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A GeV to TeV view of shell-type SNRsShock acceleration by the shells of supernova remnants (SNRs) has been hypothesized to be the mechanism that produces the bulk of Galactic Cosmic Rays, possibly up to PeV energies. SomeSNRs have been shown to accelerate cosmic rays to TeV energies and above. But which SNRs are indeed efficient accelerators of protons and nuclei? And what is the maximum energy up to which they can efficiently accelerate particles? Measurements of non-thermal emission, especially in the gamma-ray regime, are essential to answer these questions.
Document ID
20210018580
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
A. U. Abeysekara (University of Utah Salt Lake City, Utah, United States)
A. Albert (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
R. Alfaro (Universidad Nacional Autónoma de México )
C. Alvarez (Universidad Autónoma de Chiapas )
J.R. Angeles Camacho (Universidad Nacional Autónoma de México )
J.C. Arteaga-Velázquez (Universidad Michoacana de San Nicolás de Hidalgo Morelia, Mexico)
K. P. Arunbabu (Universidad Nacional Autónoma de México )
D. Avila Rojas (Universidad Nacional Autónoma de México )
H. A. Ayala Solares (Pennsylvania State University State College, Pennsylvania, United States)
R. Babu (Michigan Technological University Houghton, Michigan, United States)
V. Baghmanyan (Polish Academy of Sciences Warsaw, Poland)
A. S. Barber (University of Utah Salt Lake City, Utah, United States)
Josefa Becerra Gonzalez ORCID(OTHER EMPLOYER / AFFILIATE Santa Cruz de Tenerife, Spain)
E. Belmont-Moreno (Universidad Nacional Autónoma de México)
S. Y. BenZvi (University of Rochester Rochester, New York, United States)
D. Berley (University of Maryland, College Park College Park, Maryland, United States)
C. Brisbois (University of Maryland, College Park College Park, Maryland, United States)
K. S. Caballero-Mora (Universidad Autónoma de Chiapas)
T. Capistrán ( Universidad Nacional Autónoma de México)
A. Carramiñana (Instituto Nacional de Astrofísica )
S. Casanova (Polish Academy of Sciences Warsaw, Poland)
O. Chaparro-Amaro (Instituto Politécnico Nacional Mexico City, Mexico)
U. Cotti (Universidad Michoacana de San Nicolás de Hidalgo Morelia, Mexico)
J. Cotzomi (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
S. Coutiño de León (Instituto Nacional de Astrofísica)
E. De la Fuente (Universidad de Guadalajara)
C. de León (Universidad Michoacana de San Nicolás de Hidalgo Morelia, Mexico)
L. Diaz-Cruz (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
R. Diaz Hernandez (Instituto Nacional de Astrofísica)
J. C. Díaz-Vélez ( Universidad de Guadalajara)
B. L. Dingus (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
M. Durocher (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
M. A. DuVernois (University of Wisconsin–Madison Madison, Wisconsin, United States)
R. W. Ellsworth (University of Maryland, College Park College Park, Maryland, United States)
K. Engel (University of Maryland, College Park College Park, Maryland, United States)
C. Espinoza (Universidad Nacional Autónoma de México )
K. L. Fan (University of Maryland, College Park College Park, Maryland, United States)
K. Fang (University of Wisconsin–Madison Madison, Wisconsin, United States)
M. Fernández Alonso (Pennsylvania State University State College, Pennsylvania, United States)
B. Fick (Michigan Technological University Houghton, Michigan, United States)
H. Fleischhack (Catholic University of America Washington D.C., District of Columbia, United States)
J. L. Flores ( Universidad de Guadalajara)
N. I. Fraija (Universidad Nacional Autónoma de México )
D. Garcia ( Universidad Nacional Autónoma de México)
J. A. García-González (Tecnologico de Monterrey )
J. L. García-Luna (Universidad de Guadalajara)
G. García-Torales (Universidad de Guadalajara)
F. Garfias (Universidad Nacional Autónoma de México )
G. Giacinti (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
Joshua R Wood (Universities Space Research Association Columbia, Maryland, United States)
M.M. González (Universidad Nacional Autónoma de México )
J. A. Goodman (University of Maryland, College Park College Park, Maryland, United States)
J.P. Harding (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
S. Hernandez (Universidad Nacional Autónoma de México)
I. Herzog (Michigan Technological University Houghton, Michigan, United States)
J. Hinton (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
B. Hona (University of Utah Salt Lake City, Utah, United States)
D. Huang (Michigan Technological University Houghton, Michigan, United States)
F. Hueyotl-Zahuantitla (Universidad Autónoma de Chiapas)
C Michelle Hui (OTHER EMPLOYER / AFFILIATE)
B. Humensky (University of Maryland, College Park College Park, Maryland, United States)
P. Hüntemeyer (Michigan Technological University Houghton, Michigan, United States)
A. Iriarte (Universidad Nacional Autónoma de México)
A. Jardin-Blicq (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
H. Jhee (University of Seoul Seoul, South Korea)
