MAGIC and Fermi-LAT Gamma-ray Results on Unassociated HAWC Sources

M L. Ahnen, ETH Zurich
S Ansoldi, Università di Udine, and INFN Trieste, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University
L A. Antonelli, National Institute for Astrophysics (INAF)
C Arcaro, Università di Padova and INFN
D Baack, Technische Universität Dortmund
A Babić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb, University of Osijek
B Banerjee, Saha Institute of Nuclear Physics, HBNI
P Bangale, Max-Planck-Institut für Physik
U Barres de Almeida, Max-Planck-Institut für Physik, Centro Brasileiro de Pesquisas Físicas (CBPF)
J A. Barrio, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
J Becerra González, Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica
W Bednarek, University of Łódź
E Bernardini, Università di Padova and INFN, Deutsches Elektronen-Synchrotron (DESY), Humboldt University of Berlin, Institut für Physik
R Ch Berse, Technische Universität Dortmund
A Berti, Università di Udine, and INFN Trieste, Università di Trieste
W Bhattacharyya, Deutsches Elektronen-Synchrotron (DESY)
A Biland, ETH Zurich
O Blanch, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
G Bonnoli, Università di Siena and INFN Pisa
R Carosi, Università di Siena and INFN Pisa
A Carosi, National Institute for Astrophysics (INAF)
G Ceribella, Max-Planck-Institut für Physik
A Chatterjee, Saha Institute of Nuclear Physics, HBNI
S M. Colak, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
P Colin, Max-Planck-Institut für Physik
E Colombo, Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica
J L. Contreras, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
J Cortina, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
S Covino, National Institute for Astrophysics (INAF)
P Cumani, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
P Da Vela, Università di Siena and INFN Pisa
F Dazzi, National Institute for Astrophysics (INAF)
A De Angelis, Università di Padova and INFN
B De Lotto, Università di Udine, and INFN Trieste
M Delfino, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
J Delgado, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
F Di Pierro, Università di Padova and INFN
A Domínguez, Grupo de Altas Energías, Universidad Complutense de Madrid
D Dominis Prester, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
D Dorner, Universität Würzburg
M Doro, Università di Padova and INFN
S Einecke, Technische Universität Dortmund
D Elsaesser, Technische Universität Dortmund
V Fallah Ramazani, Finnish MAGIC Consortium: Tuorla Observatory and Finnish Centre of Astronomy with ESO (FINCA), University of Turku
A Fernández-Barral, Università di Padova and INFN, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
D Fidalgo, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
M V. Fonseca, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
L Font, CERES-IEEC, Universitat Autónoma de Barcelona
C Fruck, Max-Planck-Institut für Physik
D Galindo, Universitat de Barcelona
R J. García López, Inst. de Astrofísica de Canarias, Universidad de La Laguna, Dpto. Astrofísica
M Garczarczyk, Deutsches Elektronen-Synchrotron (DESY)
M Gaug, CERES-IEEC, Universitat Autónoma de Barcelona
P Giammaria, National Institute for Astrophysics (INAF)
N Godinović, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
D Gora, Deutsches Elektronen-Synchrotron (DESY)
D Guberman, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
D Hadasch, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Department of Physics, Kyoto University, Tokai University
A Hahn, Max-Planck-Institut für Physik
T Hassan, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
M Hayashida, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
J Herrera, Inst. de Astrofísica de Canarias, Universidad de La Laguna
J Hose, Max-Planck-Institut für Physik
D Hrupec, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
K Ishio, Max-Planck-Institut für Physik
Y Konno, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
H Kubo, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Department of Physics, Kyoto University, Tokai University
J Kushida, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
D Kuveždić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
D Lelas, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
E Lindfors, Finnish MAGIC Consortium: Tuorla Observatory and Finnish Centre of Astronomy with ESO (FINCA), University of Turku, Astronomy Division, University of Oulu
S Lombardi, National Institute for Astrophysics (INAF)
