Upcoming photometric surveys will discover tens of thousands of Type Ia supernovae (SNe Ia), vastly outpacing the capacity of our spectroscopic resources. In order to maximize the scientific return of these observations in the absence of spectroscopic information, we must accurately extract key parameters, such as SN redshifts, with photometric information alone. We present Photo-
How to Obtain the Redshift Distribution from Probabilistic Redshift Estimates
A reliable estimate of the redshift distribution
- NSF-PAR ID:
- 10364681
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 928
- Issue:
- 2
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 127
- Size(s):
- ["Article No. 127"]
- Sponsoring Org:
- National Science Foundation
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