Photometric classification and redshift estimation of LSST Supernovae

Author:

Dai Mi1ORCID,Kuhlmann Steve2,Wang Yun3,Kovacs Eve2

Affiliation:

1. Department of Physics & Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Rd, Piscataway, NJ 08854, USA

2. Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439, USA

3. IPAC, California Institute of Technology, Mail Code 314-6, 1200 East California Boulevard, Pasadena, CA 91125, USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 17 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Forecasting supernova observations with the CSST: I. Photometric samples;Science China Physics, Mechanics & Astronomy;2024-09-03

2. Multiview Symbolic Regression;Proceedings of the Genetic and Evolutionary Computation Conference;2024-07-14

3. Photo-zSNthesis: Converting Type Ia Supernova Lightcurves to Redshift Estimates via Deep Learning;The Astrophysical Journal;2023-09-01

4. Using Host Galaxy Photometric Redshifts to Improve Cosmological Constraints with Type Ia Supernovae in the LSST Era;The Astrophysical Journal;2023-02-01

5. Concerning colour: The effect of environment on type Ia supernova colour in the dark energy survey;Monthly Notices of the Royal Astronomical Society;2022-12-19

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