I am analyzing the data of a strong X-Ray source. After determining the
spectrum of the source, I subtracted the Marx-estimate of the source
emission from the data and a statistically highly significant residuum
remains with an event excess at 15''-50'' angular distances from the
Has anybody used in-flight data to compare the wings of the point spread
function with the predictions of the Marx simulations?
In the "Memo regarding the PSF analysis"
wings measured at the XRCF are shown, but the absolute number of events at
a given angular distance from the source is not compared to Marx
-- ** Henric Krawczynski, email: firstname.lastname@example.org, tel: (203) 432 5796 Astronomy Dept.-Yale University-P.O. Box 208101-New Haven, CT 06520-8101 USA
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