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The VIMOS Public Extragalactic Redshift Survey (VIPERS)
- 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
- Subjects :
- Active galactic nucleus
Galaxies: statistics
Astrophysics
Galaxies: groups: general
Astrophysics::Cosmology and Extragalactic Astrophysics
Parameter space
01 natural sciences
star formation [Galaxies]
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
0103 physical sciences
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Physics
Sequence
Galaxies: star formation
010308 nuclear & particles physics
Spectral density
Galaxies: evolution
Astronomy and Astrophysics
Galaxy: fundamental parameters
Astronomy and Astrophysic
Redshift survey
evolution [Galaxies]
Galaxies: stellar content
Astrophysics - Astrophysics of Galaxies
Galaxy
Redshift
Space and Planetary Science
Unsupervised learning
stellar content [Galaxies]
Subjects
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⟩