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Record W2975493583 · doi:10.1093/mnras/stz2742

Lick Observatory Supernova Search follow-up program: photometry data release of 93 Type Ia supernovae

2019· article· en· W2975493583 on OpenAlexfundno aff
Benjamin E. Stahl, WeiKang Zheng, Thomas de Jaeger, A. V. Filippenko, A. Bigley, Kyle Blanchard, P. K. Blanchard, Thomas G. Brink, S.K. Cargill, Chadwick Casper, Sanyum Channa, Byung Yun Choi, Nick Choksi, J. Chu, K. I. Clubb, Daniel P. Cohen, Michael Ellison, Edward Falcon, Pegah Fazeli, Kiera Fuller, M. Ganeshalingam, E. L. Gates, Carolina Gould, Goni Halevi, Kevin T Hayakawa, Julia Hestenes, Benjamin T. Jeffers, N. Joubert, M. T. Kandrashoff, Minkyu Kim, Haejung Kim, Michelle E Kislak, I. K. W. Kleiser, Jason Kong, Maxime de Kouchkovsky, Daniel Krishnan, Sahana Kumar, Joel Leja, Erin Leonard, Gary Li, Weidong Li, Philip Lu, M. Mason, Jeffrey Molloy, Kenia Pina, J. Rex, Timothy W. Ross, Samantha Stegman, Kevin Tang, P. Thrasher, Xiang-Gao Wang, Andrew Wilkins, Heechan Yuk, Sameen Yunus, Keto Zhang

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionScience Mission DirectorateSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryMax-Planck-Institut für AstrophysikEötvös Loránd TudományegyetemNational Central UniversityMax-Planck-GesellschaftGordon and Betty Moore FoundationQueen's University BelfastMax-Planck-Institut für AstronomieUniversity of EdinburghSpace Telescope Science InstituteNew Mexico State UniversityU.S. Naval ObservatorySmithsonian InstitutionU.S. Department of EnergyNational Natural Science Foundation of ChinaUniversity of PittsburghLos Alamos National LaboratoryUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationSilicon Valley Community FoundationJohns Hopkins UniversityUniversity of ChicagoCalifornia Institute of TechnologyDurham UniversityNational Aeronautics and Space AdministrationQueen's UniversityAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyHeising-Simons FoundationFermilabNational Science Foundation
KeywordsSupernovaPhysicsPhotometry (optics)Light curveObservatoryAstrophysicsAstronomyRedshiftStarsGalaxy

Abstract

fetched live from OpenAlex

ABSTRACT We present BVRI and unfiltered light curves of 93 Type Ia supernovae (SNe Ia) from the Lick Observatory Supernova Search (LOSS) follow-up program conducted between 2005 and 2018. Our sample consists of 78 spectroscopically normal SNe Ia, with the remainder divided between distinct subclasses (3 SN 1991bg-like, 3 SN 1991T-like, 4 SNe Iax, 2 peculiar, and 3 super-Chandrasekhar events), and has a median redshift of 0.0192. The SNe in our sample have a median coverage of 16 photometric epochs at a cadence of 5.4 d, and the median first observed epoch is ∼4.6 d before maximum B-band light. We describe how the SNe in our sample are discovered, observed, and processed, and we compare the results from our newly developed automated photometry pipeline to those from the previous processing pipeline used by LOSS. After investigating potential biases, we derive a final systematic uncertainty of 0.03 mag in BVRI for our data set. We perform an analysis of our light curves with particular focus on using template fitting to measure the parameters that are useful in standardizing SNe Ia as distance indicators. All of the data are available to the community, and we encourage future studies to incorporate our light curves in their analyses.

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)0.002
metaresearch head score (Gemma)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Dataset · Consensus signal: none
Teacher disagreement score0.035
Threshold uncertainty score0.070

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0060.004
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0060.005

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 head0.027
GPT teacher head0.265
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 designNot applicable
Domainnot available
GenreDataset

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

Citations82
Published2019
Admission routes1
Has abstractyes

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