fredvanner
Well-known member
The output is from the Process Console - the final output from ImageSolver.
ImageSolver needs two inputs: an estimate of the image centre, and an estimate of the image scale (how many arc-seconds per pixel).
The approximate position of M65 is more than precise enough as a start point for ImageSolver.
The image scale is usually specified as the approximate focal length and the approximate pixel size. If you have an Astrometry.net solution it will include the image scale, which you can enter into the ImageSolver interface.
Since I didn't have the image scale, the pixel size or the focal length I estimated the scale from the image.
My planetarium software (Cartes du Ciel) tells me that the angular distance between M65 and 73 Leonis (the brightest star in the image) is about 46' 37.1". Reading the positions out with the cursor in PixInsight, and applying Pythagoras, I find the distance between them in the image is 1076 pixels, giving me about 2.6"/pix.
ImageSolver needs two inputs: an estimate of the image centre, and an estimate of the image scale (how many arc-seconds per pixel).
The approximate position of M65 is more than precise enough as a start point for ImageSolver.
The image scale is usually specified as the approximate focal length and the approximate pixel size. If you have an Astrometry.net solution it will include the image scale, which you can enter into the ImageSolver interface.
Since I didn't have the image scale, the pixel size or the focal length I estimated the scale from the image.
My planetarium software (Cartes du Ciel) tells me that the angular distance between M65 and 73 Leonis (the brightest star in the image) is about 46' 37.1". Reading the positions out with the cursor in PixInsight, and applying Pythagoras, I find the distance between them in the image is 1076 pixels, giving me about 2.6"/pix.