Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel’dovich effect

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Table 3

Results for both datasets.

Input maps	Found clusters	Confirmed clusters	Purity^a (%)	Completeness^b (%)

“Homemade” + HWGN	766	725	94.6	72.5
“Homemade” + NASC	813	804	98.9	80.4
LAMBDA + HWGN	3928	3873	98.6	0.034
LAMBDA + NASC	3560	3550	99.7	0.031

Notes.

^(a)

Purity = true detections/total detection;

^(b)

completeness = true detections/simulated clusters.

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