Issue |
A&A
Volume 423, Number 3, September I 2004
|
|
---|---|---|
Page(s) | 881 - 894 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20035948 | |
Published online | 12 August 2004 |
Type Ia supernova rate at a redshift of ~0.1
1
DSM/DAPNIA, CEA/Saclay, 91191 Gif-sur-Yvette Cedex, France
2
Osservatorio Astronomico di Padova, INAF, vicolo dell'Osservatorio 5, 35122 Padova, Italy e-mail: blanc@pd.astro.it
3
Université Paris 7 - Denis Diderot, 2 place Jussieu, 75005 Paris, France
4
Collège de France, Physique Corpusculaire et Cosmologie, IN2P3 CNRS, 11 pl. M. Berthelot, 75231 Paris Cedex, France
5
Department of Astronomy, New Mexico State University, Las Cruces, NM 88003-8001, USA
6
NASA/Ames Research Center, Mail Stop 244, Moffet Field, CA 94035, USA
7
GEPI, Observatoire de Paris, 77 avenue de l'Observatoire, 75014 Paris, France
8
Laboratoire de l'Accélérateur Linéaire, IN2P3 CNRS, Université Paris-Sud, 91405 Orsay Cedex, France
9
Lawrence Berkeley National Lab, 1 Cyclotron Road, Berkeley, CA 94720, USA
10
Astronomical Observatory, Copenhagen University, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
11
Laboratoire de Physique Nucléaire et de Hautes Énergies, IN2P3 - CNRS - Universités Paris 6 et Paris 7, 4 place Jussieu, 75252 Paris Cedex 05, France
12
Institut d'Astrophysique Spatiale, Bâtiment 121, Université Paris 11, 91405 Orsay Cedex, France
13
Institut d'Astrophysique de Paris, INSU CNRS, 98 bis boulevard Arago, 75014 Paris, France
14
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA
15
Steward Observatory, The University of Arizona, 933 N. Cherry Ave, Tucson, AZ 85721-0065, USA
16
Department of Physics, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden
17
European Southern Observatory (ESO), Casilla 19001, Santiago 19, Chile
18
Observatoire Midi-Pyrénées, 14 avenue Edouard Belin, 31400 Toulouse, France
19
Departments of Astronomy and Physics, Ohio State University, Columbus, OH 43210, USA
20
Department of Physics, University of Oxford, Nuclear and Astrophysics laboratory, Keble Road, Oxford OX1 3RH, UK
21
Fermilab Wilson and Kirk Roads, Batavia, IL 60510-0500, USA
22
Observatoire de Marseille, 2 pl. Le Verrier, 13248 Marseille Cedex 04, France
23
LUTH, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon Cedex, France
24
Rensselaer Polytechnic Institute, 110 Eighth Street, Troy, NY 12180, USA
25
Laboratoire Leprince-Ringuet, LLR/École Polytechnique, Route de Saclay, 91128 Palaiseau Cedex, France
26
Department of Astronomy, University of Barcelona, Barcelona, Spain
27
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
Received:
24
December
2003
Accepted:
28
April
2004
We present the type Ia rate measurement based on two EROS
supernova search campaigns (in 1999 and 2000). Sixteen supernovae
identified as type Ia were discovered. The measurement of the
detection efficiency, using a Monte Carlo simulation, provides the
type Ia supernova explosion rate at a redshift ~0.13. The result
is SNu where 1 SNu = 1 SN /
/ century. This value is
compatible with the previous EROS measurement [CITE], done
with a much smaller sample, at a similar redshift. Comparison with
other values at different redshifts suggests an evolution of the
type Ia supernova rate.
Key words: stars: supernovae: general / galaxies: evolution / cosmology: miscellaneous / methods: observational
© ESO, 2004
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