MUZZIN A. byWILSON G. , LACY M., YEE H.K.C., STANFORD S.A. Astrophys. J., 686, 966-994 (2008) The evolution of dusty star formation and stellar mass assembly in clusters: results from the IRAC 3.6, 4.5, 5.8, and 8.0 µm cluster luminosity functions. oTable 1: <[MWL2008] NN> (Nos 0-98) = <[MWL2008] FLS JHHMMSS+DDMM.m> N=99. =E=Catalogue in electronic form as <J/ApJ/686/966/>
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