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Record W4395485070 · doi:10.1093/mnras/stae927

Transient fading X-ray emission detected during the optical rise of a tidal disruption event

2024· article· en· W4395485070 on OpenAlexfundno aff
A. Malyali, A. Rau, Clément Bonnerot, A J Goodwin, Z Liu, G. E. Anderson, J. Brink, D. A. H. Buckley, A. Merloni, J. C. A. Miller‐Jones, I. Grotova, A. Kawka

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityRussian Academy of SciencesLeibniz-GemeinschaftScience and Technology Facilities CouncilOffice of ScienceJet Propulsion LaboratoryLeibniz-Institut für Astrophysik PotsdamUniversity of Illinois at Urbana-ChampaignRheinische Friedrich-Wilhelms-Universität BonnUniversity of LeicesterMax-Planck-GesellschaftDeutsches Zentrum für Luft- und RaumfahrtChinese Academy of SciencesHigh Energy PhysicsDeutsche ForschungsgemeinschaftCommonwealth Scientific and Industrial Research OrganisationQueen's University BelfastLawrence Berkeley National LaboratoryDivision of Astronomical SciencesFinanciadora de Estudos e ProjetosK2Nuclear Safety and Security CommissionUniversity of SussexAustralian Research CouncilSpace Telescope Science InstituteUniversity of PortsmouthCalifornia Institute of TechnologyUniversität HamburgNational Energy Research Scientific Computing CenterAspen Center for PhysicsSLAC National Accelerator LaboratoryQueen's UniversityOhio State UniversityUniversity of ChicagoNational Aeronautics and Space AdministrationCurtin University of TechnologyU.S. Department of EnergyFermilabNational Science Foundation
KeywordsPhysicsFadingTransient (computer programming)AstrophysicsEvent (particle physics)X-ray transientAstronomyTelecommunicationsNeutron star

Abstract

fetched live from OpenAlex

ABSTRACT We report on the SRG/eROSITA detection of ultra-soft ($kT=47^{+5}_{-5}$ eV) X-ray emission (LX =$2.5^{+0.6}_{-0.5} \times 10^{43}$ erg s−1) from the tidal disruption event (TDE) candidate AT 2022dsb ∼14 d before peak optical brightness. As the optical luminosity increases after the eROSITA detection, then the 0.2–2 keV observed flux decays, decreasing by a factor of ∼39 over the 19 d after the initial X-ray detection. Multi-epoch optical spectroscopic follow-up observations reveal transient broad Balmer emission lines and a broad He ii 4686 Å emission complex with respect to the pre-outburst spectrum. Despite the early drop in the observed X-ray flux, the He ii 4686 Å complex is still detected for ∼40 d after the optical peak, suggesting the persistence of an obscured hard ionizing source in the system. Three outflow signatures are also detected at early times: (i) blueshifted H α emission lines in a pre-peak optical spectrum, (ii) transient radio emission, and (iii) blueshifted Ly α absorption lines. The joint evolution of this early-time X-ray emission, the He ii 4686 Å complex, and these outflow signatures suggests that the X-ray emitting disc (formed promptly in this TDE) is still present after optical peak, but may have been enshrouded by optically thick debris, leading to the X-ray faintness in the months after the disruption. If the observed early-time properties in this TDE are not unique to this system, then other TDEs may also be X-ray bright at early times and become X-ray faint upon being veiled by debris launched shortly after the onset of circularization.

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: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.122
Threshold uncertainty score0.456

Codex and Gemma teacher scores by category

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

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 head0.005
GPT teacher head0.206
Teacher spread0.201 · 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 designSimulation or modeling
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

Citations14
Published2024
Admission routes1
Has abstractyes

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