The nu flags, net, background, and ripple-corrected fluxes may be optionally returned. In general, one may not know what data fields these p-arguments correspond to until they are printed out. An input string array header can be specified for creating the primary FITS header. Additional rows can be appended to existing binary tables. Converts images to primary array FITS images.
Output is FITS primary array or binary table extensions.
Each row of the binary table denotes data for a spectral order. Most are modified forms of borrowed versions suitable for IUE data.