Determination of the eROSITA mirror half energy width (HEW) with subpixel resolution

Konrad Dennerl; Wolfgang Burkert; Vadim Burwitz; Michael Freyberg; Peter Friedrich; Gisela Hartner

doi:10.1117/12.926988

17 September 2012 Determination of the eROSITA mirror half energy width (HEW) with subpixel resolution

Konrad Dennerl, Wolfgang Burkert, Vadim Burwitz, Michael Freyberg, Peter Friedrich, Gisela Hartner

Proceedings Volume 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray; 844350 (2012) https://doi.org/10.1117/12.926988
Event: SPIE Astronomical Telescopes + Instrumentation, 2012, Amsterdam, Netherlands

Abstract

The Point Spread Function (PSF) of the eROSITA miror modules is specified to have an on-axis Half Energy Width (HEW) of 15 arcsec. This is only slightly larger than the eROSITA pixel size of 75 microns, which corresponds to 9.6 arcsec at the PANTER test facility, where the PSF is being measured with a prototype of the eROSITA CCD. We have developed a fast algorithm which provides a substantially higher spatial resolution by utilizing the information contained in the charge ratios of split events. By applying this algorithm to measurements where the CCD is systematically shifted in subpixel increments (typically in a 12x12 pattern), we are able to achieve an effective resolution of ~2 arcsec for specific pixel patterns. This algorithm can also be used to compute the two dimensional probability distribution for detecting a photon from an incident point-like beam, for each combination of photon energy, low energy threshold, selected pixel patterns, and subpixel scan properties. These maps allow us to deconvolve the measured PSF and thus to minimize the influence of the spatial detector resolution on the determination of the eROSITA mirror HEW. After launch, the algorithm for improving the spatial resolution by reconstructing the subpixel position will also be applied to the science data.

Citation Download Citation

Konrad Dennerl, Wolfgang Burkert, Vadim Burwitz, Michael Freyberg, Peter Friedrich, and Gisela Hartner "Determination of the eROSITA mirror half energy width (HEW) with subpixel resolution", Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 844350 (17 September 2012); https://doi.org/10.1117/12.926988

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