The Astrophysical Journal Letters (Jan 2025)

Characterization of a Peculiar Einstein Probe Transient EP240408a: An Exotic Gamma-Ray Burst or an Abnormal Jetted Tidal Disruption Event?

  • Brendan O’Connor,
  • Dheeraj Pasham,
  • Igor Andreoni,
  • Jeremy Hare,
  • Paz Beniamini,
  • Eleonora Troja,
  • Roberto Ricci,
  • Dougal Dobie,
  • Joheen Chakraborty,
  • Mason Ng,
  • Noel Klingler,
  • Viraj Karambelkar,
  • Sam Rose,
  • Steve Schulze,
  • Geoffrey Ryan,
  • Simone Dichiara,
  • Itumeleng Monageng,
  • David Buckley,
  • Lei Hu,
  • Gokul P. Srinivasaragavan,
  • Gabriele Bruni,
  • Tomás Cabrera,
  • S. Bradley Cenko,
  • Hendrik van Eerten,
  • James Freeburn,
  • Erica Hammerstein,
  • Mansi Kasliwal,
  • Chryssa Kouveliotou,
  • Keerthi Kunnumkai,
  • James K. Leung,
  • Amy Lien,
  • Antonella Palmese,
  • Takanori Sakamoto

DOI
https://doi.org/10.3847/2041-8213/ada7f5
Journal volume & issue
Vol. 979, no. 2
p. L30

Abstract

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We present the results of our multiwavelength (X-ray to radio) follow-up campaign of the Einstein Probe transient EP240408a. The initial 10 s trigger displayed bright soft X-ray (0.5–4 keV) radiation with peak luminosity L _X ≳ 10 ^49 (10 ^50 ) erg s ^−1 for an assumed redshift z ≳ 0.5 (2.0). The Neil Gehrels Swift Observatory and Neutron star Interior Composition ExploreR discovered a fading X-ray counterpart lasting for ∼5 days (observer frame), which showed a long-lived (∼4 days) plateau-like emission ( t ^−0.5 ) before a sharp power-law decline ( t ^−7 ). The plateau emission was in excess of L _X ≳ 10 ^46 (10 ^47 ) erg s ^−1 at z ≳ 0.5 (2.0). Deep optical and radio observations resulted in nondetections of the transient. Our observations with Gemini South revealed a faint potential host galaxy ( r ≈ 24 AB mag) near the edge of the X-ray localization. The faint candidate host, and lack of other potential hosts ( r ≳ 26 AB mag; J ≳ 23 AB mag), imply a higher redshift origin ( z ≳ 0.5), which produces extreme X-ray properties that are inconsistent with many known extragalactic transient classes. In particular, the lack of a bright gamma-ray counterpart, with the isotropic-equivalent energy (10–10,000 keV) constrained by GECam and Konus-Wind to E _γ _,iso ≲ 4 × 10 ^50 (6 × 10 ^51 ) erg at z ≈ 0.5 (2.0), conflicts with known gamma-ray bursts of similar X-ray luminosities. We therefore favor a jetted tidal disruption event as the progenitor of EP240408a at z ≳ 1.0, possibly caused by the disruption of a white dwarf by an intermediate-mass black hole. The alternative is that EP240408a may represent a new, previously unknown class of transient.

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