Discovery of the most distant very-high-energy gamma-ray blazar with LST-1
Published 2023-12-28The extreme Universe will never cease to amaze us! The LST-1 telescope has detected significant gamma-ray emission from the distant blazar OP 313, discovering for the first time this source in the very-high-energy gamma-ray band (see the published ATel). It is also the first discovery made by the LST-1 telescope of the Cherenkov Telescope Array Observatory (CTAO). This detection comes after several days of enhanced activity from this source observed by the Fermi-LAT telescope.
This motivated the observations performed by LST-1 between December 10th and December 14th, resulting in the detection of this source for the very first time at the highest energies. More interestingly, this distant blazar, located at a redshift z=0.997 (approximately 10 billion light years away from us!), is the furthest blazar ever detected at such energies. This discovery is another proof of the great potential of the upcoming CTAO.
This discovery involved several researchers and members of the LST-1 Collaboration, with VHEGA members Daniel Morcuende and Jorge Otero Santos leading the analysis of the data taken with LST-1. In addition, the group has also monitored this blazar with optical photometric and polarimetric observations using the telescopes at the Sierra Nevada Observatory, providing broader coverage along the electromagnetic spectrum.
For more information, check the CTAO and IAA press releases.
Image credits: CTAO gGmbH, NASA, ESA, J. Olmsted (STScI).