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The PHSF supported five Space Shuttle missions: Gamma Ray Observatory, Upper Atmospheric Research Satellite, Advanced Communications Technology Satellite, Hubble Space Telescope Servicing Mission 1, and Hubble Space Telescope Servicing Mission 2.
NASA’s Psyche mission carried an imager, magnetometers, and a gamma-ray and neutron spectrometer during the Mars flyby.
Intuitive Machines' Nova-C Trinity lander will study lunar swirls in the Reiner Gamma region.
Intuitive Machines’ planned IM-3 mission aims to achieve the first-ever soft landing in the Reiner Gamma region.
The Psyche spacecraft carries a magnetometer, a gamma-ray and neutron spectrometer, and a multispectral camera.
After landing at Shackleton, Chang’e 7’s orbiter will use its Wide-Band Infrared Spectrum Mineral Imaging Analyzer and Lunar Neutron Gamma Spectrometer to assist exploration planning and monitor the lander, rover, and hopper.
The COSI telescope will survey the soft gamma-ray sky to observe energy-specific processes in deep space.
Katalyst Space Technologies is developing a spacecraft to support NASA's Swift gamma-ray observatory.
NASA's Swift gamma-ray observatory is in low Earth orbit that is decaying.
The Space Development Agency’s Transport Layer Gamma variant added another roughly $424 million for 20 satellites.
Fermi detected GRB 230906A by capturing the distinctive signal of a gamma-ray burst.
NASA's Chandra X-ray Observatory, Fermi Gamma-ray Space Telescope, Neil Gehrels Swift Observatory, and Hubble Space Telescope were used to find GRB 230906A.
Collisions between new portions of matter in OP 313’s jet accelerate particles and convert light into gamma rays.
Multiple-telescope observations enabled the first clear reconstruction of the jet-collision gamma-ray production process for OP 313.
The team found that gamma-ray flares in OP 313 originate when newly ejected portions of matter from the region around the central black hole collide inside the collimated jet.
Swift studies gamma ray bursts and other energetic cosmic phenomena.
The research team designed a fast sourceless efficiency calibration algorithm that uses Geant4-based ray deposition modeling and Boolean operations to simulate how gamma rays deposit energy in the detector.
Swift normally slews rapidly to observe transient targets such as gamma ray bursts with its suite of telescopes.
The Burst Alert Telescope will continue detecting gamma ray bursts, but Swift will no longer slew to follow up these events with its other instruments.
The research team aims to enhance the adaptability of airborne gamma ray spectrometry for diverse survey conditions, including variable flight geometries and heterogeneous geological settings.