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SN 2024bfu, SN 2025qe, and the early light curves of type Iax supernovae

Abstract:
Type Iax supernovae (SNe Iax) are one of the most common subclasses of thermonuclear supernova and yet their sample size, particularly those observed shortly after explosion, remains relatively small. In this paper, we present photometric and spectroscopic observations of two SNe Iax discovered shortly after explosion, SN 2024bfu and SN 2025qe. Both SNe were observed by multiple all-sky surveys, enabling tight constraints on the moment of first light and the shape of the early light curve. Our observations of SN 2025qe begin <2 d after the estimated time of first light and represent some of the earliest observations of any SN Iax. Spectra show features consistent with carbon absorption throughout the evolution of SN 2025qe, potentially indicating the presence of unburned material throughout the ejecta. We gather a sample of SNe Iax observed by the Asteroid Terrestrial-impact Last Alert System (ATLAS), Gravitational-wave Optical Transient Observer (GOTO), and Zwicky Transient Facility (ZTF) shortly after explosion and measure their rise times and early light curve power-law rise indices. We compare our results to a sample of normal SNe Ia and find indications that SNe Iax show systematically shorter rise times, consistent with previous work. We also find some indication that SNe Iax show systematically lower rise indices than normal SNe Ia. The low rise indices observed among SNe Iax are qualitatively consistent with extended Ni distributions and more thoroughly-mixed ejecta compared to normal SNe Ia, similar to predictions from pure deflagration explosions.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/staf1675

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Role:
Author
ORCID:
0000-0002-0629-8931
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Role:
Author
ORCID:
0000-0002-0440-9597
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Role:
Author
ORCID:
0000-0003-4663-4300


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Funder identifier:
https://ror.org/057g20z61
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Funder identifier:
https://ror.org/02ap3w078
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Funder identifier:
https://ror.org/02gn6ta77
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Funder identifier:
https://ror.org/001aqnf71


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
543
Issue:
4
Pages:
3731-3753
Publication date:
2025-10-03
Acceptance date:
2025-09-28
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
UUID:
uuid_aae60e87-ac74-49e5-aeb7-3dc50f1c41af
Source identifiers:
3396121
Deposit date:
2025-10-22
ARK identifier:
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