The Supernova Rate in the Nearby and Distant Universe

Details The Supernova Rate in the Nearby and Distant Universe The Supernova Rate in the Nearby and Distant Universe

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...19311103r&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #111.03; Bulletin of the American Astronomical Society, Vol. 30, p.1419

Astronomy and Astrophysics

Astronomy

Scientific paper

I present the supernova rates computed from the Mount Stromlo Abell Cluster SN Search (MSACSS) and the High-Z SN Search, two CCD-based searches which use difference imaging techniques. These searches are approximately magnitude-limited with well-defined selection functions, unlike previous visual and photographic surveys which have suffered from selection problems such as deficiencies near the centers of galaxies, poorly-understood detection limits, or preferential treatment of field regions of high galaxy density. The SN samples collected from field galaxies at z<0.2 from the MSACSS ( ~ 60 squ-degree-years to mV ~ 20), rich Abell clusters at 0.02

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