Also included are the date and time. Analysis Files SAS outputs files to a directory specified in the configuration file . If a file for a given galaxy already exists, then the new analysis data is appending to the old file. At the top of each output file, the same identification lines that were input into the galaxy list file are printed. If the spectrum was fluxed, all amplitudes are microJanskys.
All wavelengths are angstroms.
This lists the name of the spectrum file used for the current analysis, the spacing in angstroms per pixel in both the observed and rest frames, and the grating type of the mask. The wavelength of the feature in both the observed and rest frames is first listed, followed by the continuum intervals that were used. The final equivalent width value given is that calculated by integrating the Gaussian fit divided by the continuum level over the feature region. Lastly, the Chi squared value of the fit is included. Just as before, the data is output with an identifying line followed by the continuum intervals and the mean, standard deviation, center, and pixels of the continua.