Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-03-14
Astronomy and Astrophysics
Astrophysics
Scientific paper
10.1051/0004-6361:20053498
A procedure is described for estimating an optimum kernel for the detection
by convolution of signals among Poissonian noise. The technique is applied to
the detection of x-ray point sources in XMM-Newton data, and is shown to yield
an improvement in detection sensitivity of up to 60% over the sliding-box
method used in the creation of the 1XMM catalog.
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