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Record W4413756402 · doi:10.1051/0004-6361/202555892

A real-time search for Type Ia Supernovae with late-time interactions with circumstellar material in ZTF data

2025· article· en· W4413756402 on OpenAlexfundno aff
J. Terwel, K. Maguire, S. Brennan, L. Galbany, Simeon Reusch, S. Schulze, Niilo Koivisto, Tapio Pursimo, Søren Sørensen, María Alejandra Díaz Teodori, Astrid Guldberg Theil, Mikael Turkki, T. E. Müller-Bravo, U. Burgaz, Young-Lo Kim, J. S. Bloom, Matthew J. Graham, M. M. Kasliwal, Shri Kulkarni, Frank J. Masci, Josiah Purdum, O. Pyshna, Avery Wold

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionAgència de Gestió d'Ajuts Universitaris i de RecercaAgencia Estatal de InvestigaciónScience Mission DirectorateSmithsonian Astrophysical ObservatoryInstituto de Astrofísica de CanariasMax-Planck-Institut für AstronomieEötvös Loránd TudományegyetemStockholms UniversitetHORIZON EUROPE Framework ProgrammeHáskóli ÍslandsUniversitetet i OsloMax-Planck-GesellschaftNational Central UniversityNational Research Foundation of KoreaQueen's UniversityNational Research FoundationGordon and Betty Moore FoundationQueen's University BelfastSpace Telescope Science InstituteLos Alamos National LaboratoryAlfred P. Sloan FoundationJohns Hopkins UniversityEuropean CommissionSmithsonian InstitutionU.S. Department of EnergyCalifornia Institute of TechnologyHorizon 2020 Framework ProgrammeTurun YliopistoAarhus UniversitetUniversity of WarwickNorthwestern UniversityDurham UniversityDrexel UniversityNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsAstrophysicsSupernovaType (biology)Astronomy

Abstract

fetched live from OpenAlex

While it is generally accepted that Type Ia supernovae (SNe Ia) are the terminal explosions of white dwarfs (WDs), the nature of their progenitor systems and the mechanisms that lead up to these explosions remain widely debated. In rare cases, the SN ejecta interact with circumstellar material (CSM) that had previously been ejected from the progenitor system. The longer the delay between the creation of the CSM and the SN explosion, the greater the distance between the SN explosion site and the CSM and the later the onset of the interaction. The unknown distance between the CSM and SN explosion site makes it impossible to predict when the interaction will start. If the time between the SN explosion and the onset of the CSM interaction is of the order of several months to years, the SN has generally faded and it is no longer actively followed up on. This makes it even more difficult to detect the interaction while it is happening. In this work, we report on a real-time monitoring programme running between 13 November 2023 and 9 July 2024. It monitored 6914 SNe Ia for signs of late-time rebrightening using the Zwicky Transient Facility (ZTF). Flagged candidates were rapidly followed up on with photometry and spectroscopy to confirm the late-time excess and its position. We report the discovery of a ∼50 day rebrightening event in SN 2020qxz around 1200 rest-frame days after the peak of its light curve. SN 2020qxz exhibited signs of an early CSM interaction, but had faded from view over two years before its reappearance. Initial follow-up spectroscopy revealed the presence of four emission lines, while later follow-up spectroscopy showed that these had faded shortly after the end of the ZTF-detected rebrightening event. Our best match for these emission lines are Hβ (blueshifted by ∼5900 km s−1) and Ca IIλ8542, N Iλ8567, and K Iλλ8763, 8767 (all blueshifted by 5100 km s−1; although we note that the line identifications are uncertain). This shows that catching and following up on late-time interactions as they occur can offer new clues on the nature of the progenitor systems that produce these SNe by putting constraints on the possible type of donor star. The only way to do this systematically is to use large sky surveys such as ZTF and the upcoming Vera C. Rubin Observatory’s Legacy Survey of Space and Time (LSST) to monitor a large sample of objects for the rare events that reappear long after the object has faded from view.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.012
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0010.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.016
GPT teacher head0.265
Teacher spread0.249 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations2
Published2025
Admission routes1
Has abstractyes

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