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high-energy astrophysics

Long-term gamma-ray observations of the binary HESS J0632+057 with H.E.S.S., MAGIC and VERITAS

arXiv:1908.03589

summary

The paper presents over ten years of very‑high‑energy gamma‑ray observations of the binary system HESS J0632+057 with the H.E.S.S., MAGIC, and VERITAS telescopes, including a bright TeV outburst in January 2018 and a light curve covering almost all orbital phases, complemented by simultaneous Swift X‑ray data.

Abstract

The gamma-ray binary HESS J0632+057 has been observed at very-high energies (E $>$ 100 GeV) for more than ten years by the major systems of imaging atmospheric Cherenkov telescopes. We present a summary of results obtained with the H.E.S.S., MAGIC, and VERITAS experiments based on roughly 440 h of observations in total. This includes a discussion of an unusually bright TeV outburst of HESS J0632+057 in January 2018. The updated gamma-ray light curve now covers all phases of the orbital period with significant detections in almost all orbital phases. Results are discussed in context with simultaneous observations with the X-ray Telescope onboard the Neil Gehrels Swift Observatory.

Proceedings of the 36th International Cosmic Ray Conference (ICRC2019) Madison, WI July 24-Aug 1, 2019

Topics & keywords

#gamma-ray binary#very-high-energy observations#orbital modulation#multi-instrument campaign#TeV outburstHESS J0632+057imaging atmospheric Cherenkov telescopeslight curveSwift XRTTeV outburst