As I try to understand the SeeStar and applicability to photometry, I imaged the Standard Fields M 67 and Melotte 111. I extracted the TG/TB from the FITS files, and plotted the Catalog G/B versus my measured TG/TB:
It appears that I have good correlation for V vs TG and B vs. TB, however there is more noise in the B/TB data.
Next, from there, I captured the catalog B-V and plotted it against my instrumental TB-TG:
Looking at the data, there is an offset between the M 67 and Melotte 111 data, however the slopes of the curves are virtually identical.
My question is “Did I do this right?” and “Does my data look reasonable?”
Thanks
Scott (MDSA)