Basic Reduction Steps

  The software available in the CCD package takes care of the relative calibrations of the pixels intensities, for averaging, and for cleaning frames. Cleaning in this context means removal of instrumental signature and other defects from the frames.

A full reduction of CCD data involves the steps outlined below:

• fit and subtract a readout bias given by the overscan strip;
• trim the frame of the overscan strip and other irrelevant columns and/or rows;
• combine the bias, dark, and flats calibration frames (if taken);
• subtract the average bias frame;
• remove the defects from the average dark frame;
• scale and subtract by the average dark frame;
• remove the defects from the average flat frame;
• prepare the final flat (subtract dark and normalize; possibly apply illumination correction);
• divide by the flat field;
• fix the bad pixels in the output frame;
• correct for fringing pattern;
• combine science frames.

Some of these steps are optional and depend on the kind of data you have taken. In addition to the operations described here, MIDAS contains a number of other operations like removing of cosmic rays. As indicated above, all steps can be executed in an automatic (batch) mode provided the keyword settings have been done correctly.

In the automatic procedure, the highest level of processing is the loop over all science frames selected in the reduction table. If, for whatever reason, the processing of a frame fails, this frame is skipped and the processing is continued with the next one.

The CCD package system provides a single command for doing the entire calibration of the CCD frames: REDUCE/CCD. The command is built upon number of lower level procedures, each of them taking care of a particular part of the calibration procedure, and executable via a separate MIDAS command. These components are: overscan correction, trimming, combining, bias correction, dark subtraction, flat fielding, illumination correction, and fringe correction.

Whether you want one or more of calibration steps be executed depends on the settings for the various options. Therefore, before starting be sure that the keywords for the reduction are set correctly. These keywords are listed, with these description, in Table . Also, the keywords for combining calibration frames should be checked. Furthermore, fill the keywords CCDASSOC and CCDREDUC with the name of the association and reduction tables, and check that these tables are correct. All keywords can be filled and displayed with the commands SET/CCD and SHOW/CCD.

  
Table: Keywords for combining bias calibration frames