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Record W4389979069 · doi:10.3847/1538-4357/ad0153

Strong Carbon Features and a Red Early Color in the Underluminous Type Ia SN 2022xkq

2023· article· en· W4389979069 on OpenAlexafffund
Jeniveve Pearson, David J. Sand, Peter Lundqvist, L. Galbany, Jennifer E. Andrews, K. Azalee Bostroem, Yize Dong, Emily Hoang, G. Hosseinzadeh, Daryl Janzen, J. Jencson, M. Lundquist, Darshana Mehta, N. Meza, Manisha Shrestha, S. Valenti, S. Wyatt, J. P. Anderson, C. Ashall, Katie Auchettl, E. Baron, S. Blondin, C. R. Burns, Yongzhi Cai, T. W. Chen, Laura Chomiuk, D. A. Coulter, Dane Cross, Kyle W. Davis, Thomas de Jaeger, James M. DerKacy, D. Desai, G. Dimitriadis, A. Do, Joseph Farah, R. J. Foley, M. Gromadzki, C. P. Gutiérrez, J. Haislip, J. I. Gónzalez Hernández, Jason T. Hinkle, W. B. Hoogendam, D. A. Howell, P. Hoêflich, E. Y. Hsiao, M. E. Huber, Saurabh W. Jha, Cristina Jiménez-Palau, C. D. Kilpatrick, Vladimir Kouprianov, Sahana Kumar, Lindsey A. Kwok, Conor Larison, Natalie LeBaron, X. K. Le Saux, Jing Lü, C. McCully, Tycho Mera Evans, Peter Milne, M. Modjaz, N. Morrell, T. E. Müller-Bravo, Megan Newsome, M. Nicholl, Estefania Padilla Gonzalez, A. V. Payne, C. Pellegrino, Kim Phan, Jonathan Pineda-García, Anthony L. Piro, L. Piscarreta, Abigail Polin, D. Reichart, C. Rojas-Bravo, S. D. Ryder, I. Salmaso, Michaela Schwab, Melissa Shahbandeh, B. J. Shappee, M. R. Siebert, Nathan Smith, Jay Strader, K. Taggart, G. Terreran, Samaporn Tinyanont, M. A. Tucker, G. Valerin, D. R. Young

Bibliographic record

VenueThe Astrophysical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of Saskatchewan
FundersEuropean Social FundAgencia Estatal de InvestigaciónConsejo Superior de Investigaciones CientíficasJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilUniversity of North Carolina at Chapel HillAgencia Nacional de Investigación y DesarrolloAstrophysics DivisionIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueNuclear Safety and Security CommissionMinistério da Ciência, Tecnologia e InovaçãoCommonwealth Scientific and Industrial Research OrganisationQueen's University BelfastAustralian GovernmentHeising-Simons FoundationSpace Telescope Science InstituteVetenskapsrådetSmithsonian InstitutionJohn Templeton FoundationNational Natural Science Foundation of ChinaArizona Board of RegentsLeibniz-GemeinschaftUniversity of Notre DameQueen's UniversityJet Propulsion LaboratoryLeibniz-Institut für Astrophysik PotsdamUniversity of California, Santa CruzOhio State UniversityNational Science FoundationUniversity of MinnesotaCentre National d’Etudes SpatialesAspen Center for PhysicsCollege of Engineering, Michigan State UniversityUniversità degli Studi di PadovaMinistero dell’Istruzione, dell’Università e della RicercaAlfred P. Sloan FoundationMinisterio de Ciencia e InnovaciónEuropean CommissionPrecursory Research for Embryonic Science and TechnologyCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationMichigan State University
KeywordsPhysicsSupernovaAstrophysicsLight curveWhite dwarfPair-instability supernovaSpectral lineAstronomyInfraredEjectaStars

Abstract

fetched live from OpenAlex

Abstract We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining Type Ia supernova (SN Ia) in NGC 1784 (D ≈ 31 Mpc), from <1 to 180 days after explosion. The high-cadence observations of SN 2022xkq, a photometrically transitional and spectroscopically 91bg-like SN Ia, cover the first days and weeks following explosion, which are critical to distinguishing between explosion scenarios. The early light curve of SN 2022xkq has a red early color and exhibits a flux excess that is more prominent in redder bands; this is the first time such a feature has been seen in a transitional/91bg-like SN Ia. We also present 92 optical and 19 near-infrared (NIR) spectra, beginning 0.4 days after explosion in the optical and 2.6 days after explosion in the NIR. SN 2022xkq exhibits a long-lived C i 1.0693 μm feature that persists until 5 days post-maximum. We also detect C ii λ6580 in the pre-maximum optical spectra. These lines are evidence for unburnt carbon that is difficult to reconcile with the double detonation of a sub-Chandrasekhar mass white dwarf. No existing explosion model can fully explain the photometric and spectroscopic data set of SN 2022xkq, but the considerable breadth of the observations is ideal for furthering our understanding of the processes that produce faint SNe Ia.

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)0.000
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 score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.015
GPT teacher head0.252
Teacher spread0.237 · 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

Citations10
Published2023
Admission routes2
Has abstractyes

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