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Title:Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
Authors:ID Petrushevska, Tanja (Author)
Files:.pdf symmetry-967869.pdf (863,97 KB)
MD5: 894563D2874400DB685DB98A309855CF
 
Language:English
Work type:Not categorized
Typology:1.01 - Original Scientific Article
Organization:UNG - University of Nova Gorica
Abstract:Strong lensing by galaxy clusters can be used to significantly expand the survey reach, thus allowing observation of magnified high-redshift supernovae that otherwise would remain undetected. Strong lensing can also provide multiple images of the galaxies that lie behind the clusters. Detection of strongly lensed Type Ia supernovae (SNe Ia) is especially useful because of their standardizable brightness, as they can be used to improve either cluster lensing models or independent measurements of cosmological parameters. The cosmological parameter, the Hubble constant, is of particular interest given the discrepancy regarding its value from measurements with different approaches. Here, we explore the feasibility of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) of detecting strongly lensed SNe in the field of five galaxy clusters (Abell 1689 and Hubble Frontier Fields clusters) that have well-studied lensing models. Considering the 88 systems composed of 268 individual multiple images in the five cluster fields, we find that the LSST will be sensitive to SNe Ia (SNe IIP) exploding in 41 (23) galaxy images. The range of redshift of these galaxies is between 1.01 < z < 3.05. During its 10 years of operation, LSST is expected to detect 0.2 ± 0.1 SN Ia and 0.9 ± 0.3 core collapse SNe. However, as LSST will observe many more massive galaxy clusters, it is likely that the expectations are higher. We stress the importance of having an additional observing program for photometric and spectroscopic follow-up of the strongly lensed SNe detected by LSST.
Keywords:supernovae, strong gravitational lensing, galaxy clusters
Publication version:Version of Record
Year of publishing:2020
Number of pages:13
Numbering:12
PID:20.500.12556/RUNG-5949 New window
COBISS.SI-ID:39882243 New window
DOI:10.3390/sym12121966 New window
NUK URN:URN:SI:UNG:REP:IWK3NYPC
Publication date in RUNG:28.11.2020
Views:2485
Downloads:92
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Record is a part of a journal

Title:Symmetry
Publisher:MDPI
Year of publishing:2020

Document is financed by a project

Funder:ARRS - Slovenian Research Agency
Project number:Z1-1853
Name:Unveiling the expansion of the Universe with strongly lensed supernovae

Licences

License:CC BY 4.0, Creative Commons Attribution 4.0 International
Link:http://creativecommons.org/licenses/by/4.0/
Description:This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Licensing start date:28.11.2020

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