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Record W4406267199 · doi:10.1051/0004-6361/202452571

ZTF SN Ia DR2: Properties of the low-mass host galaxies of Type Ia supernovae in a volume-limited sample

2025· article· en· W4406267199 on OpenAlexaff
U. Burgaz, K. Maguire, G. Dimitriadis, J. Sollerman, L. Galbany, M. Rigault, A. Goobar, Young-Lo Kim, A. Alburai, M. Amenouche, M. Deckers, M Ginolin, L. Harvey, T. E. Müller-Bravo, J. Nordin, Kim Phan, P. Rosnet, P.E. Nugent, J. Terwel, M. J. Graham, David Hale, M. Kasliwal, Russ R. Laher, J.D. Neill, Josiah Purdum, B. Rusholme

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsHerzberg Institute of Astrophysics
FundersAgencia Estatal de InvestigaciónDeutsches Elektronen-SynchrotronHorizon 2020 Framework ProgrammeH2020 European Research CouncilStockholms UniversitetMinisterio de Ciencia e InnovaciónKnut och Alice Wallenbergs StiftelseTrinity College DublinIrish Research CouncilCalifornia Institute of TechnologyEuropean CommissionInstitut National de Physique Nucléaire et de Physique des ParticulesVetenskapsrådetUniversity of WarwickNorthwestern UniversityScience and Technology Facilities CouncilWeizmann Institute of ScienceAgència de Gestió d'Ajuts Universitaris i de RecercaNational Science FoundationUniversity of WashingtonGordon and Betty Moore Foundation
KeywordsPhysicsAstrophysicsSupernovaGalaxySample (material)Host (biology)Type (biology)Volume (thermodynamics)Astronomy

Abstract

fetched live from OpenAlex

In this study, we explore the characteristics of ‘low-mass’ (log( M ⋆ / M ⊙ ) ≤ 8) and ‘intermediate-mass’ (8 < log( M ⋆ / M ⊙ ) ≤ 10) host galaxies of Type Ia supernovae (SNe Ia) from the second data release (DR2) of the Zwicky Transient Facility survey. We investigated their correlations with different sub-types of SNe Ia. We used the photospheric velocities measured from the Si II λ 6355 feature, SALT2 light-curve stretch ( x 1 ), and host-galaxy properties of SNe Ia to re-investigate the existing relationship between host galaxy mass and Si II λ 6355 velocities. We also investigated sub-type preferences for host populations. We show that the more energetic and brighter 91T-like SNe Ia tend to reside among the younger host populations, while 91bg-like SNe Ia are found among the older populations. Our findings suggest that high-velocity SNe Ia (HV SNe Ia) do indeed come from older populations, but they can also come from young populations as well. Therefore, while our findings can partly provide support for HV SNe Ia in the context of single degenerate progenitor models, they indicate that HV SNe Ia (rather than comprising a different population) might be a continued distribution with different explosion mechanisms. Lastly, we investigate the specific rate of SNe Ia in the volume-limited SN Ia sample of DR2 and compare our results with other surveys.

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 score0.006
Threshold uncertainty score0.011

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.008
GPT teacher head0.209
Teacher spread0.201 · 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

Citations6
Published2025
Admission routes1
Has abstractyes

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