The High-Altitude Water Cherenkov Gamma-Ray Observatory. HAWC is a facility designed to observe gamma rays and cosmic rays between 100 GeV and 100 TeV. HAWC is located on the flanks of the Sierra .

Engineering, IT and Library. HEA Lab and Facility Telephone Numbers. CfA Soc and Rec Club.

Desde el origen de los rayos cósmicos, pasando por los mecanismos de aceleración de las partículas en el entorno de los agujeros negros, hasta la búsqueda del origen de la materia y estudio de la física mas halla del modelo estandar. Descarga de documentos relacionados .

Past Events - Photos and More. Atomic, Molecular, Optical Seminars. Nicholas Giordano named 2018 College of Science Distinguished Alumnus. New research from the Iyer-Biswas group connects noisy single-cell dynamics to smooth population growth. Prof Erica Carlson named 150th Anniversary Professor.

HAWC is complementary to satellite experiments like the Fermi Gamma-Ray Space Telescope, which covers the energy range between MeV and GeV, and the ground-based imaging atmospheric Cherenkov telescopes such as VERITAS, H. and MAGIC, which have excellent sensitivity to gamma-ray sources at TeV energies but have only about 1 degree field of view. HAWC scientists at the University of Wisconsi.

Astroparticle Physics in the Very-High Energy Gamma-Ray Band. We are an experimental astroparticle physics research group at the Georgia Institute of Technology. We analyze data taken with VERITAS. And participate in the development and construction of a novel telescope type for the next generation VHE instrument CTA.