F Longo, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Università di Trieste
M López, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
C Maggio, CERES-IEEC, Universitat Autónoma de Barcelona
P Majumdar, Saha Institute of Nuclear Physics, HBNI
M Makariev, Inst. for Nucl. Research and Nucl. Energy, Bulgarian Academy of Sciences
G Maneva, Inst. for Nucl. Research and Nucl. Energy, Bulgarian Academy of Sciences
M Manganaro, Inst. de Astrofísica de Canarias, Universidad de La Laguna
K Mannheim, Universität Würzburg
L Maraschi, National Institute for Astrophysics (INAF)
M Mariotti, Università di Padova and INFN
M Martínez, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
S Masuda, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
D Mazin, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
K Mielke, Technische Universität Dortmund
M Minev, Inst. for Nucl. Research and Nucl. Energy, Bulgarian Academy of Sciences
J M. Miranda, Università di Siena and INFN Pisa
R Mirzoyan, Max-Planck-Institut für Physik
A Moralejo, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
V Moreno, CERES-IEEC, Universitat Autónoma de Barcelona
E Moretti, Max-Planck-Institut für Physik
T Nagayoshi, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
V Neustroev, Finnish MAGIC Consortium: Tuorla Observatory and Finnish Centre of Astronomy with ESO (FINCA), University of Turku, University of Oulu
A Niedzwiecki, University of Łódź
M Nievas Rosillo, Unidad de Partículas y Cosmología (UPARCOS), Universidad Complutense
C Nigro, Deutsches Elektronen-Synchrotron (DESY)
K Nilsson, Finnish MAGIC Consortium: Tuorla Observatory and Finnish Centre of Astronomy with ESO (FINCA), University of Turku, University of Oulu
D Ninci, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
K Nishijima, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
K Noda, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
L Nogués, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
S Paiano, Università di Padova and INFN
J Palacio, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
D Paneque, Max-Planck-Institut für Physik
R Paoletti, Università di Siena and INFN Pisa
J M. Paredes, Universitat de Barcelona, ICC, IEEC-UB
G Pedaletti, Deutsches Elektronen-Synchrotron (DESY)
M Peresano, Università di Udine, and INFN Trieste
M Persic, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Osservatorio Astronomico di Trieste, Istituto Nazionale di Astrofisica
P G. Prada Moroni, Università di Pisa, and INFN Pisa
E Prandini, Università di Padova and INFN
I Puljak, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
J R Garcia, Max-Planck-Institut für Physik
I Reichardt, Università di Padova and INFN
W Rhode, Technische Universität Dortmund
M Ribó, Universitat de Barcelona, ICC, IEEC-UB
J Rico, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
C Righi, National Institute for Astrophysics (INAF)
A Rugliancich, Università di Siena and INFN Pisa
T Saito, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
K Satalecka, Deutsches Elektronen-Synchrotron (DESY)
T Schweizer, Max-Planck-Institut für Physik
J Sitarek, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
I Šnidarić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
D Sobczynska, University of Łódź
A Stamerra, National Institute for Astrophysics (INAF)
M Strzys, Max-Planck-Institut für Physik
T Surić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
M Takahashi, Max-Planck-Institut für Physik
L Takalo, Finnish MAGIC Consortium: Tuorla Observatory and Finnish Centre of Astronomy with ESO (FINCA), University of Turku, University of Oulu
F Tavecchio, National Institute for Astrophysics (INAF)
P Temnikov, Inst. for Nucl. Research and Nucl. Energy, Bulgarian Academy of Sciences
T Terzić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
M Teshima, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
N Torres-Albà, Universitat de Barcelona, ICC, IEEC-UB
A Treves, Università di Udine, and INFN Trieste
S Tsujimoto, Japanese MAGIC Consortium: ICRR, The University of Tokyo, Kyoto University, Tokai University
G Vanzo, Inst. de Astrofísica de Canarias, Universidad de La Laguna
M Vazquez Acosta, Inst. de Astrofísica de Canarias, Universidad de La Laguna
I Vovk, Max-Planck-Institut für Physik
J E. Ward, Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST)
M Will, Max-Planck-Institut für Physik
D Zarić, Croatian MAGIC Consortium: University of Rijeka, University of Split, University of Zagreb
A Albert, Physics Division, Los Alamos National Laboratory, Los Alamos
R Alfaro, Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de México
