Can anyone point me to some references? Greetings All. I am searching for a couple of numbers, but my books are packed away and stored somewhere due to moving. I was hoping someone could provide the best accepted observational values and the reference sources for those numbers. First I am searching for the best number for the observed number density of all galaxies within about redshift 0.5, ...that is, ..the total number of galaxies per unit volume. I found one publication online that seems to imply that there are about 6 or 12 per cubic Mpc, but not sure about it. I suppose one could find a histogram of galaxies vs redshift and integrate out to say z=0.4, and then divide by the volume therein, but I'm not sure if those histograms are over the total angular sky or just a section of it. Also there's probably galaxies that don't show up on the histogram maybe because they're not big or bright enough or something. Secondly I am looking for the best accepted average cross sectional size, ( or equivalently the diameter) for all the galaxies implied in the above paragraph, ..indeed if there is such a calculation somewhere. There are surely several ways to do this. I think over half of those galaxies are irregulars, maybe a third spirals, and the rest ellipticals, etc. Also I think the diameters of those are supposed to be maybe 1 to 10 kpc for irregulars, 5 to 50 kpc for spirals, and 1 to 200 kpc for ellipticals. Maybe the geometric mean or something for each type could be taken and then multiplied times the respective percentage of that type, and then all types averaged together or something like that. Also, maybe the total semi-local mass density could be divided by the average mass of all galactic types, or mass of each type averaged individually, and then multiplied by the percentage of the type, and then by the average size But I digress......maybe the best average cross section is already done and published somewhere, ...and so that's what I am asking. Wikipedia says that the diameters range from about 1,000 to about 100,000 parsecs, and so from that I'd guess that an average would end up being about 10,000 pc or less. Thirdly, but less importantly, I could use the reference to the best histogram of all types of quasars vs redshift, ...out to maybe z=4, or around there. It would also be helpful to know the total local number density of all quasars semi-locally within redshift 0.3 or 0.4. Again, I'm not sure if those counts have been done over the total angular sky or not. Maybe they've been done over part of the sky and then extrapolated to the entire sky or something. Thanks much in advance if you can help finding any of those references, and best regards.