RT Journal Article
T1 MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sources
A1 Barrio Uña, Juan Abel
A1 Contreras González, José Luis
A1 Domínguez Díaz, Alberto
A1 Carreto Fidalgo, David Friedrich
A1 Fonseca González, Mª Victoria
A1 López Moya, Marcos
A1 Nievas Rosillo, Mireia
A1 otros, ...
AB The HAWC Collaboration released the 2HWC catalogue of TeV sources, in which 19 show no association with any known high-energy (HE; E greater than or similar to 10 GeV) or very-high-energy (VHE; E greater than or similar to 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 degrees 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 degrees (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.
PB Wiley
SN 0035-8711
YR 2019
FD 2019-05
LK https://hdl.handle.net/20.500.14352/13395
UL https://hdl.handle.net/20.500.14352/13395
LA eng
NO © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Artículo firmado por 343 autores. The MAGIC Collaboration would like to thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The financial support of the German BMBF and MPG, the Italian INFN and INAF, the Swiss National Fund SNF, the ERDF under the Spanish MINECO (FPA2015-69818-P, FPA2012-36668, FPA2015-68378-P, FPA2015-69210-C6-2-R, FPA2015-69210-C6-4-R, FPA2015-69210-C6-6-R, AYA2015-71042-P, AYA2016-76012-C3-1-P, ESP2015-71662-C2-2-P, CSD2009-00064), and the Japanese JSPS and MEXT is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia 'Severo Ochoa' SEV-2012-0234 and SEV-2015-0548, and Unidad de Excelencia 'María de Maeztu' MDM-2014-0369, by the Croatian Science Foundation (HrZZ) Project 09/176 and the University of Rijeka Project 13.12.1.3.02, by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3, and by the Polish MNiSzW grant 745/N-HESS-MAGIC/2010/0.; The HAWC Collaboration acknowledges the support from the US National Science Foundation (NSF) the US Department of Energy Office of High-Energy Physics; the Laboratory Directed Research and Development (LDRD) programme of Los Alamos National Laboratory; Consejo Nacional de Ciencia y Tecnologia (CONACyT), Mexico (grants 271051, 232656, 260378, 179588, 239762, 254964, 271737, 258865, 243290, 132197, 281653)(Cátedras 873, 1563), Laboratorio Nacional HAWC de rayos gamma; L'OREAL Fellowship for Women in Science 2014; Red HAWC, Mexico; DGAPA-UNAM(grants IG100317, IN111315, IN111716-3, IA102715, 109916, IA102917, IN112218); VIEP-BUAP; PIFI 2012, 2013, PROFOCIE 2014, 2015; the University of Wisconsin Alumni Research Foundation; the Institute of Geophysics, Planetary Physics, and Signatures at Los Alamos National Laboratory; Polish Science Centre grant DEC-2014/13/B/ST9/945; Coordinacion de la Investigación Científica de la Universidad Michoacana; Royal Society -Newton Advanced Fellowship 180385. The authors thank to Scott Delay, Luciano Diaz, and Eduardo Murrieta for technical support.; The Fermi-LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States, the Commissariat a l'Energie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan, and the K. A. Wallenberg Foundation, the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is greatefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d'Etudes Spatiales in France. This work is performed in part under DOE Contract DE-AC02- 76SF00515. MR is funded by contract FIRB-2012-RBFR12PM1F from the 847 Italian Ministry of Education, University and Research 848 (MIUR).
NO Ministerio de Economía y Competitividad (MINECO)/FEDER
NO Centro de Excelencia Severo Ochoa
NO Unidad de Excelencia "María de Maeztu"
NO German BMBF
NO MPG
NO Italian INFN
NO INAF
NO Swiss National Fund SNF
NO Japanese JSPS
NO MEXT
NO Croatian Science Foundation (HrZZ)
NO University of Rijeka Project
NO DFG Collaborative Research Centers
NO Polish MNiSzW
NO US National Science Foundation (NSF) the US Department of Energy Office of High-Energy Physics
NO Laboratory Directed Research and Development (LDRD) programme of Los Alamos National Laboratory
NO Consejo Nacional de Ciencia y Tecnologia (CONACyT), Mexico
NO Laboratorio Nacional HAWC de rayos gamma
NO L'OREAL Fellowship for Women in Science
NO Red HAWC, Mexico
NO DGAPA-UNAM
NO VIEP-BUAP
NO PIFI
NO PROFOCIE
NO University of Wisconsin Alumni Research Foundation
NO Institute of Geophysics, Planetary Physics, and Signatures at Los Alamos National Laboratory
NO Polish Science Centre
NO Coordinación de la Investigación Científica de la Universidad Michoacana
NO Royal Society -Newton Advanced Fellowship
NO National Aeronautics and Space Administration
NO Department of Energy in the United States
NO Commissariat a l'Energie Atomique
NO Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France
NO Agenzia Spaziale Italiana
NO Istituto Nazionale di Fisica Nucleare in Italy
NO Ministry of Education, Culture, Sports, Science and Technology (MEXT)
NO K. A. Wallenberg Foundation
NO Swedish Research Council
NO Swedish National Space Board in Sweden
NO Istituto Nazionale di Astrofisica in Italy
NO Centre National d'Etudes Spatiales in France
NO DOE
NO 847 Italian Ministry of Education, University and Research 848 (MIUR)
NO High Energy Accelerator Research Organization (KEK)
NO Japan Aerospace Exploration Agency (JAXA)
DS Docta Complutense
RD 29 abr 2024