Abstract
The DArk Matter Particle Explorer (DAMPE) can measure γ-rays in the energy range from a few GeV to about 10 TeV. The direction of each γ-ray photon is reconstructed in the DAMPE payload reference system. To convert this to celestial coordinates, we require the celestial orientation of the payload system, which, however, may slightly deviate from that of the satellite system provided by the star-tracker. In this paper, we adopt a maximum likelihood method and use the γ-rays centered around several bright point-like sources to measure and correct the angular deviations between the DAMPE payload and satellite system, the so-called “boresight alignment”. We also check our method of boresight alignment for some sets of simulation data with artificial orientations and obtain consistent results. The time-dependent boresight alignment analysis does not show evidence for significant variation of the parameters.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
