solve_astrometry_xy#

astropop.astrometry.solve_astrometry_xy(x, y, flux, width, height, image_header=None, options=None, command=None, **kwargs)#

Solve astrometry from a (x,y) sources list using astrometry.net.

Parameters:

x: array-like: x positions of the sources in the image.
y: array-like: y positions of the sources in the image.
flux: array_like: Estimated fluxes of the sources. A higher value indicates a brighter star.
width: int: Image width.
height: int: Image height.
image_header: `~astropy.fits.Header` (optional): Original image header.
options: dict: Dictionary of solve-field options. See print_options_help for all available options. The most useful are: - center or ra and dec: field center - radius: maximum search radius - scale: pixel scale in arcsec/pixel - tweak-order: SIP order to fit - index-path: path to index files
command: str: Full path of astrometry.net solve-field command.

Returns:

solve_astrometry_xy