GRB 160625B

GRB 160625B
Typical Gamma-Ray Burst (illustration)
Event type Gamma-ray burst Edit this on Wikidata
Right ascension 20h 34m 23.25s
Declination +06° 55 ′ 10.5″
Other designations GRB 160625B

GRB 160625B was a bright gamma-ray burst (GRB) detected by NASA's Fermi Gamma-ray Space Telescope on 25 June 2016 and, three minutes later, by the Large Area Telescope. This was followed by a bright prompt optical flash, during which variable linear polarization was measured. This was the first time that these observations were made when the GRB was still bright and active. The source of the GRB was a possible black hole, within the Delphinus constellation, about 9 billion light-years (light travel distance) away (a redshift of z = 1.406). It had a fluence of 5.7×10−4 erg cm−2, and energy of 5 × 1054 erg.

See also