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Journal article

SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise

Abstract:

Moore et al.We present multiwavelength photometry and spectroscopy of SN 2022jli, an unprecedented Type Ic supernova discovered in the galaxy NGC 157 at a distance of ≈ 23 Mpc. The multiband light curves reveal many remarkable characteristics. Peaking at a magnitude of g = 15.11 ± 0.02, the high-cadence photometry reveals periodic undulations of 12.5 ± 0.2 days superimposed on the 200-day supernova decline. This periodicity is observed in the light curves from nine separate filter and instrum...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/2041-8213/acfc25

Authors


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Role:
Author
ORCID:
https://orcid.org/0000-0001-8385-3727
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Institution:
University of Oxford
Role:
Author
ORCID:
https://orcid.org/0000-0002-8229-1731
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Role:
Author
ORCID:
https://orcid.org/0000-0002-2555-3192
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Role:
Author
ORCID:
https://orcid.org/0000-0003-4524-6883
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Institution:
University of Oxford
Role:
Author
ORCID:
https://orcid.org/0000-0002-0504-4323


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Funder identifier:
https://ror.org/05nqkay65
Grant:
19054
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Funder identifier:
https://ror.org/027ka1x80
Grant:
80NSSC18K1575
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Funder identifier:
https://ror.org/02ap3w078
Grant:
ICN12_009


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal Letters More from this journal
Volume:
956
Issue:
1
Publication date:
2023-10-01
DOI:
EISSN:
2041-8213
ISSN:
2041-8205


Language:
English
Pubs id:
1560613
Local pid:
pubs:1560613
Source identifiers:
W4387613311
Deposit date:
2025-06-14
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

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