Journal article icon

Journal article

On the Nature of Einstein Probe Transient EP250916a: Insights from X-Ray, Optical, and Radio Observations

Abstract:
Abstract We report multiwavelength studies of the transient EP250916a, detected by the Einstein Probe on 2025 September 16. Located at low Galactic latitude, the source exhibited a rapid X-ray brightening, reaching an unabsorbed 0.5–10 keV flux of (6.4 ± 0.1) × 10 −10  erg cm −2  s −1 , followed by a plateau and a two-stage decay lasting over 40 days. Swift/X-Ray Telescope (XRT) monitoring shows a persistently hard spectrum (Γ ≈ 1.6–2.2) with only modest softening during decay, while a Nuclear Spectroscopic Telescope Array (NuSTAR)  observation confirms a hard-state continuum extending up to 70 keV. Timing analysis of XMM-Newton data reveals a weak quasiperiodic oscillation (QPO) at ∼13 Hz. No other coherent pulsations or thermonuclear bursts are detected. Broadband spectral modeling favors a nonthermal power-law continuum with partial-covering absorption and shows no significant thermal disk component. Optical imaging obtained with Nordic Optical Telescope, Las Campanas Observatory, and GaiaDR3 identifies two faint sources within the 2″ Swift/XRT positional uncertainty. A MeerKAT observation at 1.28 GHz yielded no radio counterpart, with a 3 σ upper limit of 60  μ Jy beam −1 . The combination of a long-lasting outburst, a hard nonthermal X-ray spectrum, a weak QPO detection, the absence of coherent timing features, and faint potential optical counterparts disfavors a stellar-flare or extragalactic origin and supports an accreting compact-object scenario. Comparisons with similar faint, hard-state transients place EP250916a within a growing population of low-luminosity, hard-state black hole X-ray binary candidates.
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.3847/1538-4357/ae7a58

Authors

More by this author
Role:
Author
ORCID:
0000-0002-6789-2723
More by this author
Role:
Author
ORCID:
0000-0003-4795-7072
More by this author
Role:
Author
ORCID:
0000-0002-0426-3276
More by this author
Role:
Author
ORCID:
0000-0002-3500-631X


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
1005
Issue:
2
Pages:
161-161
Publication date:
2026-07-02
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


Language:
English
Keywords:
Pubs id:
2442369
Local pid:
pubs:2442369
Source identifiers:
W7167063085
Deposit date:
2026-07-08
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP