| Title: | Spectroscopic analysis of the strongly lensed SN Encore : constraints on cosmic evolution of Type Ia supernovae |
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| Authors: | ID Dhawan, S. (Author)
ID Pierel, Justin (Author)
ID Gu, M. (Author)
ID Newman, A. B. (Author)
ID Larison, C. (Author)
ID Siebert, M. (Author)
ID Petrushevska, Tanja (Author)
ID Poidevin, F. (Author)
ID Jha, S. W. (Author)
ID Chen, W. (Author) |
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| Files: |  SN_Encore_Spectra__MNRAS.pdf (6,45 MB)
MD5: 540D72DF4A87C9B66AF94B6F298F52A1
 https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae2434/60184772/stae2434.pdf
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae2434/60184772/stae2434.pdf
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| Language: | English |
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| Work type: | Unknown |
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| Typology: | 1.01 - Original Scientific Article |
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| Organization: | UNG - University of Nova Gorica
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| Abstract: | Abstract
Strong gravitational lensing magnifies the light from a background source, allowing us to study these sources in detail. Here, we study the spectra of a z = 1.95 lensed Type Ia supernova SN Encore for its brightest Image A, taken 39 days apart. We infer the spectral age with template matching using the supernova identification (SNID) software and find the spectra to be at 29.0 ±5.0 and 37.4 ±2.8 rest-frame days post maximum respectively, consistent with separation in the observer frame after accounting for time-dilation. Since SNe Ia measure dark energy properties by providing relative distances between low- and high-z SNe, it is important to test for evolution of spectroscopic properties. Comparing the spectra to composite low-z SN Ia spectra, we find strong evidence for similarity between the local sample and SN Encore. The line velocities of common SN Ia spectral lines, Si II 6355 and Ca II NIR triplet are consistent with the distribution for the low-z sample as well as other lensed SNe Ia, e.g. iPTF16geu (z = 0.409)and SN H0pe (z = 1.78). The consistency between the low-z sample and lensed SNe at high-z suggests no obvious cosmic evolution demonstrating their using as high-z distance indicators, though this needs to be confirmed/refuted via a larger sample. We also find that the spectra of SN Encore match the predictions for explosion models very well. With future large samples of lensed SNe Ia e.g. with the Vera C. Rubin Observatory, spectra at such late phases will be important to distinguish between different explosion scenarios. |
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| Keywords: | Encore |
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| Publication status: | Published |
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| Publication version: | Author Accepted Manuscript |
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| Publication date: | 01.01.2024 |
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| Year of publishing: | 2024 |
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| Number of pages: | str. 1-9 |
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| Numbering: | Vol. , issue |
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| PID: | 20.500.12556/RUNG-9444  |
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| COBISS.SI-ID: | 213339139 |
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| UDC: | 52 |
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| ISSN on article: | 0035-8711 |
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| DOI: | 10.1093/mnras/stae2434 |
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| NUK URN: | URN:SI:UNG:REP:JDUDGYBX |
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| Publication date in RUNG: | 29.10.2024 |
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| Views: | 428 |
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| Downloads: | 1 |
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