Space/Science » Transient Alerts
Transient Alerts
Gamma-ray bursts, gravitational waves and other transients (NASA GCN), magnitude 6+ earthquakes (USGS), strong space weather (NOAA), bright supernovae and novae (IAU TNS), interstellar objects and bright comets (NASA/JPL). One thread per event; replies welcome.
- GRB 261005A Routine
In plain words: A burst of gamma rays, the most energetic form of light, reached Earth on 5 October 2026 and was recorded by three separate space telescopes: Fermi, Glowbug (an experiment on the International Space Station) and China's GECAM-B. Fermi places it in the constellation region around 22h 39m right ascension and +5.5 degrees declination, but only roughly, with an uncertainty of about 6 degrees. Fermi classed it as a likely long burst, the kind usually linked to the collapse of a massive star. Glowbug measured a single peak lasting about 5 seconds, and GECAM-B estimated about 9 seconds with a large margin of error. No distance, afterglow or visible-light counterpart has been reported so far.
How unusual is it? This is a typical single-pulse long gamma-ray burst, of a kind Fermi and Swift see a few hundred times a year, with only a rough location and no distance or afterglow reported. A measured distance or a detected afterglow would make it notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- EP261007a — GRB, X-ray Transient Routine
In plain words: A burst of X-rays was picked up by Einstein Probe, a Chinese-led space X-ray telescope, on 7 October 2026. The same spot on the sky was also linked to a gamma-ray burst seen by another satellite, SVOM. A follow-up X-ray telescope found a previously unknown X-ray source within the first position, which was in the southern sky at roughly right ascension 11.6 degrees, declination -17.7 degrees. About 8 hours after the trigger, a ground telescope at Xinglong Observatory in China detected a fading visible-light afterglow, about 20th magnitude, which is far too faint to see without a large telescope. Together these point to an ordinary gamma-ray burst, most likely from a distant exploding star. The reports give no distance yet, and no data on how long or how bright the burst was.
How unusual is it? A gamma-ray burst with an X-ray and optical afterglow is typical, since Fermi and Swift report a few hundred bursts a year and many have afterglows. A measured distance (redshift) or unusual brightness or duration would make it notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261007A — GRB, X-ray Transient Notable
In plain words: A burst of gamma rays, the most energetic form of light, was detected on 7 October 2026 by the SVOM satellite and by Fermi, with NuSTAR also catching it in its shield data. Einstein Probe saw it in X-rays too. It came from a spot in the southern sky, in the direction of the constellation Cetus. Telescopes quickly found a fading optical afterglow there, and the European Southern Observatory's Very Large Telescope measured its distance. The light left about 2.1 in redshift, a measure of how much the universe has stretched the light since it set out, which puts the burst very roughly 11 billion light-years away. The gamma rays lasted about 23 seconds and were fairly bright. This is most likely the death of a massive star collapsing into a black hole.
How unusual is it? A measured redshift (z = 2.101) and a bright, quickly found optical afterglow make this better studied than most gamma-ray bursts, which often have no distance. Otherwise it looks like an ordinary long burst from a collapsing massive star, so it is not exceptional.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261007A/EP261007a: Optical follow-up observations with Kinder
- GRB 261007A / EP261007a: SVOM/VT optical observations
- GRB 261007A: Swift-XRT afterglow detection
- GRB 261007A: SVOM/COLIBRÍ (FM-GFT) optical observations
- GRB 261007A / EP261007a: NuSTAR detection of prompt emission
- GRB 261007A / EP261007a: ULL-ASTRO-MASTER detection of the optical afterglow with LCO 40-cm telescope at McDonald Observatory
- Autonomous identification and follow-up of the counterpart to GRB 261007A by BTSbot with ZTF and P60/SEDM
- GRB 261007A: GROWTH-India Telescope optical observations
- GRB 261007A / EP261007a: TRT optical observations
- GRB 261007A: Swift ToO observations
- GRB 261007A: SVOM/C-GFT optical observations
- GRB 261007A / EP261007a: LCO optical observations
- GRB 261007A: WINTER J-band observations
- GRB 261007A: Fermi GBM observation
- GRB 261007A / EP261007a: VLT/X-shooter spectroscopic redshift z = 2.101
- GRB 261007A: KAIT optical counterpart candidate
- GRB 261007.27 Routine
In plain words: The SVOM satellite detected a burst of gamma rays, the most energetic form of light, on 7 October 2026. It came from a patch of sky in the southern constellation region near right ascension 00h 46m, declination -17.7 degrees, far from the plane of our Galaxy. About 28 minutes after the burst, a robotic telescope in Argentina (MASTER-OAFA) looked at that spot and saw no visible afterglow. It could only say that anything there was fainter than roughly magnitude 17 to 19.7, so no counterpart in visible light has been found yet. No distance or other details are given in this report.
