_version_ 1866912490853498880
author Levan, Andrew J.
Martin-Carrillo, Antonio
Laskar, Tanmoy
Eyles-Ferris, Rob A. J.
Sneppen, Albert
Ravasio, Maria Edvige
Rastinejad, Jillian C.
Bright, Joe S.
Carotenuto, Francesco
Chrimes, Ashley A.
Corcoran, Gregory
Gompertz, Benjamin P.
Jonker, Peter G.
Lamb, Gavin P.
Malesani, Daniele B.
Saccardi, Andrea
Sierras, Javier Sanchez
Schneider, Benjamin
Schulze, Steve
Tanvir, Nial R.
Vergani, Susana D.
Watson, Darach
An, Jie
Bauer, Franz E.
Campana, Sergio
Cotter, Laura
van Dalen, Joyce N. D.
D'Elia, Valerio
de Pasquale, Massimiliano
Postigo, Antonio de Ugarte
Dimple
Hartmann, Dieter H.
Hjorth, Jens
Izzo, Luca
Jakobsson, Pall
Kumar, Amit
Melandri, Andrea
O'Brien, Paul
Piranomonte, Silvia
Pugliese, Giovanna
Quirola-Vasquez, Jonathan
Starling, Rhaana
Tagliaferri, Gianpiero
Xu, Dong
Wortley, Makenzie E.
author_facet Levan, Andrew J.
Martin-Carrillo, Antonio
Laskar, Tanmoy
Eyles-Ferris, Rob A. J.
Sneppen, Albert
Ravasio, Maria Edvige
Rastinejad, Jillian C.
Bright, Joe S.
Carotenuto, Francesco
Chrimes, Ashley A.
Corcoran, Gregory
Gompertz, Benjamin P.
Jonker, Peter G.
Lamb, Gavin P.
Malesani, Daniele B.
Saccardi, Andrea
Sierras, Javier Sanchez
Schneider, Benjamin
Schulze, Steve
Tanvir, Nial R.
Vergani, Susana D.
Watson, Darach
An, Jie
Bauer, Franz E.
Campana, Sergio
Cotter, Laura
van Dalen, Joyce N. D.
D'Elia, Valerio
de Pasquale, Massimiliano
Postigo, Antonio de Ugarte
Dimple
Hartmann, Dieter H.
Hjorth, Jens
Izzo, Luca
Jakobsson, Pall
Kumar, Amit
Melandri, Andrea
O'Brien, Paul
Piranomonte, Silvia
Pugliese, Giovanna
Quirola-Vasquez, Jonathan
Starling, Rhaana
Tagliaferri, Gianpiero
Xu, Dong
Wortley, Makenzie E.
contents Gamma-ray bursts (GRBs) are singular outbursts of high-energy radiation with durations typically lasting from milliseconds to minutes and, in extreme cases, a few hours. They are attributed to the catastrophic outcomes of stellar-scale events and, as such, are not expected to recur. Here, we present observations of an exceptional GRB\,250702BDE which triggered the {\em Fermi} gamma-ray burst monitor on three occasions over several hours, and which was detected in soft X-rays by the \textit{Einstein Probe} a day before the $γ$-ray triggers (EP250702a). We present the discovery of an extremely red infrared counterpart of the event with the VLT, as well as radio observations from MeerKAT. Hubble Space Telescope observations pinpoint the source to a non-nuclear location in a host galaxy with complex morphology, implying GRB 250702BDE is an extragalactic event. The multi-wavelength counterpart is well described with standard afterglow models at a relatively low redshift $z \sim 0.2$, but the prompt emission does not readily fit within the expectations for either collapsar or merger-driven GRBs. Indeed, a striking feature of the multiple prompt outbursts is that the third occurs at an integer multiple of the interval between the first two. Although not conclusive, this could be indicative of periodicity in the progenitor system. We discuss several possible scenarios to explain the exceptional properties of the burst, which suggest that either a very unusual collapsar or the tidal disruption of a white dwarf by an intermediate-mass black hole are plausible explanations for this unprecedented GRB.
format Preprint
id arxiv_https___arxiv_org_abs_2507_14286
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The day-long, repeating GRB 250702BDE / EP250702a: A unique extragalactic transient
Levan, Andrew J.
Martin-Carrillo, Antonio
Laskar, Tanmoy
Eyles-Ferris, Rob A. J.
Sneppen, Albert
Ravasio, Maria Edvige
Rastinejad, Jillian C.
Bright, Joe S.
Carotenuto, Francesco
Chrimes, Ashley A.
Corcoran, Gregory
Gompertz, Benjamin P.
Jonker, Peter G.
Lamb, Gavin P.
Malesani, Daniele B.
Saccardi, Andrea
Sierras, Javier Sanchez
Schneider, Benjamin
Schulze, Steve
Tanvir, Nial R.
Vergani, Susana D.
Watson, Darach
An, Jie
Bauer, Franz E.
Campana, Sergio
Cotter, Laura
van Dalen, Joyce N. D.
D'Elia, Valerio
de Pasquale, Massimiliano
Postigo, Antonio de Ugarte
Dimple
Hartmann, Dieter H.
Hjorth, Jens
Izzo, Luca
Jakobsson, Pall
Kumar, Amit
Melandri, Andrea
O'Brien, Paul
Piranomonte, Silvia
Pugliese, Giovanna
Quirola-Vasquez, Jonathan
Starling, Rhaana
Tagliaferri, Gianpiero
Xu, Dong
Wortley, Makenzie E.
High Energy Astrophysical Phenomena
Gamma-ray bursts (GRBs) are singular outbursts of high-energy radiation with durations typically lasting from milliseconds to minutes and, in extreme cases, a few hours. They are attributed to the catastrophic outcomes of stellar-scale events and, as such, are not expected to recur. Here, we present observations of an exceptional GRB\,250702BDE which triggered the {\em Fermi} gamma-ray burst monitor on three occasions over several hours, and which was detected in soft X-rays by the \textit{Einstein Probe} a day before the $γ$-ray triggers (EP250702a). We present the discovery of an extremely red infrared counterpart of the event with the VLT, as well as radio observations from MeerKAT. Hubble Space Telescope observations pinpoint the source to a non-nuclear location in a host galaxy with complex morphology, implying GRB 250702BDE is an extragalactic event. The multi-wavelength counterpart is well described with standard afterglow models at a relatively low redshift $z \sim 0.2$, but the prompt emission does not readily fit within the expectations for either collapsar or merger-driven GRBs. Indeed, a striking feature of the multiple prompt outbursts is that the third occurs at an integer multiple of the interval between the first two. Although not conclusive, this could be indicative of periodicity in the progenitor system. We discuss several possible scenarios to explain the exceptional properties of the burst, which suggest that either a very unusual collapsar or the tidal disruption of a white dwarf by an intermediate-mass black hole are plausible explanations for this unprecedented GRB.
title The day-long, repeating GRB 250702BDE / EP250702a: A unique extragalactic transient
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2507.14286