Type Ia supernova rate at a redshift of 0.1

Details Type Ia supernova rate at a redshift of 0.1 Type Ia supernova rate at a redshift of 0.1

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf...77b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

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At the present time, there are few well studied supernovae and systematic searches are necessary. It happens that the rate measurement is an interesting by-product of such systematic supernova search programs (basically made for cosmological purposes). In the beginning of 1999 the Supernova Cosmology Project coordinated a worldwide nearby (z sim 0.01 - 0.2) type Ia supernova search, and provided spectroscopic and photometric follow-up. The EROS experiment was involved as a search facility and discovered almost half of the whole sample obtained. The type Ia supernova rate has been derived from this search, at a mean redshift of 0.1.

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