Author

J. A. Morales-Soto
J. A. Morales-Soto
J. C. Arteaga-Velázquez
J. C. Arteaga-Velázquez
A. U. Abeysekara
A. Albert
R. Alfaro
C. Alvarez
J. D. Álvarez
J. R. Angeles Camacho
K. P. Arunbabu
D. Avila Rojas
H. A. Ayala Solares
R. Babu
V. Baghmanyan
A. S. Barber
J. Becerra Gonzalez
E. Belmont-Moreno
S. Y. BenZvi
D. Berley
C. Brisbois
K. S. Caballero-Mora
T. Capistran
A. Caraminana
S. Casanova
O. Chaparro-Amaro
U. Cotti
J. Cotzomi
S. Coutino de Leon
E. De la Fuente
C. de Leon
L. Diaz-Cruz
R. Diaz Hernandez
J. C. Diaz-Velez
B. L. Dingus
M. Durocher
M. A. DuVernois
R. W. Ellsworth
K. Engel
C. Ezpinoza
K. L. Fan
K. Fang
M. Fernandez Alonso
B. Fick
H. Fleischhack
J. L. Flores
N. I. Fraija
D. Garcia
J. A. Garcia-Gonzalez
J. L. Garcia-Luna
G. Garcia-Torales
F. Garfias
G. Giacinti
H. Goksu
M. M. Gonzalez
J. A. Goodman
J. P. Harding
S. Hernandez
I. Herzog
J. Hinton
B. Hona
D. Huang
F. Hueyotl-Zahuantitla
C. M. Hui
B. Humensky
P. Huntemeyer
A. Iriarte
A. Jardin-Blicq
H. Jhee
V. Joshi
D. Kieda
G. J. Kunde
S. Kunwar
A. Lara
J. Lee
W. H. Lee
D. Lennarz
H. Leon Vargas
J. Linnemann
A. L. Longinotti
R. Lopez-Coto
G. Luis-Raya
J. Lundeen
K. Malone
V. Marandon
O. Martinez
I. Martinez-Castellanos
H. Martinez-Huerta
J. Martinez-Castro
J. A. J. Matthews
J. McEnery
P. Miranda-Romagnoli
J. A. Morales-Soto
E. Moreno
M. Mostafa
A. Nayerhoda
L. Nellen
M. Newbold
M. U. Nisa
R. Noriega-Papaqui
L. Olivera-Nieto
N. Omodei
A. Peisker
Y. Perez Araujo
E. G. Perez-Perez
C. D. Rho
C. Riviere
D. Rosa-Gonzalez
E. Ruiz-Velasco
J. Ryan
H. Salazar
F. Salesa Grues
A. Sandoval
M. Schneider
H. Schoorlemmer
J. Serna-Franco
G. Sinnis
A. J. Smith
R. W. Springer
P. Surajbali
I. Taboada
M. Tanner
K. Tollefson
I. Torres
R. Torres-Escobedo
R. Turner
F. Urena-Mena
L. Villasenor
Xiaojie Wang, Missouri University of Science and TechnologyFollow
I. J. Watson
T. Weisgerber
F. Werner
E. Willox
J. Wood
G. B. Yodh
A. Zepeda
H. Zhou

Abstract

Thanks to recent technological development, a new generation of cosmic ray experiments have been developed with more sensitivity to study these particles in the primary energy interval from 10 TeV to 1 PeV, such as HAWC. Due to its design and high altitude, the HAWC gamma-ray and cosmic ray observatory can provide a bridge between the data from direct and indirect cosmic ray detectors. In 2017 the HAWC collaboration published its first result on the total energy spectrum of cosmic rays, which covers the range from 10 to 500 TeV. This work updates the previous result by extending the energy interval of the measured all-particle cosmic-ray energy spectrum up to 1 PeV. The energy spectrum was obtained from the analysis of two years of HAWC's data using an unfolding method. We employed the QGSJET-II-04 model for the energy calibration and the spectrum reconstruction. The results confirm the presence of a knee like feature at tens of TeV, as previously reported by the HAWC collaboration in 2017.

Department(s)

Physics

Comments

National Science Foundation, Grant PRODEP-SEP UDG-CA-499

International Standard Serial Number (ISSN)

1824-8039

Document Type

Article - Conference proceedings

Document Version

Citation

File Type

text

Language(s)

English

Rights

© 2025 Sissa Medialab Srl, All rights reserved.

Publication Date

18 Mar 2022

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