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The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Authors :
Małgorzata Siudek
G. De Lucia
Daniela Vergani
P. Franzetti
C. Adami
Stéphane Arnouts
M. Scodeggio
V. Le Brun
A. Zanichelli
T. Moutard
Julien Bel
Lauro Moscardini
Chris P. Haines
D. Bottini
D. Maccagni
Iary Davidzon
Enzo Branchini
Tsutomu T. Takeuchi
Lidia Tasca
Jean Coupon
Olga Cucciati
Bianca Garilli
Olivier Ilbert
G. Zamorani
A. Cappi
Agnieszka Pollo
Luigi Guzzo
Katarzyna Małek
A. Iovino
J. Krywult
Ummi Abbas
Tomasz Krakowski
Benjamin R. Granett
M. Bolzonella
Alexander Fritz
Federico Marulli
O. Le Fèvre
M. Polletta
S. de la Torre
Rita Tojeiro
Siudek, M.
Małek, K.
Pollo, A.
Krakowski, T.
Iovino, A.
Scodeggio, M.
Moutard, T.
Zamorani, G.
Guzzo, L.
Garilli, B.
Granett, B.R.
Bolzonella, M.
De La Torre, S.
Abbas, U.
Adami, C.
Bottini, D.
Cappi, A.
Cucciati, O.
Davidzon, I.
Franzetti, P.
Fritz, A.
Krywult, J.
Le Brun, V.
Le Fèvre, O.
MacCagni, D.
Marulli, F.
Polletta, M.
Tasca, L.A.M.
Tojeiro, R.
Vergani, D.
Zanichelli, A.
Arnouts, S.
Bel, J.
Branchini, E.
Coupon, J.
De Lucia, G.
Ilbert, O.
Haines, C.P.
Moscardini, L.
Takeuchi, T.T.
Center for Theoretical Physics, Polish Academy of Sciences , Al. Lotników 32/46, 02-668 Warsaw, Poland (CFT PAN)
National Centre for Nuclear Research (Warszawa)
INAF - Osservatorio Astronomico di Brera (OAB)
Istituto Nazionale di Astrofisica (INAF)
Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI)
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
Università degli Studi di Milano [Milano] (UNIMI)
INAF - Osservatorio Astrofisico di Torino (OATo)
Joseph Louis LAGRANGE (LAGRANGE)
Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS)
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Jan Kochanowski University
Alma Mater Studiorum University of Bologna (UNIBO)
Istituto Nazionale di Fisica Nucleare, Sezione di Bologna (INFN, Sezione di Bologna)
Istituto Nazionale di Fisica Nucleare (INFN)
Institut de recherche en astrophysique et planétologie (IRAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)
University of St Andrews [Scotland]
Istituto di Radioastronomia [Bologna] (IRA)
Centre de Physique Théorique - UMR 7332 (CPT)
Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)
CPT - E3 Cosmologie
Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)
Università degli Studi Roma Tre
Istituto Nazionale di Fisica Nucleare, Sezione di Roma 3 (INFN, Sezione di Roma 3)
INAF - Osservatorio Astronomico di Roma (OAR)
University of Geneva [Switzerland]
INAF - Osservatorio Astronomico di Trieste (OAT)
Nagoya University
Università degli Studi di Milano = University of Milan (UNIMI)
Université Nice Sophia Antipolis (1965 - 2019) (UNS)
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Università degli Studi Roma Tre = Roma Tre University (ROMA TRE)
Université de Genève = University of Geneva (UNIGE)
Granett, B. R.
Maccagni, D.
Tasca, L. A. M.
Haines, C. P.
Takeuchi, T. T.
ITA
USA
GBR
FRA
DEU
Source :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 617, pp.A70. ⟨10.1051/0004-6361/201832784⟩, Astronomy and Astrophysics-A&A, 2018, 617, pp.A70. ⟨10.1051/0004-6361/201832784⟩
Publication Year :
2018

Abstract

Various galaxy classification schemes have been developed so far to constrain the main physical processes regulating evolution of different galaxy types. In the era of a deluge of astrophysical information and recent progress in machine learning, a new approach to galaxy classification becomes imperative. We employ a Fisher Expectation-Maximization unsupervised algorithm working in a parameter space of 12 rest-frame magnitudes and spectroscopic redshift. The model (DBk) and the number of classes (12) were established based on the joint analysis of standard statistical criteria and confirmed by the analysis of the galaxy distribution with respect to a number of classes and their properties. This new approach allows us to classify galaxies based just on their redshifts and UV-NIR spectral energy distributions. The FEM unsupervised algorithm has automatically distinguished 12 classes: 11 classes of VIPERS galaxies and an additional class of broad-line AGNs. After a first broad division into blue, green and red categories we obtained a further sub-division into three red, three green, and five blue galaxy classes. The FEM classes follow the galaxy sequence from the earliest to the latest types that is reflected in their colours (which are constructed from rest-frame magnitudes used in classification procedure) but also their morphological, physical, and spectroscopic properties (not included in the classification scheme). We demonstrate that the members of each class share similar physical and spectral properties. In particular, we are able to find three different classes of red passive galaxy populations. Thus, we demonstrate the potential of an unsupervised approach to galaxy classification and we retrieve the complexity of galaxy populations at z~0.7, a task that usual simpler colour-based approaches cannot fulfil.<br />Comment: published in A&A, 27 pages, 10 figures, 4 appendixes. Please contact Malgorzata Siudek (msiudek@ifae.es) if you are interested in the catalogue

Details

Language :
English
ISSN :
00046361
Database :
OpenAIRE
Journal :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 617, pp.A70. ⟨10.1051/0004-6361/201832784⟩, Astronomy and Astrophysics-A&A, 2018, 617, pp.A70. ⟨10.1051/0004-6361/201832784⟩
Accession number :
edsair.doi.dedup.....d2f565e09b5c2c59835403241135dd9d
Full Text :
https://doi.org/10.1051/0004-6361/201832784⟩