Status: WIP
For any source that passes the Caltech ZTF CLU filter, we know that the source by default will have cross-match redshifts, and separation in arcseconds from the CLU galaxy. We have identified several cases that:
- The CLU redshift is not consistent with the SDSS galaxy spectrum redshift (usually when one is available)
- Some other group might have identified the redshift of this source & is not associated with that CLU galaxy
To collect the proper redshift information from Fritz. Here are a few ideas & cases on when and how to collect the proper redshift information:
- By default, always assume that the correct redshift has been entered to Fritz in the source redshift tab.
1A. Given the redshift collected from the header (i.e redshift tab) of the source, we will search through all the CLU cross-matches and find that redshift with the closest
Status: WIP
For any source that passes the Caltech ZTF CLU filter, we know that the source by default will have cross-match redshifts, and separation in arcseconds from the CLU galaxy. We have identified several cases that:
To collect the proper redshift information from Fritz. Here are a few ideas & cases on when and how to collect the proper redshift information:
1A. Given the redshift collected from the header (i.e redshift tab) of the source, we will search through all the CLU cross-matches and find that redshift with the closest