
TL;DR: In this paper, the authors proposed a method to use the NIRCam NIR system to detect the presence of a single photon in the image of the Space Telescope Science Institute (SSI).
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The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0
Gergö Popping,Karina Caputi,Scott Trager,Rachel S. Somerville,Avishai Dekel,Susan A. Kassin,Dale D. Kocevski,Anton M. Koekemoer,S. M. Faber,Henry C. Ferguson,Audrey Galametz,Norman A. Grogin,Yicheng Guo,Yu Lu,A. van der Wel,Ben Weiner +15 more
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Stochastic modelling of star-formation histories I: the scatter of the star-forming main sequence
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Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at $z \sim 4.5$
Carlos Gómez-Guijarro,S. Toft,Alexander Karim,Benjamin Magnelli,Georgios E. Magdis,E. F. Jiménez-Andrade,Peter Capak,Filippo Fraternali,Seiji Fujimoto,Dominik Riechers,Eva Schinnerer,V. Smolcic,Manuel Aravena,Frank Bertoldi,Isabella Cortzen,G. Hasinger,Esther M. Hu,G. C. Jones,Anton M. Koekemoer,N. Lee,H. J. McCracken,Michał J. Michałowski,F. Navarrete,Mirjana Pović,Alfio Puglisi,Emilio Romano-Diaz,Kartik Sheth,John D. Silverman,Johannes Staguhn,Charles L. Steinhardt,Mikkel Stockmann,Mikito Tanaka,Francesco Valentino,E. van Kampen,Andrew Zirm +34 more
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MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5
Rhythm Shimakawa,Tadayuki Kodama,Masao Hayashi,J. Xavier Prochaska,Ichi Tanaka,Zheng Cai,Tomoko L. Suzuki,Ken-ichi Tadaki,Yusei Koyama +8 more
TL;DR: In this article, the authors carried out deep H$\alpha$ narrowband imaging with 10 hours net integrations towards the young protocluster, USS1558$-$003 at $z=2.53$ with the Subaru Telescope.
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