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Record W3104491049

PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk

2019· article· en· W3104491049 on OpenAlexfundno aff
T. W. S. Holoien, M. E. Huber, B. J. Shappee, Michael Eracleous, Katie Auchettl, M. A. Tucker, K. C. Chambers, C. S. Kochanek, K. Z. Stanek, A. Rest, D. Bersier, R. S. Post, G. Aldering, K. A. Ponder, Joshua D. Simon, E. Kankare, Dillon Dong, Gregg Hallinan, Naveen A. Reddy, Ryan L. Sanders, J. Bulger, T. Lowe, E. A. Magnier, A. S. B. Schultz, C. Waters, M. Willman, D. E. Wright, D. R. Young, Subo Dong, J. L. Prieto, Todd A. Thompson, L. Denneau, H. Flewelling, A. Heinze, S. J. Smartt, B. Stalder, J. Tonry, H. Weiland

Bibliographic record

VenueeScholarship (California Digital Library) · 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 AstronomieEötvös Loránd TudományegyetemMax-Planck-GesellschaftQueen's UniversityChinese Academy of SciencesIstituto Nazionale di AstrofisicaDurham UniversitySpace Telescope Science InstituteNew Mexico State UniversityUniversity of California, Los AngelesUniversity of PortsmouthCenter for Cosmology and Astroparticle Physics, Ohio State UniversityNational Central UniversityVillum FondenScience and Technology Facilities CouncilUniversität BaselFermilabLiverpool John Moores UniversityUniversity of MinnesotaNational Science FoundationCase Western Reserve UniversityUniversity of Notre DameUniversity of PittsburghLos Alamos National LaboratoryPrinceton UniversityAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityOhio State UniversityDrexel UniversityU.S. Naval ObservatoryNational Natural Science Foundation of ChinaU.S. Department of EnergySmithsonian InstitutionEuropean CommissionCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationChinese Academy of Sciences South America Center for AstronomyQueen's University BelfastGordon and Betty Moore Foundation
KeywordsPhysicsRotational symmetryAccretion discAccretion (finance)AstrophysicsAstronomyEvent (particle physics)Mechanics
DOInot available

Abstract

fetched live from OpenAlex

We present the discovery of PS18kh, a tidal disruption event discovered at the center of SDSS J075654.53+341543.6 (d ≃ 322 Mpc) by the Pan-STARRS Survey for Transients. Our data set includes pre-discovery survey data from Pan-STARRS, the All-sky Automated Survey for Supernovae, and the Asteroid Terrestrial-impact Last Alert System as well as high-cadence, multiwavelength follow-up data from ground-based telescopes and Swift, spanning from 56 days before peak light until 75 days after. The optical/UV emission from PS18kh is well-fit as a blackbody with temperatures ranging from T ≃ 12,000 K to T ≃ 25,000 K and it peaked at a luminosity of L ≃ 8.8 × 1043 erg s-1. PS18kh radiated E = (3.45 ± 0.22) × 1050 erg over the period of observation, with (1.42 ± 0.20) × 1050 erg being released during the rise to peak. Spectra of PS18kh show a changing, boxy/double-peaked Hα emission feature, which becomes more prominent over time. We use models of non-axisymmetric accretion disks to describe the profile of the Hα line and its evolution. We find that at early times the high accretion rate leads the disk to emit a wind which modifies the shape of the line profile and makes it bell-shaped. At late times, the wind becomes optically thin, allowing the non-axisymmetric perturbations to show up in the line profile. The line-emitting portion of the disk extends from r in ∼ 60r g to an outer radius of r out ∼ 1400r g and the perturbations can be represented either as an eccentricity in the outer rings of the disk or as a spiral arm in the inner disk.

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)0.002
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.006
Threshold uncertainty score0.021

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0020.001
Insufficient payload (model declined to judge)0.0060.002

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 head0.007
GPT teacher head0.206
Teacher spread0.199 · 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

Citations35
Published2019
Admission routes1
Has abstractyes

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