https://doi.org/10.1051/epjconf/201920803005
Information Technologies on High-Energy Astrophysics: Cosmic Ray Anisotropy using HAWC Observatory
1
Information Technologies Ph.D. Program, Centro Universitario de Ciencias Económico Administrativas (CUCEA), Universidad de Guadalajara, Periferico Norte 799, Módulo L305, Los Belenes, 45100, Zapopan, Jalisco, México
2
WIPAC & Department of Physics, University of Wisconsin–Madison, Madison, WI 53706, USA
3
Departamento. de Física, Centro Universitario de Ciencias Exactas e Ingenierías (CUCEI), Universidad de Guadalajara, Blvd. Marcelino García Barragán 1421, esq Calzada Olímpica, 44430, Guadalajara, Jalisco, México
4
Departamento de Ciencias Naturales y Exactas, Centro Universitario de los Valles (CUValles), Universidad de Guadalajara, Carretera Guadalajara–Ameca Km. 45.5, C.P. 46600. Ameca, Jalisco, México
* e-mail: edfuente@gmail.com
** e-mail: juan.diazvelez@alumnos.udg.mx
*** e-mail: paolo.desiati@icecube.wisc.edu
**** e-mail: jlgalu2013@gmail.com
† e-mail: cjanet.torrealba@gmail.com
‡ e-mail: chesirepoincar@gmail.com
Published online: 10 May 2019
The detection of astroparticles, specially at high energies (>100 GeV), requires special techniques and instruments (telescopes or observatories), for example, those that use the Water Cherenkov radiation technique. In this paper we show an example of how Information Technologies can be used to perform maps and produce high impact results. The latter case is illustrated in the summary of the generation of a high statistics map of cosmic rays at 10 TeV in the northern sky with data collected by the High Altitude Water Cherenkov (HAWC) observatory.
© The Authors, published by EDP Sciences, 2019
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