How unusual is it? This is a typical gamma-ray burst report: the only follow-up is a visible-light non-detection, with no afterglow, distance measurement or other unusual feature. A redshift or an afterglow found by other telescopes would raise it to notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261007B Routine
In plain words: NASA's Fermi space telescope detected a burst of gamma rays, the most energetic form of light, on 7 October 2026 at 13:20 UT. The burst, named GRB 261007B, came from a patch of sky in the southern constellations, around 14h 48m right ascension and -54 degrees declination. That position is only rough, with an uncertainty of about 9 degrees, which is roughly the width of a fist held at arm's length. Fermi's team classes it as probably a long gamma-ray burst, the kind usually produced when a very massive star collapses. No other telescope has reported seeing it yet, and its distance is not known.
How unusual is it? Fermi and Swift together catch a few hundred gamma-ray bursts a year, and this is a typical Fermi detection with a coarse position and no follow-up yet. It would become notable if an afterglow were found in X-ray, optical or radio light, or if a distance (redshift) were measured.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261007.23 Routine
In plain words: A burst of gamma rays, the most energetic form of light, was detected by the SVOM satellite on 7 October 2026 at 05:53 UT, in the southern sky in the direction of the constellation Cetus. The robotic MASTER telescope in Argentina began looking at that spot about 16 minutes later and saw no visible light from it, down to about magnitude 21 (very faint, far beyond what the eye or binoculars can see). Later images got shallower because of observing conditions, and these limits are not detections. So no afterglow (the fading light that often follows a burst) has been found yet, and nothing is reported on what kind of burst it is or how far away it is. The observers say their analysis will continue.
How unusual is it? This is a typical gamma-ray burst with only a non-detection in visible light so far, with no distance, afterglow or unusual property reported. A found afterglow, a measured distance or an unusually long or bright burst would raise it to notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261005B Routine
In plain words: On the evening of 5 October 2026 (UTC), two space telescopes, NASA's Swift and Fermi, both caught a burst of gamma rays (the most energetic form of light) from a spot in the sky near the border of the constellations Ophiuchus and Hercules. The burst flickered with several peaks and lasted somewhere between about 20 and 90 seconds, depending on which instrument and energy range measured it. Swift's X-ray telescope found a fading X-ray afterglow and pinned its position to within about 2 arcseconds, but ultraviolet, optical and infrared searches hours later found no visible afterglow. No distance has been reported, so how far away it is remains unknown. It looks like an ordinary long gamma-ray burst, the kind usually linked to the death of a massive star.
How unusual is it? This is a typical gamma-ray burst: moderate brightness, an X-ray afterglow found, no visible-light afterglow and no distance measured. A redshift (distance) measurement or a supernova or other counterpart found later would make it more notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261002A — GRB, Gamma-ray Transient Routine
In plain words: NASA's Fermi space telescope detected a burst of gamma rays (the most energetic form of light) on 2 October 2026 at about 20:48 UT. It came from the direction of the constellation region near 10h 20m right ascension and about 2 degrees south of the celestial equator. The position is only rough, uncertain by about 5.5 degrees, which is roughly the width of a few fingers held at arm's length. The Fermi team classes it as a likely long gamma-ray burst, the kind usually linked to the collapse of a massive star. No distance, afterglow or follow-up observations are reported yet.
How unusual is it? This is one of the few hundred gamma-ray bursts Fermi and Swift catch each year, with only an initial rough location and no distance or counterpart reported. A measured distance or a found afterglow in other light would make it notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 261001A — GRB, Gamma-ray Transient Routine
In plain words: On 1 October 2026, a Chinese gamma-ray satellite called GECAM-B detected a burst of high-energy light, known as a gamma-ray burst. These bursts usually come from far outside our Galaxy, often from the collapse of a massive star. The burst came as several pulses and lasted about 42 seconds, which is why the team calls it a likely 'long' burst (one lasting more than about two seconds). The report gives no sky position, distance, or sign of a fading glow in X-ray, visible or radio light, so what exactly produced it is not yet known.
