Issue |
A&A
Volume 614, June 2018
|
|
---|---|---|
Article Number | A56 | |
Number of page(s) | 21 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201732407 | |
Published online | 15 June 2018 |
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)
I. Introduction to the survey★
1
Aix-Marseille Université, CNRS, CNES, LAM (Laboratoire d’Astrophysique de Marseille), UMR 7326,
13388
Marseille,
France
e-mail: alessandro.boselli@lam.fr
2
Max-Planck-Institut für extraterrestrische Physik,
Giessenbachstrasse 1,
85748
Garching,
Germany
e-mail: mfossati@mpe.mpg.de
3
Universitäts-Sternwarte München,
Scheinerstrasse 1,
81679
München,
Germany
4
NRC Herzberg Astronomy and Astrophysics,
5071 West Saanich Road,
Victoria,
BC
V9E 2E7,
Canada
e-mail: laura.ferrarese@nrc-cnrc.gr.ca
5
Università di Milano-Bicocca,
Piazza della Scienza 3,
20100
Milano,
Italy
6
INAF – Osservatorio Astronomico di Brera,
via Brera 28,
20159
Milano,
Italy
7
Kavli Institute for Astronomy and Astrophysics, Peking University,
Beijing
100871,
PR China
8
Department of Physics and Astronomy, University of Waterloo,
Waterloo,
ON
N2L 3G1,
Canada
9
Department of Physics & Astronomy, University of Western Ontario,
London,
ON
N6A 3K7,
Canada
10
Unidad de Astronomía, Facultad de Ciencias Básicas, Universidad de Antofagasta,
Avda. U. de Antofagasta 02800,
Antofagasta,
Chile
11
Institut d’Astrophysique Spatiale, UMR 8617, Université Paris-Sud,
Bâtiment 121,
91405
Orsay,
France
12
Laboratoire d’Astrophysique de Bordeaux, Université de Bordeaux, CNRS,
B18N, allée Geoffroy Saint-Hilaire,
33615
Pessac,
France
13
Collège de France,
11 Pl. M. Berthelot,
75005
Paris,
France
14
LERMA, Observatoire de Paris, CNRS, PSL Research University, Sorbonne Universités,
UPMC Univ. Paris 06,
75014
Paris,
France
15
IRAP, Institut de Recherche en Astrophysique et Planétologie, CNRS,
14 avenue Edouard Belin,
31400
Toulouse,
France
16
International Centre for Radio Astronomy Research, The University of Western Australia,
35 Stirling Highway,
Crawley,
WA
6009,
Australia
17
CEA/IRFU/SAP, Laboratoire AIM Paris-Saclay, CNRS/INSU, Université Paris Diderot, Observatoire de Paris, PSL Research University,
91191
Gif-sur-Yvette Cedex,
France
18
Université Laval,
2325, rue de l’université,
Québec,
QC
G1V 0A6,
Canada
19
Institute for Computational Cosmology and Centre for Extragalactic Astronomy, Department of Physics, Durham University,
South Road,
Durham
DH1 3LE,
UK
20
Department of Physics & Astronomy, McMaster University,
Hamilton
ON L8S 4K1,
Canada
21
Department of Astrophysics, University of Vienna,
Türkenschanzstrasse 17,
1180
Vienna,
Austria
22
Australia Telescope National Facility, CSIRO Astronomy and Space Science,
PO Box 76,
Epping,
NSW
1710,
Australia
23
Department of Physics and Astronomy, University of Victoria,
PO Box 1700 STN CSC,
Victoria,
BC
V8W 2Y2,
Canada
24
Department of Physics and Astronomy, Trent University,
1600 West Bank Drive,
Peterborough,
ON
K9L 0G2,
Canada
25
Department of Astronomy, Peking University,
Beijing
100871,
PR China
26
Laboratório de Astrofísica Teórica e Observacional, Universidade Estadual de Santa Cruz, 45650-000
Ilhéus,
Brazil
27
Institut d’Astrophysique de Paris, UMR7095 CNRS, Université P. & M. Curie,
98bis Bd. Arago,
75104
Paris,
France
28
Astronomy Centre, Department of Physics and Astronomy, University of Sussex,
Falmer,
Brighton
BN1 9QH,
UK
29
UK Astronomy Technology Centre, Royal Observatory Edinburgh,
Blackford Hill,
Edinburgh
EH9 3HJ,
UK
30
Osservatorio Astronomico di Cagliari,
via della Scienza 5,
09047
Selargius,
Cagliari,
Italy
31
Department of Physics, Royal Military College of Canada,
PO Box 17000, Station Forces,
Kingston,
ON
K7L 7B4,
Canada
32
Department of Physics, Engineering Physics, and Astronomy, Queen’s University,
Kingston,
ON
K7L 3N6,
Canada
33
Department of Physics and Astronomy, University of Alabama in Huntsville,
Huntsville,
AL
35899,
USA
34
Center for Computational Astrophysics, Flatiron Institute,
162 5th Avenue,
New York,
NY
10003,
USA
35
Observatoire Astronomique de Strasbourg, UMR 7750,
11, rue de l’Université,
67000
Strasbourg,
France
36
LUPM, Université de Montpellier, CNRS, Pl. Eugène Bataillon,
34095
Montpellier,
France
37
Canada France Hawaii Telescope Corporation,
Kamuela,
HI
96743,
USA
Received:
4
December
2017
Accepted:
7
February
2018
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France–Hawaii Telescope. The survey covers the whole Virgo cluster region from its core to one virial radius (104 deg2). The sensitivity of the survey is of f(Hα) ~ 4 × 10−17 erg s−1 cm−2 (5σ detection limit) for point sources and Σ(Hα) ~ 2 × 10−18 erg s−1 cm−2 arcsec−2 (1σ detection limit at 3 arcsec resolution) for extended sources, making VESTIGE the deepest and largest blind NB survey of a nearby cluster. This paper presents the survey in all its technical aspects, including the survey design, the observing strategy, the achieved sensitivity in both the NB Hα+[NII] and in the broad-band r filter used for the stellar continuum subtraction, the data reduction, calibration, and products, as well as its status after the first observing semester. We briefly describe the Hα properties of galaxies located in a 4 × 1 deg2 strip in the core of the cluster north of M87, where several extended tails of ionised gas are detected. This paper also lists the main scientific motivations for VESTIGE, which include the study of the effects of the environment on galaxy evolution, the fate of the stripped gas in cluster objects, the star formation process in nearby galaxies of different type and stellar mass, the determination of the Hα luminosity function and of the Hα scaling relations down to ~106 M⊙ stellar mass objects, and the reconstruction of the dynamical structure of the Virgo cluster. This unique set of data will also be used to study the HII luminosity function in hundreds of galaxies, the diffuse Hα+[NII] emission of the Milky Way at high Galactic latitude, and the properties of emission line galaxies at high redshift.
Key words: galaxies: clusters: general / galaxies: clusters: individual: Virgo / galaxies: evolution / galaxies: interactions / galaxies: ISM
Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii.
© ESO 2018
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0;), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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