Optical/Infrared Observations of the Extraordinary GRB 250702B: A Highly Obscured Afterglow in a Massive Galaxy Consistent with Multiple Possible Progenitors

Abstract GRB 250702B was the longest gamma-ray burst ever detected, with a duration that challenges standard collapsar models and suggests an exotic progenitor. We collected a rich set of optical and infrared follow-up observations of its rapidly fading afterglow using a suite of telescopes including the W. M. Keck Observatory, the Gemini telescopes, the Magellan Baade Telescope, the Victor M. Blanco 4 m telescope, and the Fraunhofer Telescope at Wendelstein Observatory. Our analysis reveals that the afterglow emission is well described by forward shock emission from a highly obscured relativistic jet. Deep photometric observations of the host galaxy reveal a massive (10 10.66 M ⊙ ), dusty, and extremely asymmetric system that is consistent with two galaxies undergoing a major merger. The galactocentric offset, host galaxy properties, and jet characteristics disfavor a jetted tidal disruption event (TDE) around a supermassive black hole but do not definitively distinguish between competing progenitor scenarios. We find that the afterglow and host are consistent with a range of progenitors, including an atypical collapsar, a merger between a helium star and a stellar-mass black hole, the disruption of a star by a stellar-mass compact object (micro-TDE), and the tidal disruption of a star by an off-nuclear intermediate-mass black hole.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-11-26
DOI
https://doi.org/10.3847/2041-8213/ae1d67
Citations
3
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
3.46
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article

Optical/Infrared Observations of the Extraordinary GRB 250702B: A Highly Obscured Afterglow in a Massive Galaxy Consistent with Multiple Possible Progenitors

C. D. Kilpatrick, Silona Wilke, G. Damke, Weicheng Zang et al.
3 citations
The Astrophysical Journal Letters
Gamma-ray bursts and supernovae
3.46
article

Optical/Infrared Observations of the Extraordinary GRB 250702B: A Highly Obscured Afterglow in a Massive Galaxy Consistent with Multiple Possible Progenitors

C. D. Kilpatrick, Silona Wilke, G. Damke, Weicheng Zang, Xander J. Hall, Kritti Sharma, Jonathan Carney, D. Gruen, A. Riffeser, Akash Anumarlapudi, Steve Heathcote, Hank Corbett, Ramandeep Gill, James Freeburn, Christopher J. Conselice, Kaustav K. Das, Nicholas M. Law, A. Palmese, Brendan O’Connor, A. Gal‐Yam, Lei Hu, Kathleen Labrie, Igor Andreoni, Eric R. Coughlin, Hannah Skobe, Dheeraj R. Pasham, Paz Beniamini, Viraj Karambelkar, M. J. Schmidt, Tomás Ahumada, Lewi Westcott, Ping Chen, M. M. Kasliwal, Malte Busmann
article en
3 citations

Abstract

Abstract GRB 250702B was the longest gamma-ray burst ever detected, with a duration that challenges standard collapsar models and suggests an exotic progenitor. We collected a rich set of optical and infrared follow-up observations of its rapidly fading afterglow using a suite of telescopes including the W. M. Keck Observatory, the Gemini telescopes, the Magellan Baade Telescope, the Victor M. Blanco 4 m telescope, and the Fraunhofer Telescope at Wendelstein Observatory. Our analysis reveals that the afterglow emission is well described by forward shock emission from a highly obscured relativistic jet. Deep photometric observations of the host galaxy reveal a massive (10 10.66 M ⊙ ), dusty, and extremely asymmetric system that is consistent with two galaxies undergoing a major merger. The galactocentric offset, host galaxy properties, and jet characteristics disfavor a jetted tidal disruption event (TDE) around a supermassive black hole but do not definitively distinguish between competing progenitor scenarios. We find that the afterglow and host are consistent with a range of progenitors, including an atypical collapsar, a merger between a helium star and a stellar-mass black hole, the disruption of a star by a stellar-mass compact object (micro-TDE), and the tidal disruption of a star by an off-nuclear intermediate-mass black hole.

The Astrophysical Journal LettersVol. 994(2)
Northwestern University (US), University of North Carolina at Chapel Hill (US), California Institute of Technology (US), Open University of Israel (IL), George Washington University (US), University of Manchester (GB), Excellence Cluster Origins (DE), Gemini North Observatory (US), Center for Astrophysics Harvard & Smithsonian (US), Cerro Tololo Inter-American Observatory (CL), Eureka Scientific (US), Weizmann Institute of Science (IL), Syracuse University (US), Carnegie Mellon University (US), Zhejiang University (CN), Ludwig-Maximilians-Universität München (DE), Universidad Nacional Autónoma de México (MX)
Openalex Percentile: Top 7%
Gamma-ray bursts and supernovae
3.46
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