Hi Jon, 

Sorry for the late response! For Q4, I have 5 targets that I need to get KOSMOS (red and/or blue) observations for, and 6 targets that I need to get DIS R1200/B1200 observations for. 

The PAs for these targets should be aligned with the radio axis of the sources as indicated by FIRST imaging. I have already calculated those PAs, but I can upload the FIRST images to a google drive if you would like to have the students compute those angles. 

I am attaching a tui catalog for each set of targets (KOSMOS or DIS) and some READ ME files with a few more details on each set of targets. Let me know if you need anything else from me. 

Best,
Kelly

Target list:
Green DRAGNs: Gp238_parad (blue only), Gp145_parad (red only), Gp059_parad, Gp023_parad, Gp166_parad


Main Scientific Goals: 

As detailed in the program proposal text, we have completed our redshift campaign to identify a subset of AGN hosting radio jets that lie in the redshift range 0.3 < z < 0.6, i.e. the redshift range of the confirmed radio-quiet Green Bean galaxies. In collecting these data, we discovered evidence for jet-CGM interactions in sources for which the long-slit position angle (PA) happened to be aligned with the radio-jet axis of the source. Motivated by these findings, we are returning to some of the previously observed sources for which the PA was not aligned with the radio-jet axis to obtain follow-up observations with the long-slit PA aligned to the radio emission.  


Observation Requirements: 

        Instrument: KOSMOS

                center+1.18” setup
        
        Sky requirements: Dark

        SN requirement for each target: S/N >= 15 (at least 3 exp per target)

        Position angles: Determined to be aligned with the radio axes of the targets as indicated by FIRST imaging. For sources whose radio axes is not well defined, the PA is aligned with the best guess of the radio axes. These PAs are given in the tui catalog. 


File Description:

Q4_ASTR535_KSandersonKOSMOSObs.tui.txt: tui catalog of the sources and their PAs