The Astrophysical Journal Letters (Jan 2025)

EP240801a/XRF 240801B: An X-Ray Flash Detected by the Einstein Probe and the Implications of Its Multiband Afterglow

  • Shuai-Qing Jiang,
  • Dong Xu,
  • Agnes P. C. van Hoof,
  • Wei-Hua Lei,
  • Yuan Liu,
  • Hao Zhou,
  • Yong Chen,
  • Shao-Yu Fu,
  • Jun Yang,
  • Xing Liu,
  • Zi-Pei Zhu,
  • Alexei V. Filippenko,
  • Peter G. Jonker,
  • A. S. Pozanenko,
  • He Gao,
  • Xue-Feng Wu,
  • Bing Zhang,
  • Gavin P Lamb,
  • Massimiliano De Pasquale,
  • Shiho Kobayashi,
  • Franz Erik Bauer,
  • Hui Sun,
  • Giovanna Pugliese,
  • Jie An,
  • Valerio D’Elia,
  • Johan P. U. Fynbo,
  • WeiKang Zheng,
  • Alberto J. Castro-Tirado,
  • Yi-Han Iris Yin,
  • Yuan-Chuan Zou,
  • Adam T. Deller,
  • N. S. Pankov,
  • A. A. Volnova,
  • A. S. Moskvitin,
  • O. I. Spiridonova,
  • D. V. Oparin,
  • V. Rumyantsev,
  • O. A. Burkhonov,
  • Sh. A. Egamberdiyev,
  • V. Kim,
  • M. Krugov,
  • A. M. Tatarnikov,
  • R. Inasaridze,
  • Andrew J. Levan,
  • Daniele Bjørn Malesani,
  • Maria E. Ravasio,
  • Jonathan Quirola-Vásquez,
  • Joyce N. D. van Dalen,
  • Javi Sánchez-Sierras,
  • Daniel Mata Sánchez,
  • Stuart P. Littlefair,
  • Jennifer A. Chacón,
  • Manuel A. P. Torres,
  • Ashley A. Chrimes,
  • Nikhil Sarin,
  • Antonio Martin-Carrillo,
  • Vik Dhillon,
  • Yi Yang,
  • Thomas G. Brink,
  • Rebecca L. Davies,
  • Sheng Yang,
  • Amar Aryan,
  • Ting-Wan Chen,
  • Albert K. H. Kong,
  • Wen-Xiong Li,
  • Rui-Zhi Li,
  • Jirong Mao,
  • Ignacio Pérez-García,
  • Emilio J. Fernández-García,
  • Moira Andrews,
  • Joseph Farah,
  • Zhou Fan,
  • Estefania Padilla Gonzalez,
  • D. Andrew Howell,
  • Dieter Hartmann,
  • Jing-Wei Hu,
  • Páll Jakobsson,
  • Cheng-Kui Li,
  • Zhi-Xing Ling,
  • Curtis McCully,
  • Megan Newsome,
  • Benjamin Schneider,
  • Kaew Samaporn Tinyanont,
  • Ning-Chen Sun,
  • Giacomo Terreran,
  • Qing-Wen Tang,
  • Wen-Xin Wang,
  • Jing-Jing Xu,
  • Wei-Min Yuan,
  • Bin-Bin Zhang,
  • Hai-Sheng Zhao,
  • Juan Zhang

DOI
https://doi.org/10.3847/2041-8213/addebf
Journal volume & issue
Vol. 988, no. 1
p. L34

Abstract

Read online

We present multiband observations and analysis of EP240801a, a low-energy, extremely soft gamma-ray burst (GRB) discovered on 2024 August 1 by the Einstein Probe (EP) satellite with a weak contemporaneous signal also detected by the Fermi Gamma-ray Burst Monitor (GBM). Optical spectroscopy of the afterglow, obtained by Gran Telescopio Canarias and Keck, identified the redshift of z = 1.6734. EP240801a exhibits a burst duration of 148 s in X-rays and 22.3 s in gamma rays, with X-rays leading by 80.61 s. Spectral lag analysis indicates that the gamma-ray signal arrived 8.3 s earlier than the X-rays. Joint spectral fitting of EP Wide-field X-ray Telescope and Fermi/GBM data yields an isotropic energy ${E}_{\gamma ,{\rm{iso}}}=(5.5{7}_{-0.50}^{+0.54})\times 1{0}^{51}\,{\rm{erg}}$ , a peak energy ${E}_{{\rm{peak}}}=14.9{0}_{-4.71}^{+7.08}\,{\rm{keV}}$ , and a fluence ratio S (25–50 keV)/ S $(50\,\unicode{x02013}\,100\,{\rm{keV}})=1.6{7}_{-0.46}^{+0.74}$ , classifying EP240801a as an X-ray flash (XRF). The host-galaxy continuum spectrum, inferred using Prospector , was used to correct its contribution for the observed outburst optical data. Unusual early R -band behavior and EP Follow-up X-ray Telescope observations suggest multiple components in the afterglow. Three models are considered: a two-component jet model, a forward-reverse shock model, and a forward shock model with energy injection. All three provide reasonable explanations. The two-component jet model and the energy injection model imply a relatively small initial energy and velocity of the jet in the line of sight, while the forward-reverse shock model remains typical. Under the two-component jet model, EP240801a may resemble GRB 221009A (BOAT) if the bright narrow beam is viewed on-axis. Therefore, EP240801a can be interpreted as an off-beam (narrow) jet or an intrinsically weak GRB jet. Our findings provide crucial clues for uncovering the origin of XRFs.

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