MAXI J1820+070 shows no significant very high energy gamma-ray emission above 182 GeV despite a bright X-ray outburst, and optical transient activity drops sharply during state transitions.
The VERITAS standard data analysis
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abstract
VERITAS is an array of Imaging Atmospheric Cherenkov Telescopes designed for very high energy gamma ray (E>100,GeV) observations of astrophysical sources. The experiment began its scientific observation program in the 2006/2007 observing season. We describe here the analysis chain for reducing the data, reconstructing the direction and energy of incident gamma rays and the rejection of background cosmic rays.
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Multi-wavelength observation of MAXI J1820+070 with MAGIC, VERITAS and H.E.S.S
MAXI J1820+070 shows no significant very high energy gamma-ray emission above 182 GeV despite a bright X-ray outburst, and optical transient activity drops sharply during state transitions.