Application of an EMCCD camera for calibration of hard X-ray telescopes

摘要

Recent technological innovations make it feasible to construct efficient hard x-ray telescopes for space-basedastronomical missions. Focusing optics are capable of improving the sensitivity in the energy range above 10 keVby orders of magnitude compared to previously used instruments. The last decade has seen focusing opticsdeveloped for balloon experiments and they are implemented in approved space missions such as the NuclearSpectroscopic Telescope Array (NuSTAR). The full characterization of x-ray optics for astrophysical missions,including measurement of the point spread function (PSF) as well as scattering and reflectivity properties of substrate coatings, requires a large area detector with very high spatial resolution and sensitivity, photon countingand energy discriminating capability. Novel back-thinned Electron Multiplying Charge-Coupled Devices (EMCCDs) are suitable detectors for ground-based calibrations if combined with a scintillating material. This opticalcoupling of the EMCCD chip to a microcolumnar CsI(Tl) scintillator can be achieved via a fiberoptic taper. Notonly does this detector system exhibit low noise and high spatial resolution inherent to CCDs, but the EMCCDis also able to handle high frame rates. Additionally, thick CsI(Tl) yields high detection efficiency for x-rays. Inthis paper, we discuss the advantages of using an EMCCD to calibrate hard x-ray optics. We will illustrate thepromising features of this detector solution using examples of data obtained during the ground calibration of theNuSTAR telescopes performed at Columbia University during 2010/2011. Finally, we give an outlook on latestdevelopment and optimizations.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.