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Record W4220716814 · doi:10.1093/mnras/stac723

The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe

2022· article· en· W4220716814 on OpenAlexfundno aff
WeiKang Zheng, Benjamin E. Stahl, Thomas de Jaeger, A. V. Filippenko, Shan-Qin Wang, Wen-Pei Gan, Thomas G. Brink, Ivan Altunin, Raphael Baer-Way, A. Bigley, Kyle Blanchard, P. K. Blanchard, J. Chester Bradley, S.K. Cargill, Chadwick Casper, T. Chapman, Vidhi Chander, Sanyum Channa, Byung Yun Choi, Nick Choksi, Matthew R. Chu, K. I. Clubb, Daniel P. Cohen, Paul A. Dalba, Asia deGraw, Maxime de Kouchkovsky, Michael Ellison, Edward Falcon, Ori D. Fox, Kiera Fuller, M. Ganeshalingam, Nachiket Girish, Carolina Gould, Goni Halevi, Andrew Halle, Kevin T Hayakawa, Romain Hardy, Julia Hestenes, Andrew M. Hoffman, Michael E. Hyland, Benjamin T. Jeffers, Connor Jennings, M. T. Kandrashoff, Anthony Khodanian, Minkyu Kim, Haejung Kim, Michelle E Kislak, Daniel Krishnan, Sahana Kumar, Snehaa Ganesh Kumar, Joel Leja, Erin Leonard, Gary Li, Weidong Li, Ji-Shun Lian, Evelyn Liu, T. Lowe, Philip Lu, Emily Ma, M. Mason, Michael R. May, Kyle McAllister, Emma McGinness, Shaunak Modak, Jeffrey Molloy, Yukei S. Murakami, Omnarayani Nayak, Derek Perera, Kenia Pina, Druv H. Punjabi, A. Rikhter, Timothy W. Ross, Jackson Sipple, Costas Soler, Samantha Stegman, Haynes Stephens, James Sunseri, Kevin Tang, Stephen R. Taylor, P. Thrasher, Schuyler D. Van Dyk, Xiang-Gao Wang, Jeremy Wayland, Andrew Wilkins, Abel Yagubyan, Heechan Yuk, Sameen Yunus, Keto Zhang

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionScience Mission DirectorateSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryMax-Planck-GesellschaftSmithsonian InstitutionU.S. Department of EnergyNational Natural Science Foundation of ChinaGordon and Betty Moore FoundationQueen's University BelfastSpace Telescope Science InstituteLos Alamos National LaboratoryAlfred P. Sloan FoundationSilicon Valley Community FoundationJohns Hopkins UniversityFermilabNational Science FoundationNational Aeronautics and Space AdministrationGoogleUniversity of ChicagoUniversity of CaliforniaQueen's UniversityAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyCalifornia Institute of TechnologySun MicrosystemsEötvös Loránd TudományegyetemMax-Planck-Institut für AstronomieUniversity of California BerkeleyHewlett-Packard Development CompanyNational Central University
KeywordsPhotometry (optics)SupernovaPhysicsEjectaAstrophysicsLight curveObservatoryBrightnessAstronomyGalaxyStars

Abstract

fetched live from OpenAlex

ABSTRACT We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.

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)0.002
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 score0.019
Threshold uncertainty score0.037

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0070.006

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 head0.028
GPT teacher head0.256
Teacher spread0.228 · 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

Citations14
Published2022
Admission routes1
Has abstractyes

Explore more

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