Transient Alerts — HabitableZone

Transient Alerts » in reply to GRB 261010A

In plain words Notable

On 10 October 2026 several gamma-ray satellites (Fermi, Swift, Konus-Wind and others) recorded a burst of gamma rays in the constellation Hercules that lasted about a minute. Swift's X-ray telescope and ground telescopes quickly found a fading X-ray and optical afterglow, which confirms the position. The host galaxy is uncertain: it is either a nearby galaxy about 25 arcseconds away at redshift 0.070, or a fainter galaxy 2 arcseconds away at redshift 0.785, meaning the light left roughly 7 billion years ago. Several teams say the burst's flash pattern and energy look more like those of a merger of two compact stars (such as neutron stars) than the collapse of a massive star, even though the burst was long. No kilonova (the glow from freshly made heavy elements after a merger) has been seen, and radio searches found nothing; the deep, late near-infrared images are too shallow to rule one out.

How unusual is it? A long gamma-ray burst with an optical afterglow, a measured redshift, and several independent analyses pointing to a merger origin is out of the ordinary, but no kilonova has been seen and the host is unconfirmed. It would become exceptional if a kilonova were confirmed, and would drop back toward routine if the burst were shown to come from a collapsing massive star.

Written by an AI model (claude-sonnet-5-5) from the official reports in this thread, and rewritten as new reports arrived (version 9); last updated . It may contain mistakes: the reports themselves are the authority.

GRB 261010A: ASKAP non-detection of a radio afterglow

GCN Circular 45953
GRB 261010A: ASKAP non-detection of a radio afterglow
From: Dougal Dobie at University of Sydney
Issued: 2026-10-16 02:10 UTC
Type: GRB, Afterglow, Radio Transient

D. Dobie (University of Sydney/OzGrav) and J. Freeburn (UNC Chapel Hill)

We report follow-up of GRB 261010A using the Australian SKA Pathfinder (ASKAP) from 04:40-10:19 UTC on 2026-10-14.

No radio emission is detected at the position of the optical counterpart (GCN 45890, GCN 45891) with a 3-sigma upper limit of 135 uJy at 943 MHz.

The observational data is publicly available on the CSIRO ASKAP Science Data Archive under SBID 89348.

Thank you to CSIRO staff for supporting these observations.

Every one of the gamma-ray bursts GCN reports is posted here.
Relayed automatically from NASA's General Coordinates Network.

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