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The bimodality of the 10k zCOSMOS-bright galaxies up to z  ~ 1: a new statistical and portable classification based on optical galaxy properties

Coppa, G. and Scarlata, C. and Capak, P. and Scoville, N. (2011) The bimodality of the 10k zCOSMOS-bright galaxies up to z  ~ 1: a new statistical and portable classification based on optical galaxy properties. Astronomy and Astrophysics, 535 . A10. ISSN 0004-6361.

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Aims. Our goal is to develop a new and reliable statistical method to classify galaxies from large surveys. We probe the reliability of the method by comparing it with a three-dimensional classification cube, using the same set of spectral, photometric and morphological parameters. Methods. We applied two different methods of classification to a sample of galaxies extracted from the zCOSMOS redshift survey, in the redshift range 0.5 ≲ z ≲ 1.3. The first method is a combination of three independent classification schemes – a spectroscopic one based on the strength of the continuum break at 4000 Å and the rest-frame equivalent width of the [O ii] emission line, a photometric one based on the observed B − z colours, and a morphological one. The second method exploits an entirely new approach based on statistical analyses like principal component analysis (PCA) and unsupervised fuzzy partition (UFP) clustering method. The PCA+UFP method has also been applied to a lower redshift sample (z ≲ 0.5), exploiting the same set of data but replacing the spectroscopic indicators with the equivalent width of Hα. Results. The comparison between the two methods shows fairly good agreement on the definition on the two main populations, the early-type and the late-type galaxies. Our PCA+UFP method of classification is robust, flexible and capable of identifying the two main populations of galaxies as well as an intermediate population. The intermediate galaxy population shows many of the properties of “green valley” galaxies, and constitutes a more coherent and homogeneous population. The large redshift range of the studied sample allows us to characterize downsizing: galaxies with masses of the order of 3 × 10^(10) M_⊙ are predominantly found in the transition from the late-type to the early-type group at z > 0.5, while galaxies with lower masses, of the order of 10^(10) M_⊙, are in transition at later epochs. Galaxies with M < 10^(10) M_⊙ have not yet begun to transition, while galaxies with very large masses (M > 5 × 10^(10 M_⊙) have mostly completed their transition to the early-type regime before z ~ 1.

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Additional Information:© 2011 ESO. Article published by EDP Sciences. Received 11 November 2010; Accepted 3 August 2011. Published online 25 October 2011. Based on observations undertaken at the European Southern Observatory (ESO) Very Large Telescope (VLT) under Large Program 175.A-0839. Also based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, operated by AURA Inc., under NASA contract NAS 5-26555, with the Subaru Telescope, operated by the National Astronomical Observatory of Japan, with the telescopes of the National Optical Astronomy Observatory, operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation, and with the Canada-France-Hawaii Telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique de France, and the University of Hawaii. This work was partially supported by INAF under PRIN-2006/ and by ASI under grant ASI/COFIS I/016/07/0.
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Subject Keywords:galaxies: general; galaxies: evolution; galaxies: fundamental parameters
Record Number:CaltechAUTHORS:20120214-111508456
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Official Citation:The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on optical galaxy properties G. Coppa, M. Mignoli, G. Zamorani, S. Bardelli, S. J. Lilly, M. Bolzonella, M. Scodeggio, D. Vergani, P. Nair, L. Pozzetti, A. Cimatti, E. Zucca, C. M. Carollo, T. Contini, O. Le Fèvre, A. Renzini, V. Mainieri, A. Bongiorno, K. I. Caputi, O. Cucciati, S. de la Torre, L. de Ravel, P. Franzetti, B. Garilli, P. Memeo, A. Iovino, P. Kampczyk, J.-P. Kneib, C. Knobel, A. M. Koekemoer, K. Kovač, F. Lamareille, J.-F. le Borgne, V. le Brun, C. Maier, R. Pellò, Y. Peng, E. Perez-Montero, E. Ricciardelli, C. Scarlata, J. D. Silverman, M. Tanaka, L. Tasca, L. Tresse, U. Abbas, D. Bottini, P. Capak, A. Cappi, P. Cassata, M. Fumana, L. Guzzo, A. Leauthaud, D. Maccagni, C. Marinoni, B. Meneux, P. Oesch, C. Porciani, R. Scaramella and N. Scoville A&A 535 A10 (2011) DOI:
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:29278
Deposited By: Jason Perez
Deposited On:15 Feb 2012 15:40
Last Modified:06 Jul 2015 20:01

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