How unusual is it? This is a single detection of an ordinary long gamma-ray burst, a kind that Fermi and Swift together report a few hundred times a year. A measured distance or a bright afterglow found by other telescopes would make it notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 260930B — GRB, X-ray Transient Routine
In plain words: A short flash of gamma rays (the most energetic form of light) was recorded on 30 September 2026 by the SVOM satellite, and the same burst was also seen by two other spacecraft, Fermi and GECAM-B. The flash lasted under a second, with a few quick pulses followed by one more pulse. That points to the short type of gamma-ray burst, which is often linked to the merger of two dense stellar remnants, though the report does not say what caused this one. The position is only roughly known, somewhere in a patch of sky several degrees wide near the constellation region at coordinates RA 326, Dec +24, and it was outside the field of view of SVOM's sharper-eyed X-ray camera. No distance, afterglow or visible counterpart is mentioned in this report.
How unusual is it? This is an ordinary short gamma-ray burst of the kind Fermi and others catch many times a year, with a coarse position and no distance or afterglow reported. Finding an afterglow or a gravitational-wave signal at the same time and place would raise it to notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 260930A Routine
In plain words: NASA's Fermi Gamma-ray Burst Monitor, a space telescope that watches the whole sky for flashes of high-energy light, detected a gamma-ray burst on 30 September 2026. The flash is likely a 'long' burst, the kind that usually comes from a massive star collapsing. It came from a patch of sky in the constellation region around 11h 40m right ascension and about 7 degrees south of the celestial equator. That position is only rough, uncertain by about 8 degrees, which is roughly the width of a fist held at arm's length. This is the first, automatic report, and it says nothing yet about distance, brightness or any afterglow seen by other telescopes.
How unusual is it? Fermi and Swift together report a few hundred gamma-ray bursts a year, and this is a typical long burst with only a coarse position and no distance or counterpart reported. A measured distance or an afterglow found in other light would raise it to notable.
Written by an AI model from the official reports in this thread; it may contain mistakes.
- GRB 260924A
- GRB 260924A: VLA detection
- GRB 260924A: Swift/UVOT UV grism spectrum results
- GRB 260924A: AbAO optical observations
- GRB 260924A: Upper limits from a neutrino search with IceCube
- GRB 260924A: Near-infrared detection with MDM/MIRAGE
- GRB 260924A: COLIBRÍ optical observations
- GRB 260924A: Second-epoch J-band upper limit from the SYSU 80 cm infrared telescope
- Konus-Wind detection of GRB 260924A
- GRB 260924A: Extreme Isotropic-equivalent Gamma-ray Energy and encouragement for multiwavelength follow-up observations
- GRB 260924A: Optical follow-up observations with Kinder
- GRB 260924A: Ondrejov D50 optical afterglow detection
- GRB 260924A: SVOM/GRM observation
- GRB 260924A: 2.2m CAHA spectroscopic redshift z = 3.51
- GRB 260924A: J-band observations by the SYSU 80 cm infrared telescope
- GRB 260924A: Swift/UVOT Detection
- GRB 260924A: GROWTH-India Telescope optical observations
- GRB 260924A: Swift-BAT refined analysis
- GRB 260924A: NuSTAR detection of prompt emission
- GRB 260924A: Swift/UVOT Upper Limits
- GRB 260924A: Swift-XRT refined Analysis
- GRB 260924A: Fermi GRB Observation
- GRB 260924A: Fermi-LAT detection of a bright burst
- GRB 260924A: AstroSat CZTI detection
- GRB 260924A: NOT optical counterpart confirmation
- GRB 260924A: detection of a bright optical afterglow by the 1.5m OSN telescope
- GRB 260924A: Enhanced Swift-XRT position
- GRB 260924A: Swift detection of a burst
- GRB 260922A
- GRB 260922A: Glowbug gamma-ray detection
- Konus-Wind detection of GRB 260922A
- GRB 260922A: NuSTAR detection of prompt emission
- GRB 260922A: COLIBRÍ Confirmation of the Optical Counterpart
- GRB 260922A: CALET Gamma-Ray Burst Monitor detection
- GRB 260922A: Ondrejov D50 optical limit
- GRB 260922A: Swift-BAT refined analysis
- GRB 260922A: J-band upper limit with WINTER
- GRB 260922A: Swift/UVOT Upper Limits
- GRB 260922A: COLIBRÍ Optical Counterpart Candidate (correction to GCN 45698)
- GRB 260922A: COLIBRÍ optical upper limits
- GRB 260922A: Swift-XRT refined Analysis
- GRB 260922A: Enhanced Swift-XRT position
- GRB 260922A: SVOM/C-GFT optical upper limit
