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
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The VANDELS ESO public spectroscopic survey
Ross J. McLure,Laura Pentericci,Andrea Cimatti,James Dunlop,D. Elbaz,Adriano Fontana,Kirpal Nandra,Ricardo Amorín,M. Bolzonella,Angela Bongiorno,A. C. Carnall,Marco Castellano,Michele Cirasuolo,O. Cucciati,Fergus Cullen,S. de Barros,Steve Finkelstein,Fabio Fontanot,P. Franzetti,M. Fumana,Adriana Gargiulo,B. Garilli,Lucia Guaita,W. G. Hartley,A. Iovino,Matt J. Jarvis,S. Juneau,W. Karman,D. Maccagni,F. Marchi,E. Mármol-Queraltó,Emanuela Pompei,Lucia Pozzetti,Marco Scodeggio,V. Sommariva,Margherita Talia,Omar Almaini,Italo Balestra,S. Bardelli,Eric F. Bell,Nathan Bourne,Rebecca A. A. Bowler,Marcella Brusa,Fernando Buitrago,Karina Caputi,Paolo Cassata,Stéphane Charlot,Annalisa Citro,Giovanni Cresci,Stefano Cristiani,E. Curtis-Lake,Mark Dickinson,Giovanni G. Fazio,Henry C. Ferguson,Fabrizio Fiore,M. Franco,Johan P. U. Fynbo,Audrey Galametz,Antonis Georgakakis,M. Giavalisco,Andrea Grazian,Nimish P. Hathi,Intae Jung,Seock-Sam Kim,Anton M. Koekemoer,Y. Khusanova,O. Le Fevre,Jennifer M. Lotz,F. Mannucci,David T. Maltby,K. Matsuoka,D. J. McLeod,H. Mendez-Hernandez,Jairo Méndez-Abreu,M. Mignoli,Michele Moresco,Alice Mortlock,Mario Nonino,Maurilio Pannella,Casey Papovich,P. Popesso,D. P. Rosario,Mara Salvato,P. Santini,Daniel Schaerer,Corentin Schreiber,Daniel P. Stark,L. A. M. Tasca,R. Thomas,Tommaso Treu,Eros Vanzella,Vivienne Wild,Christina C. Williams,G. Zamorani,E. Zucca +94 more
TL;DR: The VANDELS survey as mentioned in this paper was designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.
Journal ArticleDOI
THE MOSDEF SURVEY: DYNAMICAL AND BARYONIC MASSES AND KINEMATIC STRUCTURES OF STAR-FORMING GALAXIES AT 1.4 ≤ z ≤ 2.6
Sedona H. Price,Mariska Kriek,Alice E. Shapley,Naveen A. Reddy,William R. Freeman,Alison L. Coil,Laura de Groot,Irene Shivaei,Brian Siana,Mojegan Azadi,Guillermo Barro,Bahram Mobasher,Ryan L. Sanders,Tom Zick +13 more
TL;DR: In this paper, Price et al. presented Ha gas kinematics for 178 star-forming galaxies at z ∼ 2 from the MOSFIRE Deep Evolution Field survey and developed models to interpret the kinematic measurements from fixed-angle multi-object spectroscopy, using structural parameters derived from Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey Hubble Space Telescope/F160W imaging.
Journal ArticleDOI
Dust attenuation, bulge formation and inside-out cessation of star-formation in Star-Forming Main Sequence galaxies at z~2
Sandro Tacchella,C. M. Carollo,N. M. Förster Schreiber,Alvio Renzini,A. Dekel,Reinhard Genzel,Philipp Lang,S. J. Lilly,Chiara Mancini,Masato Onodera,Linda J. Tacconi,Stijn Wuyts,G. Zamorani +12 more
TL;DR: In this paper, the authors derived two-dimensional dust attenuation maps from the UV continuum for 10 galaxies on the Star-Forming Main Sequence (SFMS) and used these maps to correct UV and H$\alpha-based starformation rates.
Journal ArticleDOI
The co-evolution of total density profiles and central dark matter fractions in simulated early-type galaxies
Rhea-Silvia Remus,Klaus Dolag,Thorsten Naab,Andreas Burkert,Michaela Hirschmann,Tadziu L. Hoffmann,Peter H. Johansson +6 more
TL;DR: In this article, cosmological hydrodynamical simulations for a coevolution of the slope of the total (dark and stellar) mass density profile, gamma (tot), and the dark matter fraction within the half-mass radius, f(DM), in early-type galaxies are presented.
Journal ArticleDOI
Extremely Small Sizes for Faint z ∼ 2-8 Galaxies in the Hubble Frontier Fields: A Key Input for Establishing Their Volume Density and UV Emissivity
TL;DR: In this article, the authors provided the first observational constraints on the sizes of the faintest galaxies lensed by the Hubble Frontier Fields (HFF) clusters, finding that the detectability of highly-magnified galaxies as a function of shear is very dependent on a galaxy's size.
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