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Record W789144982 · doi:10.1093/mnras/stv2486

Six months of multiwavelength follow-up of the tidal disruption candidate ASASSN-14li and implied TDE rates from ASAS-SN

2015· article· en· W789144982 on OpenAlexfundno aff
T. W. S. Holoien, C. S. Kochanek, J. L. Prieto, K. Z. Stanek, Subo Dong, B. J. Shappee, D. Grupe, J. S. Brown, U. Basu, J. F. Beacom, D. Bersier, J. Brimacombe, A. B. Danilet, E. Falco, Zhen Guo, Jessy Jose, Gregory J. Herczeg, Feng Long, G. Pojmański, G. Simonian, D. Szczygiel, Todd A. Thompson, J. R. Thorstensen, R. M. Wagner, P. R. Woźniak

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersBrookhaven National LaboratoryScience and Technology Facilities CouncilCenter for Cosmology and Astroparticle Physics, Ohio State UniversityNational Science FoundationLiverpool John Moores UniversityChinese Academy of SciencesYork UniversitySpace Telescope Science InstituteCarnegie Mellon UniversityOffice of SciencePennsylvania State UniversityLos Alamos National LaboratoryCollege of Engineering, Michigan State UniversityPrinceton UniversityUniversity of WashingtonAlfred P. Sloan FoundationJohns Hopkins UniversityHarvard UniversityOhio State UniversityNational Aeronautics and Space AdministrationLawrence Berkeley National LaboratoryUniversity of PennsylvaniaNew Mexico State UniversityUniversity of California, Los AngelesUniversity of PortsmouthYale UniversityVanderbilt UniversityU.S. Department of EnergyCalifornia Institute of TechnologyJet Propulsion Laboratory
KeywordsPhysicsAstrophysicsSupernovaLuminosityGalaxyBalmer seriesEmission spectrumLight curveAstronomySpectral line

Abstract

fetched live from OpenAlex

We present ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the centre of PGC 043234 (d ≃ 90 Mpc) by the All-Sky Automated Survey for SuperNovae (ASAS-SN). The source had a peak bolometric luminosity of L ≃ 1044 erg s−1 and a total integrated energy of E ≃ 7 × 1050 erg radiated over the ∼6 months of observations presented. The UV/optical emission of the source is well fitted by a blackbody with roughly constant temperature of T ∼ 35 000 K, while the luminosity declines by roughly a factor of 16 over this time. The optical/UV luminosity decline is broadly consistent with an exponential decline, |$L\propto \text{e}^{-t/t_0}$|⁠, with t0 ≃ 60 d. ASASSN-14li also exhibits soft X-ray emission comparable in luminosity to the optical and UV emission but declining at a slower rate, and the X-ray emission now dominates. Spectra of the source show broad Balmer and helium lines in emission as well as strong blue continuum emission at all epochs. We use the discoveries of ASASSN-14li and ASASSN-14ae to estimate the TDE rate implied by ASAS-SN, finding an average rate of r ≃ 4.1 × 10−5 yr−1 per galaxy with a 90 per cent confidence interval of (2.2–17.0) × 10−5 yr−1 per galaxy. ASAS-SN found roughly 1 TDE for every 70 Type Ia supernovae in 2014, a rate that is much higher than that of other surveys.

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)0.001
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 score0.007
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
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 science0.0000.001
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 head0.011
GPT teacher head0.224
Teacher spread0.212 · 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

Citations326
Published2015
Admission routes1
Has abstractyes

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