Гамма
The Swift observatory has provided nearly daily observations of fleeting gamma ray burst events and has helped scientists investigate their origins and environments.
NASA's Fermi Gamma-ray Space Telescope recorded a sequence of gamma-ray bursts from the same region of the sky nearly simultaneously with the Wide Field X-ray Telescope detection.
The researchers used observations of the gamma-ray burst GRB 221009A to probe magnetic fields in the voids between galaxies.
The results were derived using gamma-ray data collected by NASA’s Fermi space telescope, specifically the Large Area Telescope (LAT).
The Cherenkov Telescope Array Observatory (CTAO) will be crucial for future studies of primordial intergalactic magnetic fields by observing TeV-band gamma-ray transients and associated electromagnetic cascades.
Two Three-Body satellites carry cosmic X-ray polarization detectors that work with an onboard AI model to classify gamma-ray bursts in real time with 99 percent accuracy.
CTAO is the largest and most powerful gamma-ray observatory in the world currently under construction.
The Xihe-2 payload includes a High-Energy Radiation Spectrometer to detect hard X-rays and gamma rays and determine non-thermal electron and ion acceleration sites during flares.
Intuitive Machines’ IM-3 mission targets Reiner Gamma and is part of the 2026 CLPS manifest.
The IM-3 mission will carry a diverse manifest of science and technology payloads to the Reiner Gamma region.
The Swift satellite was launched in 2004 and is dedicated to studying gamma-ray bursts and other high-energy cosmic phenomena.
The pulsar primarily emits gamma rays and high-energy particles that do not overwhelm Webb's infrared detectors.
Approximately half a dozen of the roughly 15,000 gamma ray bursts recorded since 1973 approach the duration of GRB 250702B.
The reaction rate of 26P(p,gamma)27S reaches up to five times the earlier estimated rate at 1 Gigakelvin.
These structures were detected simultaneously with high-energy gamma rays from the nova by NASA's Fermi Gamma-ray Space Telescope.
NASA's Fermi Large Area Telescope (LAT) first identified novae as gamma-ray sources.
The observation of the gamma-ray burst was confirmed by the Burst Alert Telescope of the Neil Gehrels Swift Observatory and other instruments.
New shocks formed in the outflow of V1405 Cassiopeiae when it expelled its envelope, which produced gamma rays observed by Fermi.
During its first 15 years of operations, Fermi-LAT detected gamma-ray emissions from more than 20 novae.
The event lasted for several days, making GRB 250702B the longest gamma-ray burst ever observed.