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Record W4409553986 · doi:10.1051/0004-6361/202553768

4XMM J181330.1−175110: A new supergiant fast X-ray transient

2025· article· en· W4409553986 on OpenAlexfundno aff
M. Marelli, L. Sidoli, M. Polletta, A. De Luca, R. Salvaterra, A. Gargiulo

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersLos Alamos National LaboratoryPlanetary Science DivisionScience Mission DirectorateJet Propulsion LaboratorySmithsonian Astrophysical ObservatoryMax-Planck-Institut für AstronomieGordon and Betty Moore FoundationNational Central UniversitySpace Telescope Science InstituteQueen's UniversityJohns Hopkins UniversityQueen's University BelfastNational Aeronautics and Space AdministrationEötvös Loránd TudományegyetemCalifornia Institute of TechnologyDurham UniversitySmithsonian InstitutionNational Science Foundation
KeywordsPhysicsSupergiantAstrophysicsX-ray transientTransient (computer programming)AstronomyBlue supergiantStarsNeutron starRed supergiant

Abstract

fetched live from OpenAlex

Context. Supergiant fast X-ray transients (SFXTs) are a subclass of high-mass X-ray binaries (HMXBs) in which a compact object accretes part of the clumpy wind of the blue supergiant companion, triggering series of brief X-ray flares lasting a few kiloseconds. Currently, only about 15 SFXTs are known. Aims. The EXTraS (Exploring the X-ray Transient and variable Sky) catalog provides the timing signatures of every source observed by the EPIC instrument onboard XMM-Newton. Among the most peculiar sources in terms of variability, we identified a new member of the SFXT family: 4XMM J181330.1−175110 (J1813). Methods. We analyzed all publicly available XMM-Newton, Chandra, Swift, and NuSTAR data pointed at the J1813 position to determine the source’s duty cycle and to provide a comprehensive description of its timing and spectral behavior during its active phase. Additionally, we searched for the optical and infrared counterpart of the X-ray source in public databases and fitted its spectral energy distribution (SED). Results. The optical-to-mid infrared SED of J1813 is consistent with a highly absorbed (AV ∼ 38) B0 star at ∼10 kpc. During its X-ray active phase, the source is characterized by continuous thousands seconds-long flares with peak luminosities (2–12 keV) ranging from 1034 to 4 × 1035 erg s−1. Its X-ray spectrum is consistent with a high-absorbed power-law model with NH ∼ 1.8 × 1023 cm−2 and Γ ∼ 1.66. No spectral variability was observed as a function of time or flux. J1813 is in a quiescent state ∼60% of the time, with an upper-limit luminosity of 8 × 1032 erg s−1 (at 10 kpc), implying an observed long-term X-ray flux variability > 500. Conclusions. The optical counterpart alone indicates J1813 is an HMXB. Its transient nature, duty cycle, the amplitude of observed X-ray variability, the shape and luminosity of the X-ray flares – and the lack of known X-ray outbursts (> 1036 erg s−1) – strongly support the identification of J1813 as an SFXT.

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)0.000
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 score0.004
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.002
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.007
GPT teacher head0.208
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 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

Citations0
Published2025
Admission routes1
Has abstractyes

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