Mathematics – Logic
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.2401p&link_type=abstract
American Astronomical Society, 199th AAS Meeting, #24.01; Bulletin of the American Astronomical Society, Vol. 33, p.1346
Mathematics
Logic
Scientific paper
We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample, which surveyed about 12 square degrees, thirty-eight supernovae were detected at redshifts 0.25--0.85. In a spatially-flat cosmological model consistent with the results obtained by the Supernova Cosmology Project, we derive a rest-frame Type Ia supernova rate at a mean redshift z~=0.55 of 1.53 +0.28-0.25 +0.32-0.31 10-4 h3 Mpc-3 yr-1 or 0.58 +0.10-0.09 +0.10-0.09 h2 SNu (1 SNu = 1 supernova per century per 1010LB&sun; ), where the first uncertainty is statistical and the second includes systematic effects. The dependence of the rate on the assumed cosmological parameters is studied and the redshift dependence of the rate per unit comoving volume is contrasted with local estimates in the context of possible cosmic star formation histories and progenitor models.
Aldering Greg
Amanullah Rahman
Antilogus Pierre
Astier Pierre
Balland Christophe
No associations
LandOfFree
The Distant Type Ia Supernovae Rate does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Distant Type Ia Supernovae Rate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Distant Type Ia Supernovae Rate will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1230362