Once the results of the processing are assembled, they are written to a FITS file. The extensive primary header of this file contains relevant information regarding the observation run (see Appendix B). Following this header are a series of FITS binary table extension headers and associated tables. One table extension for each detected object is written. These tables contain 5 columns which contain the wavelength and flux vectors of the extracted spectra along with vectors for the statistical, deblending, and total errors from the extraction process.