In the other thread, I mentioned that whatever Arp et al had found two decades or so ago, they should be able to find 10x, 100x, or more of in the publicly available datasets. I'd love to have enough time to go through each of these, and compare them with what was available to Arp et al all those years ago (but I don't).
Suffice it to say that these data sets are incomparably richer than anything available when Arp first started his professional career. Too, the tools to analyse such vast quantities of data have advanced considerably; for example, the average 'home user' PC of today, priced under US$1,000, is something that professional astronomers would have killed for not too long ago.
So,
the 2dF Galaxy Redshift Survey, high quality redshifts of ~250,000 galaxies, by the Aussies. http://www.2dfquasar.org/results.html#example, an ancilliary survey, of ~10,000 quasars (QSOs) - results include the discovery of quasar evolution - pure luminosity evolution (and overcomes one of Burbidge's early criticisms of the identification of QSOs as cosmologically distant, namely, that the redshift-apparent brightness relationship shows no obvious 'distance' component).
http://www.sdss.org/background/index.html (Sloan Digital Sky Survey), whose description is just breath-taking: "[SDSS] will systematically map one-quarter of the entire sky, producing a detailed image of it and determining the positions and absolute brightnesses of more than 100 million celestial objects. It will also measure the distance to a million of the nearest galaxies, giving us a three-dimensional picture of the universe through a volume one hundred times larger than that explored to date. The Sky Survey will also record the distances to 100,000 quasars, ...[/color]". The object selection method differs from that of 2dF - and the sky covered overlaps! - so there are lots of opportunities to do nice statistical analyses of completeness etc.
The http://hubblesite.org/newscenter/newsdesk/archive/releases/2004/07/, and earlier HDF and HDF-S ... the Hubble Space Telescope spent hundreds of hours collecting photons from small patches of sky. What's not so widely known - outside the astronomical community - is that the same patches of sky were also observed from the X-ray to radio regions of the spectrum, with a huge range of telescopes and instruments. So the EM output of objects in each field is known across a wide range of wavelengths. Related is
GOODS - Great Observatories Origins Deep Survey, in which Spitzer will stare at HDF-N and Chandra Deep South (and Gemini and ESO telescopes will also make detailed studies).
Just one more for now: http://www.subaru.naoj.org/Pressrelease/2004/06/01/index.html , similar in some ways to GOODS.