Type Ia supernova rate at $z \sim 0.1$
| dc.creator | Hardin, D. | |
| dc.creator | Afonso, C. | |
| dc.creator | Alard, C. | |
| dc.creator | Albert, J. N. | |
| dc.creator | Amadon, A. | |
| dc.creator | Andersen, J. | |
| dc.creator | Ansari, R. | |
| dc.creator | Aubourg, É. | |
| dc.creator | Bareyre, P. | |
| dc.creator | Bauer, F. | |
| dc.creator | Beaulieu, J. P. | |
| dc.creator | Blanc, G. | |
| dc.creator | Bouquet, A. | |
| dc.creator | Char, S. | |
| dc.creator | Charlot, X. | |
| dc.creator | Couchot, F. | |
| dc.creator | Coutures, C. | |
| dc.creator | Derue, F. | |
| dc.creator | Ferlet, R. | |
| dc.creator | Glicenstein, J. F. | |
| dc.creator | Goldman, B. | |
| dc.creator | Gould, A. | |
| dc.creator | Graff, D. | |
| dc.creator | Gros, M. | |
| dc.creator | Haissinski, J. | |
| dc.creator | Hamilton, J. C. | |
| dc.creator | de Kat, J. | |
| dc.creator | Kim, A. | |
| dc.creator | Lasserre, T. | |
| dc.creator | Lesquoy, É. | |
| dc.creator | Loup, C. | |
| dc.creator | Magneville, C. | |
| dc.creator | Mansoux, B. | |
| dc.creator | Marquette, J. B. | |
| dc.creator | Maurice, É. | |
| dc.creator | Milsztajn, A. | |
| dc.creator | Moniez, M. | |
| dc.creator | Palanque-Delabrouille, N. | |
| dc.creator | Perdereau, O. | |
| dc.creator | Prévot, L. | |
| dc.creator | Regnault, N. | |
| dc.creator | Rich, J. | |
| dc.creator | Spiro, M. | |
| dc.creator | Vidal-Madjar, A. | |
| dc.creator | Vigroux, L. | |
| dc.creator | Zylberajch, S. | |
| dc.creator | collaboration, The EROS | |
| dc.date | 2000-06-29 | |
| dc.date | 2000-07-04 | |
| dc.date.accessioned | 2026-07-25T17:48:12Z | |
| dc.description | We present the EROS nearby supernova ($z \sim 0.02 - 0.2$) search and the analysis of the first year of data (1997). A total of 80 square degrees were surveyed. Eight supernovæ were detected, four of which were spectroscopically identified as type Ia supernovæ. The search efficiency was determined with a Monte-Carlo simulation taking into account the efficiencies for both supernova detection and host galaxy identification. Assuming that for a given galaxy the supernova rate is proportional to the galactic luminosity, we compute a type Ia supernova explosion rate of: ${\cal R} = 0.44 {}_{-0.21}^{+0.35} {}_{-0.07}^{+0.13} h^2: / 10^{10} \lbsun / 100 {\rm yrs}$ at an average redshift of $\sim 0.1$ where the errors are respectively statistical and systematic (type misidentification included). | |
| dc.description | 8 pages, 6 figures, accepted in A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0006424 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0006424 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/50721 | |
| dc.subject | Astrophysics | |
| dc.title | Type Ia supernova rate at $z \sim 0.1$ | |
| dc.type | text |