I have a few things I've been working on improving or fixing for a while, so here it goes:
The largest field size of my images are around 6x6 arcminutes and I can solve these in around 4-5 seconds (on a relatively beefy machine). To do this I downsample my images and provide a ra and dec and a radius of 0.2 degrees (which is actually quite big considering the field size, but lower than that and it sometimes fails). Here are the CLI parameters I use:
'--extension', '1',
'--no-plots',
'--overwrite',
'--dir', '/tmp/',
'--downsample', str(int(4/frame.binning[0])), # This is just to ensure that the product pixel size will be the same even for differently binned images
'--fits-image',
'--ra', str(frame.target_ra_deg),
'--dec', str(frame.target_dec_deg),
'--radius', '0.2', # degrees
I have also been trying to solve some .fits files with field sizes of around 2.85 x 2.85 arcmin on my local astrometry installation. They already contain a WCS accurate to a few arcseconds (which is not sufficient in my case), but for some reason I am unable to solve these images. I believe I have sufficient index files (please see below), and the
nova.astrometry.net solver is able to do it in only around a second. What gives?
I have attached two images that are representative of my data.
ALIa310083 is the larger 6x6 arcmin image while ALIa310084 is the smaller of the two.
Any help is much appreciated.