Long-term gamma-ray observations of the binary HESS J0632+057 with H.E.S.S., MAGIC and VERITAS. (arXiv:1908.03589v1 [astro-ph.HE])

Long-term gamma-ray observations of the binary HESS J0632+057 with H.E.S.S., MAGIC and VERITAS. (arXiv:1908.03589v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Maier_G/0/1/0/all/0/1">G. Maier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Blanch_O/0/1/0/all/0/1">O.Blanch</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hadasch_D/0/1/0/all/0/1">D.Hadasch</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lopez_Oramas_A/0/1/0/all/0/1">A.L&#xf3;pez-Oramas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Komin_N/0/1/0/all/0/1">N.Komin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lundy_M/0/1/0/all/0/1">M.Lundy</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Malyshev_D/0/1/0/all/0/1">D.Malyshev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moepi_J/0/1/0/all/0/1">J.Moepi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ohm_S/0/1/0/all/0/1">S.Ohm</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Puhlhofer_G/0/1/0/all/0/1">G.P&#xfc;hlhofer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Prado_R/0/1/0/all/0/1">R.Prado</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schlenstedt_S/0/1/0/all/0/1">S.Schlenstedt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Torres_D/0/1/0/all/0/1">D.F.Torres</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zitzer_B/0/1/0/all/0/1">B.Zitzer</a> (for the H.E.S.S., MAGIC, and VERITAS Collaborations)

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.

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.

http://arxiv.org/icons/sfx.gif

Comments are closed.