arxiv: 1310.0072 · v1 · submitted 2013-09-30 · 🌌 astro-ph.HE
Recognition: unknown
The HAWC Gamma-Ray Observatory: Observations of Cosmic Rays
HAWC collaboration: A. U. Abeysekara
,
R. Alfaro
,
C. Alvarez
,
J. D. \'Alvarez
,
R. Arceo
,
J. C. Arteaga-Vel\'azquez
,
H. A. Ayala Solares
,
A. S. Barber
show 93 more authors
B. M. Baughman
N. Bautista-Elivar
E. Belmont
S. Y. BenZvi
D. Berley
M. Bonilla Rosales
J. Braun
R. A. Caballero-Lopez
K. S. Caballero-Mora
A. Carrami\~nana
M. Castillo
U. Cotti
J. Cotzomi
E. De la Fuente
C. de Le\'on
T. DeYoung
R. Diaz Hernandez
J. C. D\'iaz-V\'elez
B. L. Dingus
M. A. DuVernois
R. W. Ellsworth
A. Fernandez
D. W. Fiorino
N. Fraija
A. Galindo
F. Garfias
L. X. Gonz\'alez
M. M. Gonz\'alez
J. A. Goodman
V. Grabski
M. Gussert
Z. Hampel-Arias
C. M. Hui
P. H\"untemeyer
A. Imran
A. Iriarte
P. Karn
D. Kieda
G. J. Kunde
A. Lara
R. J. Lauer
W. H. Lee
D. Lennarz
H. Le\'on Vargas
E. C. Linares
J. T. Linnemann
M. Longo
R. Luna-Garcia
A. Marinelli
H. Martinez
O. Martinez
J. Mart\'inez-Castro
J. A. J. Matthews
P. Miranda-Romagnoli
E. Moreno
M. Mostaf\'a
J. Nava
L. Nellen
M. Newbold
R. Noriega-Papaqui
T. Oceguera-Becerra
B. Patricelli
R. Pelayo
E. G. P\'erez-P\'erez
J. Pretz
C. Rivi\`ere
D. Rosa-Gonz\'alez
H. Salazar
F. Salesa
F. E. Sanchez
A. Sandoval
E. Santos
M. Schneider
S. Silich
G. Sinnis
A. J. Smith
K. Sparks
R. W. Springer
I. Taboada
P. A. Toale
K. Tollefson
I. Torres
T. N. Ukwatta
L. Villase\~nor
T. Weisgarber
S. Westerhoff
I. G. Wisher
J. Wood
G. B. Yodh
P. W. Younk
D. Zaborov
A. Zepeda
H. Zhou
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classification
🌌 astro-ph.HE
keywords
hawccosmicobservationraysgamma-raymeasurementsobservatoryangular
read the original abstract
We describe measurements of GeV and TeV cosmic rays with the High-Altitude Water Cherenkov Gamma-Ray Observatory, or HAWC. The measurements include the observation of the shadow of the moon; the observation of small-scale and large-scale angular clustering of the TeV cosmic rays; the prospects for measurement of transient solar events with HAWC; and the observation of Forbush decreases with the HAWC engineering array and HAWC-30.
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