Detection of point sources with spark chamber gamma-ray telescopes

Details Detection of point sources with spark chamber gamma-ray telescopes Detection of point sources with spark chamber gamma-ray telescopes

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..220..316m&link_type=abstract

In: High energy gamma-ray astronomy; Proceedings of the International Conference, Ann Arbor, MI, Oct. 2-5, 1990 (A93-25001 08-93

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Gamma Ray Telescopes, Point Sources, Point Spread Functions, Spark Chambers, Cross Correlation, Maximum Likelihood Estimates

Scientific paper

The sensitivity of cross correlation and maximum likelihood, two methods
under consideration by the EGRET team for detecting point sources, is
analyzed numerically. Cross correlation is found to be 9 +/- 2 percent
more sensitive than maximum likelihood.

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