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Cited article:

The correct estimate of the probability of false detection of the matched filter in weak-signal detection problems

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Astronomy & Astrophysics 604 A115 (2017)
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The first source counts at 18 μm from the AKARI NEP Survey

Chris P. Pearson, S. Serjeant, S. Oyabu, et al.
Monthly Notices of the Royal Astronomical Society 444 (1) 846 (2014)
https://doi.org/10.1093/mnras/stu1472

Detection of new point sources in WMAP cosmic microwave background maps at high Galactic latitude

E. P. R. G. Ramos, R. Vio and P. Andreani
Astronomy & Astrophysics 528 A75 (2011)
https://doi.org/10.1051/0004-6361/201015586

Bayesian Methods of Astronomical Source Extraction

Richard S. Savage and Seb Oliver
The Astrophysical Journal 661 (2) 1339 (2007)
https://doi.org/10.1086/515393

A high-accuracy method for the removal of point sources from maps of the cosmic microwave background

A. T. Bajkova
Astronomy Reports 49 (12) 947 (2005)
https://doi.org/10.1134/1.2139810

ON THE LINEAR FILTERS FOR POINT SOURCE EXTRACTION OF THE PLANCK MISSION

LUNG-YIH CHIANG, PAVEL D. NASELSKY and IGOR D. NOVIKOV
International Journal of Modern Physics D 14 (07) 1251 (2005)
https://doi.org/10.1142/S0218271805007097

Some good reasons to use matched filters for the detection of point sources in CMB maps

R. Vio, P. Andreani and W. Wamsteker
Astronomy & Astrophysics 414 (1) 17 (2004)
https://doi.org/10.1051/0004-6361:20031632