Hi Dustin, Hi everybody
I would like to solve an image that astrometry (local version) already solved but with another star catalog.
For example suppose I'd like to solve an image with 5200 index, and this image is already solved with 4100 index.
From the first solving procedure, astrometry returns these files: .axy, .corr, .out, .rdls, .solved, .wcs, .xyls
Can I use one of these files to solve again the image?
What I know is that the .xyls file returns the x y coordinates of the stars present in the field of view (is it right?), and that I can use this information to solve an image.
If I can use one of the files mentioned above file, what should be the solve-field line command format?
Thanks for the help.
GZ