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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A Cosmic Metamorphosis: The Quenching of Star-formation in Massive Galaxies Over the Last Eleven Billion Years
TL;DR: Van Dokkum et al. as mentioned in this paper studied the quenching of star-formation in massive galaxies over the last 11 billion years, using the Cosmic Dawn Center at the University of Connecticut.
Journal ArticleDOI
The puzzling origin of massive compact galaxies in MaNGA
Allan Schnorr-Müller,Marina Trevisan,R. A. Riffel,Ana L. Chies-Santos,Cristina Furlanetto,Tiago V. Ricci,F. S. Lohmann,R. Flores-Freitas,Nícolas Dullius Mallmann,Karla Alamo-Martínez +9 more
TL;DR: In this article, the kinematics, morphology, and stellar population properties of a sample of massive compact quiescent galaxies (MCGs, $10, \lesssim \, \log M_\star$ ��/M�$, 11$ and r�� e ∼ 1-3 kpc) in the MaNGA Survey were characterized.
Journal ArticleDOI
The Fundamental Plane of Massive Quiescent Galaxies at z~2.
Mikkel Stockmann,Inger Jorgensen,Sune Toft,Christopher J. Conselice,Christopher J. Conselice,Andreas L. Faisst,Berta Margalef-Bentabol,Anna Gallazzi,Stefano Zibetti,Gabriel B. Brammer,Carlos Gómez-Guijarro,Michaela Hirschmann,Claudia del P. Lagos,Francesco Valentino,Johannes Zabl +14 more
TL;DR: In this paper, the authors examined the Fundamental Plane (FP) and mass-to-light ratio (M/L$) scaling relations using the largest sample of massive quiescent galaxies at $1.5 11.26, and showed that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies.
Journal ArticleDOI
GAMA/XXL: X-ray point sources in low-luminosity galaxies in the GAMA G02/XXL-N field
E. Nwaokoro,E. Nwaokoro,Steven Phillipps,Andrew J. Young,Ivan K. Baldry,Angela Bongiorno,M. N. Bremer,Michael J. I. Brown,L. Chiappetti,R. De Propris,Simon P. Driver,Andrii Elyiv,Sotiria Fotopoulou,Paul Giles,Andrew M. Hopkins,Ben J Maughan,Sean L. McGee,Florian Pacaud,Marguerite Pierre,Manolis Plionis,Bianca M. Poggianti,Cristian Vignali,Cristian Vignali +22 more
TL;DR: In this paper, the authors matched the X-ray point sources found in the XXL-N field of the GAMA G02 survey field to galaxies with redshifts from the Galaxy And Mass Assembly (GAMA) G02 field (down to a magnitude limit r = 19.8) in order to search for active galactic nuclei and XRBs in GAMA galaxies.
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