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Record W2886533588 · doi:10.3847/1538-4357/ab2ae1

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

2019· article· en· W2886533588 on OpenAlexfundno aff

Bibliographic record

VenueThe Astrophysical Journal · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
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
KeywordsAccretion (finance)Spectral lineAccretion discBlack-body radiationRADIUSEmission spectrumLine (geometry)Luminosity

Abstract

fetched live from OpenAlex

Abstract 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 × 10 43 erg s −1 . PS18kh radiated E = (3.45 ± 0.22) × 10 50 erg over the period of observation, with (1.42 ± 0.20) × 10 50 erg being released during the rise to peak. Spectra of PS18kh show a changing, boxy/double-peaked H α emission feature, which becomes more prominent over time. We use models of non-axisymmetric accretion disks to describe the profile of the H α 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 ∼ 60 r g to an outer radius of r out ∼ 1400 r 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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.804
Threshold uncertainty score0.821

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.001

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 head0.008
GPT teacher head0.230
Teacher spread0.222 · 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 teacher head, 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

Citations103
Published2019
Admission routes1
Has abstractyes

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