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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On the Transition of the Galaxy Quenching Mode at 0.5?<?z?<?1 in CANDELS
F. S. Liu,F. S. Liu,Meng Jia,Hassen M. Yesuf,S. M. Faber,David C. Koo,Yicheng Guo,Eric F. Bell,Dongfei Jiang,Weichen Wang,Anton M. Koekemoer,X. Z. Zheng,Jerome J. Fang,Guillermo Barro,Pablo G. Pérez-González,Avishai Dekel,Dale D. Kocevski,Nimish P. Hathi,Darren J. Croton,Marc Huertas-Company,Xian-Min Meng,Wei Tong,Lu Liu +22 more
TL;DR: In this paper, the authors investigate the galaxy quenching process at intermediate redshift using a sample of similar to 4400 galaxies with M-* >10(9) M-circle dot between redshift 0.5 and 1.0 in all five CANDELS fields.
Journal ArticleDOI
The ALHAMBRA survey: tight dependence of the optical mass-to-light ratio on galaxy colour up to z = 1.5
C. López-Sanjuan,L. A. Díaz-García,A. J. Cenarro,Alberto Fernández-Soto,Kerttu Viironen,Alberto Molino,Narciso Benítez,David Cristóbal-Hornillos,Mariano Moles,Jesús A. Varela,Pablo Arnalte-Mur,B. Ascaso,Francisco J. Castander,Miguel Cerviño,R. M. González Delgado,C. Husillos,I. Márquez,J. Masegosa,A. del Olmo,Mirjana Pović,J. Perea +20 more
TL;DR: In this article, the authors derived the mass-to-light ratio vs. colour relation (MLCR) both for quiescent and star-forming galaxies and derived the intrinsic relation and its physical dispersion with a Bayesian inference model.
Journal ArticleDOI
The dynamics and distribution of angular momentum in HiZELS star-forming galaxies at z = 0.8-3.3
Steven Gillman,A. M. Swinbank,Alfred L. Tiley,Christopher Harrison,Ian Smail,U. Dudzevičiūtė,Ray M. Sharples,P. N. Best,Richard G. Bower,Rachel Cochrane,Deanne B. Fisher,James E. Geach,Karl Glazebrook,Edo Ibar,Juan Molina,Danail Obreschkow,Danail Obreschkow,Matthieu Schaller,David Sobral,Sarah M. Sweet,James W. Trayford,Tom Theuns +21 more
TL;DR: In this article, adaptive optics assisted integral field spectroscopy of 34 star-forming galaxies at 0.8-3.3 selected from the HiZELS narrow-band survey is presented.
Journal ArticleDOI
Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ̃ 0.7
A. Calabrò,Emanuele Daddi,A. Puglisi,Ernesto Oliva,Raphael Gobat,Paolo Cassata,Ricardo Amorín,Nobuo Arimoto,Médéric Boquien,R. Carraro,I. Delvecchio,Edo Ibar,Shuowen Jin,S. Juneau,Daizhong Liu,Masato Onodera,F. Mannucci,H. Mendez-Hernandez,G. Rodighiero,F. Valentino,A. Zanella +20 more
TL;DR: In this article, the authors investigate the origin of this sequence for the same sample and show that total attenuations anticorrelate with the starburst sizes in radio (3 GHz) with a significance larger than 5σ and a scatter of 0.26 dex.
Journal ArticleDOI
A local leaky-box model for the local stellar surface density–gas surface density–gas phase metallicity relation
Guangtun Zhu,Jorge K. Barrera-Ballesteros,Timothy M. Heckman,Nadia L. Zakamska,Nadia L. Zakamska,Sebastián F. Sánchez,Renbin Yan,Jonathan Brinkmann +7 more
TL;DR: In this article, the authors revisited the relation between the stellar surface density, the gas surface density and the gas-phase metallicity of typical disk galaxies in the local Universe with the SDSS-IV/MaNGA survey, using the star formation rate surface density as an indicator for the gassurface density.
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