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23.1 Data Reduction Applications

Most of the new software tools for operating on STIS FITS files are contained in two STSDAS packages:

cl> echplot "stis_x1d.fits[1][r:row=(2:4,6)]" output.igi \
>>> plot_style=m
Note that the the plot_style parameter governs whether the spectral orders are plotted one per page, overplotted, or plotted one per panel, for parameter values of "s", "m", or "p" respectively. The brightness unit is calibrated FLUX by default, though other quantities (e.g., NET counts) can be specified using the flux_col parameter.



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