Paper 13093-180
BEaTriX x-ray calibration facility: status of the project
17 June 2024 • 17:30 - 19:00 Japan Standard Time | Room G5, North - 1F
Abstract
BEaTriX, the Beam Expander Testing X-ray facility, is operated by the INAF-Brera Astronomical Observatory
at its premises in Merate (Italy) as ground support equipment for the verification phase in the context of
NewAthena. The facility is very compact but, thanks to an innovative optical design based on asymmetrical
cut crystals associated with a paraboloidal mirror, can produce an expanded low divergence X-ray beam at the two monochromatic energies of 4.51 keV and 1.49 keV. The first beamline at 4.51 keV is already operational, as the commissioning was completed in Q12023. The second beamline at 1.49 keV energy has more challenging aspects from both design and implementation points of view: the monochromator stage is made with two Quartz crystals with asymmetric cut; the expansion phase is made by two ADP crystals also with asymmetric cut; the X-ray source needs to be very brilliant due to the large fraction of photons rejected by the crystals. This paper describes the activities on going: the 4.51 keV X-ray beamline optimization and the tests performed on a coated MM will be presented. The progress in the implementation of the 1.49 keV components will be described.
Presenter
Davide Sisana
Politecnico di Milano (Italy), INAF - Osservatorio Astronomico di Brera (Italy)
PhD student in Aerospace Engineering (Politecnico di Milano and INAF-OAB) - Development of advanced facilities for calibration of optics and optical elements for future high-energy astronomical space observatories.