An empirical method corrects clustering bias in P(D) galaxy number counts, showing that clustering inflates 500μm counts by a factor of 1.6 near 10 mJy in Herschel-SPIRE GOODS-N data.
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How to count clustered galaxies
An empirical method corrects clustering bias in P(D) galaxy number counts, showing that clustering inflates 500μm counts by a factor of 1.6 near 10 mJy in Herschel-SPIRE GOODS-N data.