Upper Limits on Gamma-ray Emission from Supernovae Serendipitously Observed with H.E.S.S

Autor: N. Maxted, Jacco Vink, Rachel Simoni, Mathieu Renaud
Přispěvatelé: Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), HESS, Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), High Energy Astrophys. & Astropart. Phys (API, FNWI)
Rok vydání: 2017
Předmět:
Zdroj: IAU Symp.
IAU Symposium 331
IAU Symposium 331, Feb 2017, Saint-Gilles-Les-Bains, France. pp.325-328, ⟨10.1017/S1743921317004628⟩
Proceedings of the International Astronomical Union, 12(S331), 325-328. Cambridge University Press
ISSN: 1743-9221
1743-9213
Popis: It is hypothesized that some young supernovae might have the correct properties to accelerate cosmic rays, which in turn might generate gamma-ray emission by-products. We search for gamma-ray excesses towards supernovae in nearby galaxies which were serendipitously within the field of view of the HESS telescopes within a year of the supernova event. HESS cherenkov air-shower data collected between December 2003 and March 2015 were considered and compared to recent catalogs. Nine candidate supernovae were identified and analysed. No significant emission from these supernovae has been found, and upper limits for their very high energy emission are reported.
Databáze: OpenAIRE