Author

A. U. Abeysekara
A. Albert
R. Alfaro
C. Alvarez
J. D. Álvarez
J. R. Angeles Camacho
J. C. Arteaga-Velázquez
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. Carraminana
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. Du Vernois
R. W. Ellsworth
K. Engel
C. Espinoza
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 Greus
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. Weisgarber
F. Werner
E. Willox
J. Wood
G. B. Yodh
A. Zepeda
H. Zhou

Abstract

The High-Altitude Water Cherenkov (HAWC) Observatory is a wide-field-of-view gamma-ray observatory that is optimized to detect gamma rays between 300 GeV and several hundred TeV. The HAWC Collaboration recently released their third source catalog (3HWC), which contains 65 sources. One of these sources, the ultra-high-energy gamma-ray source 3HWC J1908+063, may exhibit a hardening of the spectral index at the highest energies (above 56 TeV). At least two populations of particles are needed to satisfactorily explain the highest energy emission. This second component could be leptonic or hadronic in origin. If it is hadronic in origin, it would imply the presence of protons with energies up to ∼1 PeV near the source. We have searched other 3HWC sources for the presence of this spectral hardening feature. If observed, this would imply that the sources could make good PeVatron candidates.

Department(s)

Physics

Publication Status

Open Access

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

Share

 
COinS