The Astrophysical Journal Letters (Jan 2024)

Discovery of the Optical and Radio Counterpart to the Fast X-Ray Transient EP 240315a

  • J. H. Gillanders,
  • L. Rhodes,
  • S. Srivastav,
  • F. Carotenuto,
  • J. Bright,
  • M. E. Huber,
  • H. F. Stevance,
  • S. J. Smartt,
  • K. C. Chambers,
  • T.-W. Chen,
  • R. Fender,
  • A. Andersson,
  • A. J. Cooper,
  • P. G. Jonker,
  • F. J. Cowie,
  • T. de Boer,
  • N. Erasmus,
  • M. D. Fulton,
  • H. Gao,
  • J. Herman,
  • C.-C. Lin,
  • T. Lowe,
  • E. A. Magnier,
  • H.-Y. Miao,
  • P. Minguez,
  • T. Moore,
  • C.-C. Ngeow,
  • M. Nicholl,
  • Y.-C. Pan,
  • G. Pignata,
  • A. Rest,
  • X. Sheng,
  • I. A. Smith,
  • K. W. Smith,
  • J. L. Tonry,
  • R. J. Wainscoat,
  • J. Weston,
  • S. Yang,
  • D. R. Young

DOI
https://doi.org/10.3847/2041-8213/ad55cd
Journal volume & issue
Vol. 969, no. 1
p. L14

Abstract

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Fast X-ray Transients (FXTs) are extragalactic bursts of soft X-rays first identified ≳10 yr ago. Since then, nearly 40 events have been discovered, although almost all of these have been recovered from archival Chandra and XMM-Newton data. To date, optical sky surveys and follow-up searches have not revealed any multiwavelength counterparts. The Einstein Probe, launched in 2024 January, has started surveying the sky in the soft X-ray regime (0.5–4 keV) and will rapidly increase the sample of FXTs discovered in real time. Here we report the first discovery of both an optical and radio counterpart to a distant FXT, the fourth source publicly released by the Einstein Probe. We discovered a fast-fading optical transient within the 3′ localization radius of EP 240315a with the all-sky optical survey ATLAS, and our follow-up Gemini spectrum provides a redshift, z = 4.859 ± 0.002. Furthermore, we uncovered a radio counterpart in the S band (3.0 GHz) with the MeerKAT radio interferometer. The optical (rest-frame UV) and radio luminosities indicate that the FXT most likely originates from either a long gamma-ray burst or a relativistic tidal disruption event. This may be a fortuitous early mission detection by the Einstein Probe or may signpost a mode of discovery for high-redshift, high-energy transients through soft X-ray surveys, combined with locating multiwavelength counterparts.

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