Revised Supernova Rates from the IfA Deep Survey
arXiv:1008.4573 · doi:10.1088/0004-637X/723/1/47
Abstract
The IfA Deep survey uncovered ~130 thermonuclear supernovae (TNSNe, i.e. Type Ia) candidates at redshifts from z=0.1 out to beyond z=1. The TNSN explosion rates derived from these data have been controversial, conflicting with evidence emerging from other surveys. This work revisits the IfA Deep survey to re-evaluate the photometric evidence. Applying the SOFT program to the light curves of all SN candidates, we derive new classification grades and redshift estimates. We find a volumetric rate for z~0.5 that is substantially smaller than the originally published values, bringing the revised IfA Deep rate into good agreement with other surveys. With our improved photometric analysis techniques, we are able to confidently extend the rate measurements to higher redshifts, and we find a steadily increasing TNSN rate, with no indication of a peak out to z=1.05.
Accepted for publication in ApJ. 12 pages, 3 figures. Table 2 to be available in full in ApJ online, or on request to authors
References in corpus (12)
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
- A Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey Data Release 6
- Supernova rates from the Southern inTermediate Redshift ESO Supernova Search (STRESS)
- The Type Ia Supernova Rate at z ~0.5 from the Supernova Legacy Survey
- The Extended HST Supernova Survey: The Rate of SNe Ia at z>1.4 Remains Low
- Supernovae in the Subaru Deep Field: An Initial Sample, and Type Ia Rate, out to Redshift 1.6
- A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
- Fuzzy Supernova Templates I: Classification
- The Rate of Type Ia Supernovae at z~0.2 from SDSS-I Overlapping Fields
- Fuzzy Supernova Templates II: Parameter Estimation
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