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Record W4417405840 · doi:10.1051/0004-6361/202556425

Normal or transitional? The evolution and properties of two type Ia supernovae in the Virgo cluster

2025· article· en· W4417405840 on OpenAlexafffund
L. Izzo, C. Gall, N. Khetan, N. Earl, J. Hjorth, W. B. Hoogendam, Yi Ni, Aidan Sedgewick, Shane Ward, Y. Zenati, K. Auchettl, S. Bhattacharjee, S. Benetti, M. Branchesi, E. Cappellaro, Alberico L. Catapano, K. C. Chambers, Douglas A. Coulter, Kelcey Davis, M. Della Valle, Serene Dhawan, Thomas de Boer, G. Dimitriadis, R. J. Foley, M. Fulton, Hua Gao, W. J. Hon, C. Lin, R. Margutti, A. Reguitti, C. Rojas-Bravo, M. R. Siebert, S. Srivastav, Jonathan Swift, K. Taggart, G. Terreran, Stephen Thorp, L. Tomasella

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of Toronto
FundersPlanetary Science DivisionUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstronomieEötvös Loránd TudományegyetemStockholms UniversitetUniversitetet i OsloLos Alamos National LaboratoryJohns Hopkins UniversityUniversità degli Studi di PadovaEuropean Research CouncilGordon and Betty Moore FoundationQueen's University BelfastUniversity of CambridgeNational Science FoundationUK Research and InnovationScience Mission DirectorateGovernment of the United KingdomNational Centre for Supercomputing ApplicationsNational Central UniversityVillum FondenEuropean CommissionCalifornia Institute of TechnologySmithsonian InstitutionU.S. Department of EnergyScience and Technology Facilities CouncilTurun YliopistoAarhus UniversitetInstitut sur la Nutrition et les Aliments FonctionnelsQueen's UniversityUniversity of California, Santa CruzHORIZON EUROPE Framework ProgrammeHáskóli ÍslandsNuclear Safety and Security CommissionHeising-Simons FoundationSpace Telescope Science InstituteW. M. Keck FoundationNational Aeronautics and Space AdministrationDurham University
KeywordsSupernovaVirgo ClusterPopulationLight curveBrightnessCluster (spacecraft)HomogeneousPair-instability supernova

Abstract

fetched live from OpenAlex

Type Ia supernovae (SNe Ia) are among the most precise cosmological distance indicators used to study the expansion history of the Universe. The vast increase in SN Ia data due to large-scale astrophysical surveys has led to the discovery of a wide variety of SN Ia sub-classes, such as transitional and fast-declining SNe Ia. However, their distinct photometric and spectroscopic properties differentiate them from the population of normal SNe Ia such that their use as cosmological tools remains challenged. Here, we present a high-cadenced photometric and spectroscopic dataset of two SNe Ia, SNe 2020ue and 2020nlb, which were discovered in the nearby Virgo cluster of galaxies. Our study shows that SN 2020nlb is a normal SN Ia whose unusually red colour is intrinsic, arising from a lower photospheric temperature rather than interstellar reddening, providing clear evidence that colour diversity among normal SNe Ia can have a physical origin. In contrast, SN 2020ue has photometric properties, such as colour evolution and light curve decay rate, similar to those of transitional SNe. It is hence more spectroscopically aligned with normal SNe Ia. This is evident from spectroscopic indicators such as the pseudo-equivalent width of Si II lines. Thus, such SNe Ia, which lie photometrically at the edge of the standard normal SNe Ia range, may be missed in cosmological SNe Ia samples. Our results highlight that a spectroscopic analysis of SNe Ia around peak brightness is crucial for identifying intrinsic colour variations and constructing a more complete and physically homogeneous SN Ia sample for precision cosmology.

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)0.000
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 score0.010
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.010
GPT teacher head0.222
Teacher spread0.212 · 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

Citations1
Published2025
Admission routes2
Has abstractyes

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