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@ARTICLE{Acharyya:623131,
      author       = {Acharyya, A. and Adams, C. B. and Bangale, P. and
                      Bartkoske, J. T. and Benbow, W. and Buckley, J. H. and
                      Christiansen, J. L. and Chromey, A. J. and Duerr, A. and
                      Errando, M. and Falcone, A. and Feng, Q. and Foote, G. M.
                      and Fortson, L. and Furniss, A. and Hanlon, W. and Hanna, D.
                      and Hervet, O. and Hinrichs, C. E. and Holder, J. and
                      Humensky, T. B. and Jin, W. and Kaaret, P. and Kertzman, M.
                      and Kieda, D. and Kleiner, T. K. and Korzoun, N. and Kumar,
                      Shashank and Lang, M. J. and Lundy, M. and Maier, G. and
                      McGrath, C. E. and Millard, M. J. and Millis, J. and Mooney,
                      C. L. and Moriarty, P. and Mukherjee, R. and Ning, W. and
                      Ong, R. A. and Park, N. and Pohl, M. and Pueschel, E. and
                      Quinn, J. and Rabinowitz, P. L. and Ragan, K. and Ribeiro,
                      D. and Roache, E. and Ryan, J. L. and Sadeh, I. and Saha, L.
                      and Sembroski, G. H. and Shang, R. and Splettstoesser, M.
                      and Talluri, A. K. and Tucci, J. V. and Valverde, J. and
                      Vassiliev, V. V. and Weinstein, A. and Williams, D. A. and
                      Wong, S. L. and Woo, J. and Alfaro, R. and Alvarez, C. and
                      Arteaga-Velázquez, J. C. and Rojas, D. Avila and Babu, R.
                      and Belmont-Moreno, E. and Bernal, A. and Caballero-Mora, K.
                      S. and Capistrán, T. and Carramiñana, A. and Casanova, S.
                      and Cotzomi, J. and de León, S. Coutiño and De la Fuente,
                      E. and Depaoli, D. and Di Lalla, N. and Hernandez, R. Diaz
                      and DuVernois, M. A. and Espinoza, C. and Fan, K. L. and
                      Fang, K. and Fraija, N. and Garcı́a-González, J. A. and
                      Garfias, F. and González, M. M. and Goodman, J. A. and
                      Groetsch, S. and Hernández-Cadena, S. and Hinton, J. and
                      Huang, D. and Hueyotl-Zahuantitla, F. and Iriarte, A. and
                      Kaufmann, S. and Kieda, D. and Lee, J. and León Vargas, H.
                      and Longinotti, A. L. and Luis-Raya, G. and Malone, K. and
                      Martı́nez-Castro, J. and Matthews, J. A. and
                      Miranda-Romagnoli, P. and Morales-Soto, J. A. and Moreno, E.
                      and Mostafá, M. and Nellen, L. and Pérez-Pérez, E. G. and
                      Rho, C. D. and Rosa-González, D. and Salazar, H. and
                      Sandoval, A. and Schneider, M. and Serna-Franco, J. and Son,
                      Y. and Springer, R. W. and Tibolla, O. and Tollefson, K. and
                      Torres, I. and Torres-Escobedo, R. and Turner, R. and
                      Ureña-Mena, F. and Varela, E. and Wang, X. and Zhou, H. and
                      Eagle, J. and Kumar, S.},
      collaboration = {{VERITAS Collaboration} and {HAWC Collaboration} and
                      Fermi-{LAT Collaboration}},
      title        = {{M}ultiwavelength {I}nvestigation of γ-{R}ay {S}ource
                      {MGRO} {J}1908+06 {E}mission {U}sing {F}ermi-{LAT},
                      {VERITAS} and {HAWC}},
      journal      = {The astrophysical journal / Part 1},
      volume       = {974},
      number       = {1},
      issn         = {0004-637X},
      address      = {London},
      publisher    = {Institute of Physics Publ.},
      reportid     = {PUBDB-2025-00618, arXiv:2408.01625},
      pages        = {61 -},
      year         = {2024},
      note         = {Grants DE-AC02-76SF00515; DE-AC02-05CH11231},
      abstract     = {This paper investigates the origin of the γ-ray emission
                      from MGRO J1908+06 in the GeV–TeV energy band. By
                      analyzing the data collected by the Fermi Large Area
                      Telescope, the Very Energetic Radiation Imaging Telescope
                      Array System, and High Altitude Water Cherenkov, with the
                      addition of spectral data previously reported by LHAASO, a
                      multiwavelength study of the morphological and spectral
                      features of MGRO J1908+06 provides insight into the origin
                      of the γ-ray emission. The mechanism behind the bright TeV
                      emission is studied by constraining the magnetic field
                      strength, the source age, and the distance through detailed
                      broadband modeling. Both spectral shape and energy-dependent
                      morphology support the scenario that inverse Compton
                      emission of an evolved pulsar wind nebula associated with
                      PSR J1907+0602 is responsible for the MGRO J1908+06 γ-ray
                      emission with a best-fit true age of T = 22 ± 9 kyr and a
                      magnetic field of B = 5.4 ± 0.8 μG, assuming the distance
                      to the pulsar d$_{PSR}$ = 3.2 kpc.},
      cin          = {$Z_GA$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)Fermi-20170101 /
                      EXP:(DE-H253)VERITAS-20170101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2408.01625},
      howpublished = {arXiv:2408.01625},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2408.01625;\%\%$},
      UT           = {WOS:001350239100001},
      doi          = {10.3847/1538-4357/ad698d},
      url          = {https://bib-pubdb1.desy.de/record/623131},
}