====== Final Spec. tables with memberships, morphologies, masses, etc ======

**A963:**

To come... I am checking consistency with latest HI tables

**A2192:**

{{budhies:optical:A2192_final_with_additional_HI.txt.tar.gz}}


__Some important notes:__

Numbers = -111 were placed when there is no information available

HI galaxies (according to latest tables by Boris) are those with ID_HI > 0
Note that we used to use zf to know which were HI galaxies but those values are old (for HI galaxies), so use ID_HI
trustable redshifts are those with trust_re >= -1

membership flag corresponds to main structure, "1" for A2192_1 for example
submembership is available for galaxies inside A2192_1: 
A2192_1a has submem ==10
1b: submem==11
1c: submem==12
1d submem=13

a couple have submem=-10 for example, these are galaxies "in" A2192_1 that we later identified as field population.

I also quote combined_ew_oii, which are: from our spectra, SDSS, OR WYIN spectra, ignore the other columns with OII things on it.

the rest should be obvious enough. Let me know if you have questions

Yara


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