C Alvarez, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
R Arceo, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
J C. Arteaga-Velázquez, Universidad Michoacana de San Nicolás de Hidalgo
D Avila Rojas, Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de México
H A. Ayala Solares, Pennsylvania State University
A Becerril, Instituto de Física, Universidad Nacional Autónoma de México
E Belmont-Moreno, Instituto de Física, Universidad Nacional Autónoma de México
S Y. BenZvi, University of Rochester
A Bernal, Instituto de Astronomía, Universidad Nacional Autónoma de México
J Braun, University of Wisconsin-Madison
K S. Caballero-Mora, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
T Capistrán, Instituto Nacional de Astrofísica, Óptica y Electrónica
A Carramiñana, Instituto Nacional de Astrofísica, Óptica y Electrónica
S Casanova, Institute of Nuclear Physics Polish Academy of Sciences
M Castillo, Universidad Michoacana de San Nicolás de Hidalgo
U Cotti, Universidad Michoacana de San Nicolás de Hidalgo
J Cotzomi, Benemérita Universidad Autónoma de Puebla
S Coutiño de León, Instituto Nacional de Astrofísica, Óptica y Electrónica
C De León, Benemérita Universidad Autónoma de Puebla
E De la Fuente, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara
R Diaz Hernandez, Instituto Nacional de Astrofísica, Óptica y Electrónica
S Dichiara, Instituto de Astronomía, Universidad Nacional Autónoma de México
B L. Dingus, Los Alamos National Laboratory
M A. DuVernois, University of Wisconsin-Madison
J C. Díaz-Vélez, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara
R W. Ellsworth, George Mason University
K Engel, University of Maryland
O Enriquez-Rivera, Instituto de Geofísica, Universidad Nacional Autónoma de México
D W. Fiorino, University of Maryland
H Fleischhack, Michigan Technological University
N Fraija, Instituto de Astronomía, Universidad Nacional Autónoma de México
J A. García-González, Instituto de Física, Universidad Nacional Autónoma de México
F Garfias, Instituto de Astronomía, Universidad Nacional Autónoma de México
A González-Muñoz, Instituto de Física, Universidad Nacional Autónoma de México
M M. González, Instituto de Astronomía, Universidad Nacional Autónoma de México
J A. Goodman, University of Maryland
Z Hampel-Arias, University of Wisconsin-Madison
J P. Harding, Los Alamos National Laboratory
S Hernandez, Instituto de Física, Universidad Nacional Autónoma de México
F Hueyotl-Zahuantitla, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
C M. Hui, NASA Marshall Space Flight Center, Astrophysics Office
P Hüntemeyer, Michigan Technological University
A Iriarte, Instituto de Astronomía, Universidad Nacional Autónoma de México
A Jardin-Blicq, Max-Planck Institute for Nuclear Physics
V Joshi, Max-Planck Institute for Nuclear Physics
S Kaufmann, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
A Lara, Instituto de Geofísica, Universidad Nacional Autónoma de México
R J. Lauer, University of New Mexico
W H. Lee, Instituto de Astronomía, Universidad Nacional Autónoma de México
D Lennarz, Georgia Institute of Technology
H León Vargas, Instituto de Física, Universidad Nacional Autónoma de México
J T. Linnemann, Michigan State University
A L. Longinotti, Instituto Nacional de Astrofísica, Óptica y Electrónica
G Luis-Raya, Universidad Politecnica de Pachuca
R Luna-García, Centro de Investigación en Computación, Instituto Politécnico Nacional
R López-Coto, Max-Planck Institute for Nuclear Physics
K Malone, Pennsylvania State University
S S. Marinelli, Michigan State University
O Martinez, Benemérita Universidad Autónoma de Puebla
I Martinez-Castellanos, University of Maryland
J Martínez-Castro, Centro de Investigación en Computación, Instituto Politécnico Nacional
H Martínez-Huerta, Centro de Investigación y de Estudios Avanzados del IPN
J A. Matthews, University of New Mexico
P Miranda-Romagnoli, Universidad Autónoma del Estado de Hidalgo
E Moreno, Benemérita Universidad Autónoma de Puebla
M Mostafá
A Nayerhoda, Institute of Nuclear Physics Polish Academy of Sciences
L Nellen, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México
M Newbold, University of Utah
M U. Nisa, University of Rochester
R Noriega-Papaqui, Universidad Autónoma del Estado de Hidalgo
R Pelayo, Centro de Investigación en Computación, Instituto Politécnico Nacional
J Pretz, Pennsylvania State University
E G. Pérez-Pérez, Universidad Politecnica de Pachuca
Z Ren, University of New Mexico
C D. Rho, University of Rochester
C Rivière, University of Maryland