V. Joshi ( Friedrich Alexander Universität )
D. Kieda (University of Utah Salt Lake City, Utah, United States)
G J. Kunde (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
S. Kunwar (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
A. Lara ( Universidad Nacional Autónoma de México)
J. Lee (University of Seoul Seoul, South Korea)
W. H. Lee (Universidad Nacional Autónoma de México)
D. Lennarz (Georgia Institute of Technology Atlanta, Georgia, United States)
H. León Vargas (Universidad Nacional Autónoma de México)
J. Linnemann (Michigan State University East Lansing, Michigan, United States)
A. L. Longinotti (Universidad Nacional Autónoma de México)
R. López-Coto (INFN Sezione di Padova Padova, Italy)
G. Luis-Raya (Universidad Politécnica de Pachuca Villa Zempoala, Mexico)
J. Lundeen (Michigan State University East Lansing, Michigan, United States)
K. Malone (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
V. Marandon (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
O. Martinez (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
I. Martinez-Castellanos (University of Maryland, College Park College Park, Maryland, United States)
H. Martínez-Huerta (Universidad de Monterrey)
J. A. J. Matthews (University of New Mexico Albuquerque, New Mexico, United States)
Julie E Mc Enery (Goddard Space Flight Center Greenbelt, Maryland, United States)
P. Miranda-Romagnoli (Universidad Autónoma del Estado de Hidalgo Pachuca, Mexico)
J.A. Morales-Soto (Universidad Michoacana de San Nicolás de Hidalgo Morelia, Mexico)
E. Moreno (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
M. Mostafá (Pennsylvania State University State College, Pennsylvania, United States)
A. Nayerhoda (Polish Academy of Sciences Warsaw, Poland)
L. Nellen (Universidad Nacional Autónoma de México)
M. Newbold (University of Utah Salt Lake City, Utah, United States)
M. U. Nisa (Max-Planck Institute for Nuclear Physics)
R. Noriega-Papaqui (Universidad Autónoma del Estado de Hidalgo)
L. Olivera-Nieto (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
N. Omodei (Stanford University Stanford, California, United States)
A. Peisker (Michigan State University East Lansing, Michigan, United States)
Y. Pérez Araujo (Universidad Nacional Autónoma de México)
E.G. Pérez-Pérez (Universidad Politécnica de Pachuca Villa Zempoala, Mexico)
C. D. Rho (University of Seoul Seoul, South Korea)
C. Rivière (University of Maryland, College Park College Park, Maryland, United States)
D. Rosa-Gonzalez (Instituto Nacional de Astrofísica)
E. Ruiz-Velasco (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
J. Ryan (University of New Hampshire Durham, New Hampshire, United States)
H. Salazar (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
F. Salesa Greus (Polish Academy of Sciences Warsaw, Poland)
A. Sandoval ( Universidad Nacional Autónoma de México )
M. Schneider (University of Maryland, College Park College Park, Maryland, United States)
H. Schoorlemmer (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
J. Serna-Franco ( Universidad Nacional Autónoma de México)
G. Sinnis (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
A. J. Smith (University of Maryland, College Park College Park, Maryland, United States)
R. W. Springer (University of Utah Salt Lake City, Utah, United States)
P. Surajbali (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
I. Taboada (Georgia Institute of Technology Atlanta, Georgia, United States)
M. Tanner (Pennsylvania State University State College, Pennsylvania, United States)
K. Tollefson (Michigan State University East Lansing, Michigan, United States)
I. Torres (Instituto Nacional de Astrofísica)
R. Torres-Escobedo (Tsung-Dao Lee Institute and School of Physics and Astronomy )
R. Turner (Michigan Technological University Houghton, Michigan, United States)
F. Ureña-Mena (8Instituto Nacional de Astrofísica)
L. Villaseñor (Benemérita Universidad Autónoma de Puebla Puebla City, Mexico)
X. Wang (Michigan Technological University Houghton, Michigan, United States)
I. J. Watson (University of Seoul Seoul, South Korea)
T. Weisgarber (University of Wisconsin–Madison Madison, Wisconsin, United States)
F. Werne (Max Planck Institute for Nuclear Physics Heidelberg, Germany)
E. Willox (University of Maryland, College Park College Park, Maryland, United States)
Joshua R Wood (Universities Space Research Association Columbia, Maryland, United States)
G. B. Yodh (University of California, Irvine Irvine, California, United States)
A. Zepeda (Centro de Investigación y de Estudios Avanzados del IPN)
H. Zhou (Tsung-Dao Lee Institute and School of Physics and Astronomy)
Date Acquired
July 12, 2021
Subject Category
Astronomy
Meeting Information
Meeting: 37th International Cosmic Ray Conference 2021
Location: online
Country: DE
Start Date: July 12, 2021
End Date: July 23, 2021
Sponsors: Karlsruhe Institute of Technology
Funding Number(s)
CONTRACT_GRANT: 80GSFC21M0002
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee

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