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The evolution of quiescent galaxies at high redshifts (z ≥ 1.4)

Domínguez-Sánchez, H. and Capak, P. (2011) The evolution of quiescent galaxies at high redshifts (z ≥ 1.4). Monthly Notices of the Royal Astronomical Society, 417 (2). pp. 900-915. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20120104-131920085

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Abstract

The goal of this work is to study the evolution of high-redshift (z ≥ 1.4) quiescent galaxies over an effective area of ~ 1.7 deg^2 in the COSMOS field. Galaxies have been divided according to their star formation activity and the evolution of the different populations, in particular of the quiescent galaxies, has been investigated in detail. We have studied an IRAC (ma_( 3.6 μm) < 22.0) selected sample of ~ 18 000 galaxies at z ≥ 1.4 in the COSMOS field with multiwavelength coverage extending from the U band to the Spitzer 24 μm one. We have derived accurate photometric redshifts (σ_(Δz/(1+zs)) = 0.06) through a SED-fitting procedure. Other important physical parameters [masses, ages and star formation rates (SFR)] of the galaxies have been obtained using Maraston models. We have divided our sample into actively star-forming, intermediate and quiescent galaxies depending on their specific star formation rate (SSFR = SFR/M). We have computed the galaxy stellar mass function (GSMF) of the total sample and the different populations at z = 1.4–3.0. We have studied the properties of high-redshift quiescent galaxies finding that they are old (1–4 Gyr), massive (〈M〉~ 10^(10.65) M_⊙), weakly star-forming stellar populations with low dust extinction [E(B−V) ≤ 0.15] and small e-folding time-scales (τ~ 0.1–0.3 Gyr). We observe a significant evolution of the quiescent stellar mass function from 2.5 < z < 3.0 to 1.4 < z < 1.6, increasing by ~1 dex in this redshift interval. We find that z ~ 1.5 is an epoch of transition of the GSMF: while the GSMF at z ≳ 1.5 is dominated by the star-forming galaxies at all stellar masses, at z ≲ 1.5 the contribution to the total GSMF of the quiescent galaxies is significant and becomes higher than that of the star-forming population for M ≥ 10^(10.75) M_⊙. The fraction of star-forming galaxies decreases from 60–20 per cent from z ~ 2.5–3.0 to 1.4–1.6 for M~10^(11.0) M_⊙, while the quiescent population increases from 10–50 per cent at the same redshift and mass intervals. We compare the fraction of quiescent galaxies derived with that predicted by theoretical models and find that the Kitzbichler & White model, implemented on the Millennium Simulation, is the one that better reproduces the shape of the data. Finally, we calculate the stellar mass density of the star-forming and quiescent populations as a function of redshift and find that there is already a significant number of quiescent galaxies at z > 2.5 (log_ρ[M_⊙ Mpc^(−3)]~ 6), meaning that efficient star formation had to take place before that time.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1365-2966.2011.19263.xDOIUNSPECIFIED
http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2011.19263.x/abstractPublisherUNSPECIFIED
Additional Information:© 2011 The Authors. Monthly Notices of the Royal Astronomical Society © 2011 RAS. Accepted 2011 June 15. Received 2011 June 15; in original form 2011 March 30. Article first published online: 15 Sep 2011. This work was supported by an International grant from Instituto de Astrofísica de Canarias (IAC) with funding from the Research Structures Departments of Instituto Nazionale di Astrofísica (INAF). We thank the anonymous referee for the useful comments which helped to improve the original manuscript.
Group:COSMOS
Funders:
Funding AgencyGrant Number
Instituto de Astrofisica de Canarias (IAC)UNSPECIFIED
Instituto Nazionale di Astrofisica (INAF) Research Structures Departments UNSPECIFIED
Subject Keywords: galaxies: evolution; galaxies: high-redshift; galaxies: star formation
Record Number:CaltechAUTHORS:20120104-131920085
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120104-131920085
Official Citation:Domínguez Sánchez, H., Pozzi, F., Gruppioni, C., Cimatti, A., Ilbert, O., Pozzetti, L., McCracken, H., Capak, P., Le Floch, E., Salvato, M., Zamorani, G., Carollo, C. M., Contini, T., Kneib, J.-P., Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovač, K., Lamareille, F., Le Borgne, J.-F., Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D. and Zucca, E. (2011), The evolution of quiescent galaxies at high redshifts (z≥ 1.4). Monthly Notices of the Royal Astronomical Society, 417: 900–915. doi: 10.1111/j.1365-2966.2011.19263.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:28652
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:04 Jan 2012 21:52
Last Modified:23 Aug 2016 00:07

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