TY - JOUR
T1 - HAWC and Fermi-LAT Detection of Extended Emission from the Unidentified Source 2HWC J2006+341
AU - HAWC Collaboration
AU - Albert, A.
AU - Alfaro, R.
AU - Alvarez, C.
AU - Angeles Camacho, J. R.
AU - Araya, M.
AU - Arteaga-Velázquez, J. C.
AU - Arunbabu, K. P.
AU - Avila Rojas, D.
AU - Ayala Solares, H. A.
AU - Baghmanyan, V.
AU - Belmont-Moreno, E.
AU - Brisbois, C.
AU - Caballero-Mora, K. S.
AU - Carramiñana, A.
AU - Casanova, S.
AU - Cotti, U.
AU - de la Fuente, E.
AU - de León, C.
AU - Diaz Hernandez, R.
AU - Dingus, B. L.
AU - DuVernois, M. A.
AU - Durocher, M.
AU - Díaz-Vélez, J. C.
AU - Espinoza, C.
AU - Fleischhack, H.
AU - Fraija, N.
AU - Galván-Gámez, A.
AU - Garcia, D.
AU - García-González, J. A.
AU - Garfias, F.
AU - González, M. M.
AU - Goodman, J. A.
AU - Harding, J. P.
AU - Hona, B.
AU - Huang, D.
AU - Hueyotl-Zahuantitla, F.
AU - Hüntemeyer, P.
AU - Iriarte, A.
AU - Jardin-Blicq, A.
AU - Joshi, V.
AU - León Vargas, H.
AU - Linnemann, J. T.
AU - Longinotti, A. L.
AU - López-Coto, R.
AU - Luis-Raya, G.
AU - Lundeen, J.
AU - Malone, K.
AU - Martinez, O.
AU - Martínez-Castro, J.
AU - Matthews, J. A.
N1 - Publisher Copyright:
© 2020. The American Astronomical Society. All rights reserved.
PY - 2020/11/1
Y1 - 2020/11/1
N2 - The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes, and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004 +3429 due to extreme energetics required, if located at a distance of 10.8 kpc.
AB - The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes, and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004 +3429 due to extreme energetics required, if located at a distance of 10.8 kpc.
UR - http://www.scopus.com/inward/record.url?scp=85095883843&partnerID=8YFLogxK
U2 - 10.3847/2041-8213/abbfae
DO - 10.3847/2041-8213/abbfae
M3 - Artículo
AN - SCOPUS:85095883843
SN - 2041-8205
VL - 903
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 1
M1 - L14
ER -