fit-wcs: invalid option -- '-' fit-wcs: invalid option -- 'e' This program is part of the Astrometry.net suite. For details, visit http://astrometry.net. Git URL https://github.com/dstndstn/astrometry.net Revision 0.72, date Mon_Jul_10_14:37:28_2017_-0400. Usage: fit-wcs -x <xyls input file> [-X <x-column-name> -Y <y-column-name>] -r <rdls input file> [-R <RA-column-name> -D <Dec-column-name>] OR -c <correspondences file> (default column names: FIELD_X, FIELD_Y, INDEX_RA, INDEX_DEC) -o <WCS output file> [-s <SIP-order>] (default is a WCS TAN solution, not SIP) [-W <image-width> ] (default: max X position; used for SIP) [-H <image-height>] (default: max Y position; used for SIP) [-C]: set CRPIX to be the center of the field; SIP only [-v]: verbose

fit-wcs: invalid option -- '-' This program is part of the Astrometry.net suite. For details, visit http://astrometry.net. Git URL https://github.com/dstndstn/astrometry.net Revision 0.72, date Mon_Jul_10_14:37:28_2017_-0400. Usage: fit-wcs -x <xyls input file> [-X <x-column-name> -Y <y-column-name>] -r <rdls input file> [-R <RA-column-name> -D <Dec-column-name>] OR -c <correspondences file> (default column names: FIELD_X, FIELD_Y, INDEX_RA, INDEX_DEC) -o <WCS output file> [-s <SIP-order>] (default is a WCS TAN solution, not SIP) [-W <image-width> ] (default: max X position; used for SIP) [-H <image-height>] (default: max Y position; used for SIP) [-C]: set CRPIX to be the center of the field; SIP only [-v]: verbose