Dan Maoz, Filippo Mannucci
The identity of the progenitor systems of type-Ia supernovae (SNe Ia) is a
major unsolved problem in astrophysics. SN Ia rates are providing some striking
clues. We review the basics of SN rate measurement, preach about some sins of
SN rate measurement and analysis, and illustrate one of these sins with an
analogy about Martian scientists. We review the recent progress in measuring SN
Ia rates in various environments and redshifts, and their use to reconstruct
the SN Ia delay time distribution (DTD) -- the SN rate versus time that would
follow a hypothetical brief burst of star formation. A good number of DTD
measurements, using a variety of methods, appear to be converging. At delays
1View original: http://arxiv.org/abs/1111.4492
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