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Title: The distant type Ia supernova rate

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/342129· OSTI ID:807402

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 red shift z {approx_equal} 0.55 of 1.53 {sub -0.25}{sub -0.31}{sup 0.28}{sup 0.32} x 10{sup -4} h{sup 3} Mpc{sup -3} yr{sup -1} or 0.58{sub -0.09}{sub -0.09}{sup +0.10}{sup +0.10} h{sup 2} SNu(1 SNu = 1 supernova per century per 10{sup 10} L{sub B}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.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Director, Office of Science. Office of High Energy and Nuclear Physics. Division of High Energy Physics; National Science Foundation (US)
DOE Contract Number:
AC03-76SF00098
OSTI ID:
807402
Report Number(s):
LBNL-47887; LPNH 02-02; ASJOAB; R&D Project: 419401; B& R KA0401010; TRN: US0301820
Journal Information:
Astrophysical Journal, Vol. 577, Issue 1, Part 1; Other Information: Journal Publication Date: September 20, 2002; PBD: 20 May 2002; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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