Detecting strongly lensed supernovae at z [similar to] 5-7 with LSST
Supernovae (SNe) could be powerful probes of the properties of stars and galaxies at high redshifts in future surveys. Wide fields and longer exposure times are required to offset diminishing star formation rates and lower fluxes to detect useful number of events at high redshift. In principle, the...
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| Hauptverfasser: | , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2020
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 491, Heft: 2, Pages: 2447-2459 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz3203 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stz3203 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/491/2/2447/5637897 
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| Verfasserangaben: | Claes-Erik Rydberg, Daniel J. Whalen, Matteo Maturi, Thomas Collett, Mauricio Carrasco, Mattis Magg and Ralf S. Klessen |
MARC
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| 520 | |a Supernovae (SNe) could be powerful probes of the properties of stars and galaxies at high redshifts in future surveys. Wide fields and longer exposure times are required to offset diminishing star formation rates and lower fluxes to detect useful number of events at high redshift. In principle, the Large Synoptic Survey Telescope (LSST) could discover large numbers of early SNe because of its wide fields but only at lower redshifts because of its AB mag limit of ∼24. However, gravitational lensing by galaxy clusters and massive galaxies could boost flux from ancient SNe and allow LSST to detect them at earlier times. Here, we calculate detection rates for lensed SNe at z ∼ 5–7 for LSST. | ||
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