D Rosa-González, Instituto Nacional de Astrofísica, Óptica y Electrónica
M Rosenberg, Pennsylvania State University
E Ruiz-Velasco, Max-Planck Institute for Nuclear Physics
F Salesa Greus, Institute of Nuclear Physics Polish Academy of Sciences
A Sandoval, Instituto de Física, Universidad Nacional Autónoma de México
M Schneider, Santa Cruz Institute for Particle Physics, University of California
M Seglar Arroyo, Pennsylvania State University
G Sinnis, Los Alamos National Laboratory
A J. Smith, University of Maryland
R W. Springer, University of Utah
P Surajbali, Max-Planck Institute for Nuclear Physics
I Taboada, Georgia Institute of Technology
O Tibolla, Universidad Autónoma de Chiapas, Tuxtla Gutiérrez
K Tollefson, Michigan State University
I Torres, Instituto Nacional de Astrofísica, Óptica y Electrónica
T N. Ukwatta, Los Alamos National Laboratory
G Vianello, Stanford University
L Villaseñor, Benemérita Universidad Autónoma de Puebla
F Werner, Max-Planck Institute for Nuclear Physics
S Westerhoff, University of Wisconsin-Madison
J Wood, University of Wisconsin-Madison
T Yapici, University of Rochester
G Yodh, University of California – Irvine
A Zepeda, Centro de Investigación y de Estudios Avanzados del IPN
H Zhou, Los Alamos National Laboratory
J D. Álvarez, Universidad Michoacana de San Nicolás de Hidalgo
M Ajello, Clemson University, Kinard Lab of Physics
L Baldini, Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
G Barbiellini, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Università di Trieste
B Berenji, California State University
E Bissaldi, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
R D. Blandford, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
R Bonino, Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Università degli Studi di Torino
E Bottacini, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University, University of Padova
T J. Brandt, NASA Goddard Space Flight Center
J Bregeon, Laboratoire Univers et Particules de Montpellier, Université Montpellier
P Bruel, Laboratoire Leprince-Ringuet, École polytechnique
R A. Cameron, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
R Caputo, Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center
P A. Caraveo, INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano
D Castro, NASA Goddard Space Flight Center, Harvard-Smithsonian Center for Astrophysics
E Cavazzuti, Italian Space Agency, Via del Politecnico snc
G Chiaro, INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano
S Ciprini, Italian Space Agency, Via del Politecnico snc, Space Science Data Center – Agenzia Spaziale Italiana
D Costantin, Università di Padova
F D’Ammando, INAF Istituto di Radioastronomia, Università di Bologna
F de Palma, Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Università Telematica Pegaso, Piazza Trieste e Trento
A Desai, Clemson University, Kinard Lab of Physics
N Di Lalla, Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
M Di Mauro, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
L Di Venere, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
C Favuzzi, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
Y Fukazawa, Hiroshima University
S Funk, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics
P Fusco, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
F Gargano, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
D Gasparrini, Space Science Data Center – Agenzia Spaziale Italiana, Via del Politecnico, snc, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
N Giglietto, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
F Giordano, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
M Giroletti, INAF Istituto di Radioastronomia
T Glanzman, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, National Accelerator Laboratory, Stanford University
D Green, NASA Goddard Space Flight Center, University of Maryland
I A. Grenier, Laboratoire AIM, CEA-IRFU/CNRS/Université Paris Diderot, Service d’Astrophysique
S Guiriec, The George Washington University, NASA Goddard Space Flight Center
A K. Harding, NASA Goddard Space Flight Center
E Hays, NASA Goddard Space Flight Center
J W. Hewitt, University of North Florida
D Horan, Laboratoire Leprince-Ringuet, École polytechnique
G Jóhannesson, Science Institute, University of Iceland, Royal Institute of Technology and Stockholm University
M Kuss, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
S Larsson, KTH Royal Institute of Technology, The Oskar Klein Centre for Cosmoparticle Physics
I Liodakis, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
