I have uploaded the catalogs with the coordinates of the UV sources with optical counterparts (from Yara's redshift catalog) for both clusters. The columns are explained below:
1. Optical number (the same one used by Yara)
2. UV number (from the GALEX pipeline, I use it because it makes my life easier)
3. Optical RA (from Yara's catalog)
4. Optical Dec (same as above)
5. UV RA (from GALEX's catalog)
6. UV Dec (same as above)
7. nuv (only detected in NUV)/ fuv (only detected in FUV). Detected in both if blank.
I have separated the catalogs in three groups:
A963
-Cluster members: 0.1897<z<0.2223 ⇒ A963 cluster members
-Foreground members: z<0.1897 ⇒ A963 foreground members
-Background members: z>0.2223 ⇒ A963 background members
A2192
-Cluster members: 0.1803<z<0.1957 ⇒ A2192 cluster members
-Foreground members: z<0.1803 ⇒ A2192 foreground members
-Background members: z>0.1957 ⇒ A2192 background members
SFRs
I have uploaded the SFRs. The columns go as above, with the exception of column 7, where I have posted the SFRs.
A963
Cluster: A963 cluster SFRs
Foreground: A963 foreground SFRs
Background: No SFR for the background source (only FUV detected)
A2192
Cluster: A2192 cluster SFRs
Foreground: A2192 foreground SFRs
Background: A2192 background SFRs
A963
A2192
