Empirical delay-time distributions of type Ia supernovae from the extended goods/hubble space telescope supernova survey

Abstract

Using the Hubble Space Telescope (HST) Advanced Camera for Surveys imaging of the GOODS North and South fields during Cycles 11, 12, and 13, we derive empirical constraints on the delay-time distribution function for type Ia supernovae (SNeIa). We extend our previous analysis to the three-year sample of 56 SNeIa over the range 0.2 < z < 1.8, using a Markov chain Monte Carlo to determine the best-fit unimodal delay-time distribution function. The test, which ultimately compares the star formation rate density history to the unbinned volumetric SNIa rate history from the GOODS/HST SN survey, reveals a SNIa delay-time distribution that is tightly confined to 3-4Gyr (to >95% confidence). This result is difficult to resolve with any intrinsic delay-time distribution function (bimodal or otherwise), in which a substantial fraction (e.g., >10%) of events are "prompt," requiring less than approximately 1Gyr to develop from formation to explosion. The result is, however, strongly motivated by the decline in the number of SNeIa at z > 1.2. Sub-samples of the HST SN data confined to lower redshifts (z < 1) show plausible delay-time distributions that are dominated by prompt events, which is more consistent with results from low-redshift supernova samples and supernova host galaxy properties. Scenarios in which a substantial fraction of z > 1.2 supernovae are extraordinarily obscured by dust may partly explain the differences in low-z and high-z results. Other possible resolutions may include environmental dependences (such as gas-phase metallicity) that affect the progenitor mechanism efficiency, especially in the early universe. © 2010. The American Astronomical Society. All rights reserved.