F Loparco, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
P Lubrano, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
J D. Magill, University of Maryland
S Maldera, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
A Manfreda, Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
M N. Mazziotta, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
I Mereu, Università degli Studi di Perugia
P F. Michelson, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
T Mizuno, Hiroshima Astrophysical Science Center, Hiroshima University
M E. Monzani, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
A Morselli, Istituto Nazionale di Fisica Nucleare, Sezione di Roma ‘Tor Vergata’
I V. Moskalenko, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
M Negro, Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Università degli Studi di Torino
E Nuss, Laboratoire Univers et Particules de Montpellier, Université Montpellier
N Omodei, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
M Orienti, INAF Istituto di Radioastronomia
E Orlando, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
J. F. Ormes, University of DenverFollow
M Palatiello, Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
V S. Paliya, Clemson University, Kinard Lab of Physics
M Pesce-Rollins, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
V Petrosian, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
F Piron, Laboratoire Univers et Particules de Montpellier, Université Montpellier
T A. Porter, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
G Principe, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics
S Rainò, Università e del Politecnico di Bari, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
B Rani, NASA Goddard Space Flight Center
M Razzano, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
S Razzaque, University of Johannesburg
A Reimer, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University, Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck
O Reimer, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University, Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck
C Sgrò, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
E J. Siskind, NYCB Real-Time Computing Inc.
G Spandre, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
P Spinelli, California State University, Università e del Politecnico di Bari
H Tajima, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University, Solar-Terrestrial Environment Laboratory, Nagoya University
J B. Thayer, W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
D J. Thompson, NASA Goddard Space Flight Center
D F. Torres, Institute of Space Sciences (CSICIEEC), Campus UAB, Carrer de Magrans, Institució Catalana de Recerca i Estudis Avançats (ICREA)
E Torresi, INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Bologna
E Troja, University of Padova, Vicolo Osservatorio, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics
J Valverde, Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3
K Wood, Praxis Inc., resident at Naval Research Laboratory
M Yassine, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Università di Trieste
Fermi-LAT Collaboration

Publication Date

5-1-2019

Document Type

Article

Organizational Units

Physics and Astronomy

Keywords

Pulsars, General, Gamma rays, General, Astroparticle physics

Abstract

The HAWC Collaboration released the 2HWC catalogue of TeV sources, in which 19 show no association with any known high-energy (HE; E ≳ 10 GeV) or very-high-energy (VHE; E ≳ 300 GeV) sources. This catalogue motivated follow-up studies by both the Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) and Fermi-LAT (Large Area Telescope) observatories with the aim of investigating gamma-ray emission over a broad energy band. In this paper, we report the results from the first joint work between High Altitude Water Cherenkov (HAWC), MAGIC, and Fermi-LAT on three unassociated HAWC sources: 2HWC J2006+341, 2HWC J1907+084*, and 2HWC J1852+013*. Although no significant detection was found in the HE and VHE regimes, this investigation shows that a minimum 1° extension (at 95 per cent confidence level) and harder spectrum in the GeV than the one extrapolated from HAWC results are required in the case of 2HWC J1852+013*, whilst a simply minimum extension of 0.16° (at 95 per cent confidence level) can already explain the scenario proposed by HAWC for the remaining sources. Moreover, the hypothesis that these sources are pulsar wind nebulae is also investigated in detail.

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