A simple recispe for reducing three nights is given below.
# Specify where the raw data are stored and which night are to be processed % cat BaseDir /home/sco/AD/HET_work/acm_nights % cat head -5 list.Dates 20170903 20180402 20190219 % acm_BigRed list.Dates N N arg1 - Name of file with list of UT dates to be processed arg2 - Allow interactive query of user (Y/N) arg3 - run in verbose/debug modeAfter the acm_BigRed has completed the run, then your processed images will reside in the current working directory in subdirectories named for each UT night processed.
% ls 20170903/ 20180402/ 20190219/ BaseDir list.Dates ACM.images ACM.parlab ACM.table list.IMAGES Mean.BIAS list.BIAS list.DARK list.OPEN Inside each date subdirectory are the processed images , for example: % pwd /home/sco/ACM_BIAS_STUDY/reds5/20190219/local_red % ls FIXUP/ HDFIX/ HDFIX = images with cleaned and augmented image headers HDFIX = bias (including FBP) and dark frame corrected imagesAs the pipeline progresses other subdirectories will appear.
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An example of before- and after- CCD-processing. |