The January 29, 2025 gamma-ray burst observed by TAROT telescopes

At 4:45 a.m. on January 29, 2025, the Swift satellite detected a gamma-ray burst from the explosion of a star 11 billion light-years away.

IRAP operates the TAROT telescope network, made up of four observatories around the world connected to the events detected by the Swift satellite.

One hundred seconds after its explosion, the gamma-ray burst was observed by both TAROT telescopes in Chile and the Calern observatory in France. The first measurements are simultaneous with the gamma-ray emission, which lasted an exceptional duration of 200 seconds. The optical emission was followed by TAROT for three hours, and its evolution promises an interesting physical interpretation.

The 1-metre telescope on the Pic du Midi was also used over the following days, enabling us to follow the decrease in brightness for up to eight days after the burst.

The illustration shows the incredible perspective offered by three stars, apparently close together in the image, but so far apart when their distances are considered.

The TAROT network is operated by CNRS in collaboration with CNES.

IRAP Contact

More news

Unprecedented mineral and organic compounds discovered in Mars’ Jezero Crater

The Perseverance rover has uncovered sedimentary rocks containing minerals and organic matter organized into structures never before seen on Mars, opening up new perspectives on the Red Planet’s past habitability. […]

Juno identifies the missing auroral footprint of the moon Callisto at Jupiter’s poles

Since July 2016, the Juno mission orbiting Jupiter has been studying the properties and physical mechanisms of auroral imprints. A study recently published in the journal Nature Communications shows that […]

Deep long-period earthquakes discovered beneath Massif Central volcanoes

A recent study published in Geophysical Research Letters reveals atypical seismic signals beneath the volcanoes of the Massif Central. These signals, combined with the active presence of magma at depth, […]

Search