WebAug 25, 2003 · The Spitzer Space Telescope is the final mission in NASA's Great Observatories Program - a family of four space-based observatories, each observing the universe in a different kind of light. Spitzer is designed to detect infrared radiation, which is primarily heat radiation. WebHAWC is located on the flanks of the Sierra Negra volcano near Puebla, Mexico at an altitude of 4100 meters (13,500 feet). The detector has an instantaneous field of view … HAWC has made its first externally-announced transient trigger, a gamma … A map of the galactic and extragalactic γ-rays observed by the Fermi Gamma-ray … HAWC: A Next-Generation All-Sky Gamma-ray Telescope S. Westerhoff … The HAWC Collaboration . HAWC is an international collaboration between … HAWC is supported by grants from the following agencies: US National Science … Our current picture of cosmic rays below the "knee" — acceleration of particles in … In HAWC, we can discriminate air showers from gamma-rays and cosmic rays by …
GCN - Missions - HAWC - NASA
WebHAWC is a very sensitive detector for TeV cosmic rays. While the high rate of cosmic rays detected in HAWC forms an undesirable background in the search for gamma-ray sources, it also enables us to use HAWC for … WebHAWC may refer to: High Altitude Water Cherenkov Experiment, a gamma-ray observatory in Mexico; HAWC, a far-infrared telescope aboard NASA's SOFIA project; Wacca … spot cases
On the sensitivity of the HAWC observatory to gamma-ray bursts
WebAbstract An incremental version of the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi Large Area Telescope is presented. This version (4LAC-DR3) derives from the third data release of the 4FGL catalog based on 12 yr of E > 50 MeV gamma-ray data, where the spectral parameters, spectral energy distributions (SEDs), … WebOn the sensitivity of the HAWC observatory to gamma-ray bursts WebRecent TeV observations of nearby pulsars with the HAWC telescope have been interpreted as evidence that the diffusion of high-energy electrons and positrons within pulsar wind nebulae is highly inefficient compared to the rest of the interstellar medium. If the diffusion coefficient well outside the nebula is close to the value inferred for ... spotcatchers gmbh