J/ApJ/827/L25      Fractions of quiescent galaxies evolution     (Martis+, 2016)

The evolution of the fractions of quiescent and star-forming galaxies as a function of stellar mass since z=3: increasing importance of massive, dusty star-forming galaxies in the early universe. Martis N.S., Marchesini D., Brammer G.B., Muzzin A., Labbe I., Momcheva I.G., Skelton R.E., Stefanon M., van Dokkum P.G., Whitaker K.E. <Astrophys. J., 827, L25-L25 (2016)> =2016ApJ...827L..25M 2016ApJ...827L..25M (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, IR Keywords: galaxies: evolution Abstract: Using the UltraVISTA DR1 and 3D-HST catalogs, we construct a stellar-mass-complete sample, unique for its combination of surveyed volume and depth, to study the evolution of the fractions of quiescent galaxies, moderately unobscured star-forming galaxies, and dusty star-forming galaxies as a function of stellar mass over the redshift interval 0.2≤z≤3.0. We show that the role of dusty star-forming galaxies within the overall galaxy population becomes more important with increasing stellar mass and grows rapidly with increasing redshift. Specifically, dusty star-forming galaxies dominate the galaxy population with log(Mstar/M)≳10.3 at z≳2. The ratio of dusty and non-dusty star-forming galaxies as a function of stellar mass changes little with redshift. Dusty star-forming galaxies dominate the star-forming population at log(Mstar/M)≳10.0-10.5, being a factor of ∼3-5 more common, while unobscured star-forming galaxies dominate at log(Mstar/M)≲10. At log(Mstar/M)>10.5, red galaxies dominate the galaxy population at all redshift z<3, either because they are quiescent (at late times) or dusty star-forming (in the early universe). Description: We used the UltraVISTA DR1 (Muzzin+ 2013, J/ApJS/206/8) covering 1.62deg2 and the 3D-HST (Skelton+ 2014, J/ApJS/214/24; Momcheva+ 2016ApJS..225...27M 2016ApJS..225...27M) covering 900arcmin2, catalogs. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 89 70 Fractions of quiescent, non-dusty star-forming (ndSF), and dusty star-forming (dSF) galaxies -------------------------------------------------------------------------------- See also: J/ApJ/827/74 : [NII]/Hα ratio in galaxies with KMOS3D (Wuyts+, 2016) J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014) J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013) J/A+A/556/A55 : Multi-color photometry of star-forming galaxies (Ilbert+, 2013) J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013) J/ApJ/675/234 : Stellar mass functions for 0<z<4 gal. (Perez-Gonzalez+, 2008) J/ApJ/655/51 : HDFS IRAC observations of 2<z<3.5 galaxies (Wuyts+, 2007) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 F4.2 --- zlow [0.2/2.5] Lower redshift value 6- 9 F4.2 --- zup [0.5/3] Upper redshift value 11- 15 F5.2 [Msun] Mlow [8.5/11.5] Lower log stellar mass bin 17- 21 F5.2 [Msun] Mup [8.8/11.8] Upper log stellar mass bin 23- 28 F6.4 --- fQ [0.03/1] Fractions of quiescent galaxies 30- 35 F6.4 --- e_fQ [0.005/0.3] Lower uncertainty in fQ 37- 42 F6.4 --- E_fQ [0/0.4] Upper uncertainty in fQ 44- 49 F6.4 --- fndSF [0/0.9] Fraction of non-dusty star-forming galaxies 51- 56 F6.4 --- e_fndSF [0/0.3] Lower uncertainty in fndSF 58- 63 F6.4 --- E_fndSF [0.007/0.5] Upper uncertainty in fndSF 65- 70 F6.4 --- fdSF [0/0.7] Fraction of dusty star-forming galaxies 72- 77 F6.4 --- e_fdSF [0/0.3] Lower uncertainty in fdSF 79- 84 F6.4 --- E_fdSF [0.005/0.3] Upper uncertainty in fdSF 86- 89 I4 --- N [11/4111] Total number of galaxies -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 29-Nov-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line