The edge of the M 87 halo and the kinematics of the diffuse light in the Virgo cluster core

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Table 4:

Number of PNs in the photometric samples, for the M 87 halo and the ICL.
Field	$N_{\rm phot}$	$N_{\rm phot}$	$N_{\rm phot}$
		M 87	ICL
FCJ	16^a	14	2
F7	24^b	10	14

^a Number of PNs above the photometric completeness limit from Aguerri et al. (2005). ^b Number of PNs above the photometric completeness from Table 1 in F7_1 and F7_2.

Source LaTeX | All tables | In the text

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