{ "id": "1509.07851", "version": "v1", "published": "2015-09-25T19:39:27.000Z", "updated": "2015-09-25T19:39:27.000Z", "title": "Highlights from the High Altitude Water Cherenkov Observatory", "authors": [ "John Pretz", "for the HAWC Collaboration" ], "comment": "Presented at the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. See arXiv:1508.03327 for all HAWC contributions", "categories": [ "astro-ph.HE" ], "abstract": "The High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory was completed this year at a 4100-meter site on the flank of the Sierra Negra volcano in Mexico. HAWC is a water Cherenkov ground array with the capability to distinguish 100 GeV - 100 TeV gamma rays from the hadronic cosmic-ray background. HAWC is uniquely suited to study extremely high energy cosmic-ray sources, search for regions of extended gamma-ray emission, and to identify transient gamma-ray phenomena. HAWC will play a key role in triggering multi-wavelength and multi-messenger studies of active galaxies, gamma-ray bursts, supernova remnants and pulsar wind nebulae. Observation of TeV photons also provide unique tests for a number of fundamental physics phenomena including dark matter annihilation and primordial black hole evaporation. Operation began mid-2013 with the partially-completed detector. Multi-TeV emission from the Galactic Plane is clearly seen in the first year of operation, confirming a number of known TeV sources, and a number of AGN have been observed. We discuss the science of HAWC, summarize the status of the experiment, and highlight first results from analysis of the data.", "revisions": [ { "version": "v1", "updated": "2015-09-25T19:39:27.000Z" } ], "analyses": { "keywords": [ "high altitude water cherenkov observatory", "high energy cosmic-ray sources", "extremely high energy cosmic-ray" ], "tags": [ "conference paper" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1394847 } } }