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Discovery of a Likely Type II Supernova at z = 3.6 with JWST

Abstract:
Transient astronomy of the early, high-redshift (z > 3) Universe is an unexplored regime that offers the possibility of probing the first stars and the epoch of reionization. During Cycles 1 and 2 of the James Webb Space Telescope (JWST), the JWST Advanced Deep Extragalactic Survey program enabled one of the first searches for transients in deep images (∼30 AB mag) over a relatively wide area (25 arcmin2). One transient, AT 2023adsv, was discovered with an F200W magnitude of 28.04 AB mag, and subsequent JWST observations revealed that the transient is a likely supernova (SN) in a host with zspec = 3.613 ± 0.001 and an inferred metallicity at the position of the SN of Z* = 0.3 ± 0.1 Z⊙. At this redshift, the first detections in F115W and F150W show that AT 2023adsv had bright rest-frame UV flux at the time of discovery. The multiband light curve of AT 2023adsv is best matched by a template of a Type IIP SN (SN IIP) with a peak absolute magnitude of MB ≈ −18.3 AB mag. We find a good match to a 20 M⊙ red supergiant progenitor star with an explosion energy of 2 × 1051 erg, likely higher than normally observed in the local Universe, but consistent with SNe IIP drawn from local, lower-metallicity environments. AT 2023adsv is the most distant photometrically classified SN IIP yet discovered with a spectroscopic redshift measurement, and may represent a global shift in SN IIP properties as a function of redshift.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/ae595d

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Author
ORCID:
0000-0003-4263-2228
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Role:
Author
ORCID:
0000-0002-2361-7201
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Author
ORCID:
0000-0002-4781-9078
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Role:
Author
ORCID:
0000-0003-1169-1954
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Role:
Author
ORCID:
0000-0003-2445-3891


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Funder identifier:
10.13039/501100000288
Grant:
G125142
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Funder identifier:
10.13039/100000893
Grant:
NAS5-02015
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Funder identifier:
10.13039/100000104
Grant:
NAS 5-03127


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
1002
Issue:
1
Pages:
83
Article number:
83
Publication date:
2026-04-28
Acceptance date:
2026-03-26
DOI:
EISSN:
1538-4357
ISSN:
0004637X, 0004-637X


Language:
English
Keywords:
Pubs id:
2419657
Local pid:
pubs:2419657
Source identifiers:
3991763
Deposit date:
2026-04-28
ARK identifier:
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