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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:
- toolbox.imgtools.mstools: Contains image manipulation tasks created especially for STIS and NICMOS image set (imset) data and which exploit the error and data quality arrays in their operations (e.g., msarith, mscombine, msstatistics, mssplit, and msjoin). These tasks are described in "Working with STIS and NICMOS Imsets" on page 3-12.
- hst_calib.stis: Contains the STIS specific tasks basic2d, calstis, ocrreject, wavecal, x1d, and x2d.
In addition to the above packages, most basic image manipulation software (e.g., display, daophot, imexamine, contour, etc.) and spectral analysis software (e.g., splot, tables, specfit, igi, etc.) available in IRAF/STSDAS can be used on STIS data, either directly through the IRAF FITS interface or by converting data to another IRAF format. Chapter 3 includes information about how to display STIS images and extracted spectra as well as how and when to convert data formats and a description of spectral analysis taks. Table 23.1 lists some of the more useful IRAF/STSDAS applications for working with STIS data.
Some of the tasks are intended for browsing data or producing publication-quality plots: the igi and sgraph tasks were described in Chapter 3. The echplot task is useful for browsing STIS extracted spectra. You can plot single spectral orders, overplot multiple orders on a single plot, or plot up to 4 orders in separate panels on the same page. For example, we overplot the orders contained in rows 2 through 4 and 6 on one page:
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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