English

Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC

High Energy Astrophysical Phenomena 2020-01-16 v2

Abstract

We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov (HAWC) Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely Galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date. We report the integral flux of each of these objects. We also report spectra for three highest-energy sources and discuss the possibility that they are PeVatrons.

Keywords

Cite

@article{arxiv.1909.08609,
  title  = {Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC},
  author = {HAWC Collaboration and A. U. Abeysekara and A. Albert and R. Alfaro and J. R. Angeles Camacho and J. C. Arteaga-Velázquez and K. P. Arunbabu and D. Avila Rojas and H. A. Ayala Solares and V. Baghmanyan and E. Belmont-Moreno and S. Y. BenZvi and C. Brisbois and K. S. Caballero-Mora and T. Capistrán and A. Carramiñana and S. Casanova and U. Cotti and J. Cotzomi and S. Coutiño de León and E. De la Fuente and C. de León and S. Dichiara and B. L. Dingus and M. A. DuVernois and J. C. Díaz-Vélez and R. W. Ellsworth and K. Engel and C. Espinoza and H. Fleischhack and N. Fraija and A. Galván-Gámez and D. Garcia and J. A. García-González and F. Garfias and M. M. González and J. A. Goodman and J. P. Harding and S. Hernandez and J. Hinton and B. Hona and D. Huang and F. Hueyotl-Zahuantitla and P. Hüntemeyer and A. Iriarte and A. Jardin-Blicq and V. Joshi and S. Kaufmann and D. Kieda and A. Lara and W. H. Lee and H. León Vargas and J. T. Linnemann and A. L. Longinotti and G. Luis-Raya and J. Lundeen and R. López-Coto and K. Malone and S. S. Marinelli and O. Martinez and I. Martinez-Castellanos and J. Martínez-Castro and H. Martínez-Huerta and J. A. Matthews and P. Miranda-Romagnoli and J. A. Morales-Soto and E. Moreno and M. Mostafá and A. Nayerhoda and L. Nellen and M. Newbold and M. U. Nisa and R. Noriega-Papaqui and A. Peisker and E. G. Pérez-Pérez and J. Pretz and Z. Ren and C. D. Rho and C. Rivière and D. Rosa-González and M. Rosenberg and E. Ruiz-Velasco and F. Salesa Greus and A. Sandoval and M. Schneider and H. Schoorlemmer and G. Sinnis and A. J. Smith and R. W. Springer and P. Surajbali and E. Tabachnick and M. Tanner and O. Tibolla and K. Tollefson and I. Torres and R. Torres-Escobedo and L. Villaseñor and T. Weisgarber and J. Wood and T. Yapici and H. Zhang and H. Zhou},
  journal= {arXiv preprint arXiv:1909.08609},
  year   = {2020}
}

Comments

Accepted by Physical Review Letters