"Phillip Helbig---remove CLOTHES to reply"
wrote in message ...
In article , "PoorRichard"
writes:

My question is, what approach for computing a (meaningful) LF is best in
this situation? I have been reading many of the major papers on LFs
(Schmidt
1968; Lynden-Bell 1971; Schechter 1976; etc.)...but it has not all fully
digested yet .

We need one additional piece of information. Are these objects and
cosmologically significant distances?


Ah yes, that is important! The objects (type 2 AGN) are fairly local; z
0.03. I am dealing with cm wavelength.

Thanks