Here I discuss how to run a night of data through fits_review. I also show how to make a table file for the results and plot various parameters from the images.
Work in: /home/sco/HET_reds/20170903/S To create input list: ls -1 /home/sco/HET_work/acm_nights/20170903/acm/201*.fits > list.all cp /home/sco/HET_work/acm_nights/20170903/*.txt . Survey all images and select images for fits_review (i.e. for wcs) ds9_list_load list.all mv List.New list.1 cp list.1 S ds9_list_load list.1 # Optional check To pocess (first pass): fits_review list.1 N # To get list with image properties fits_review_table Y xyplotter_auto fits_review hours bias 1 xyplotter_auto fits_review hours flux 1 xyplotter_auto fits_review exptime flux 1 fits_review list.1 Y NOTE: After the start of any fits_review you get the file: fits_review.params_used This can be renamed to fits_review.defaults and used to change reduction paramters % mv fits_review.params_used fits_review.defaults % vi fits_review.defaults To archive the images: fits_review_archive list.1 To studty stats: cd Archive_WCS ls -1 *.fits >list.1 fits_review_summary list.1 20170903 We see a tbale lke: RArms DECrms Nstars AZ Q pscal CROTA2 TZ Image Name 1.048 1.114 61 29.52 52.83 0.27101 216.529 90.637 20170906T064343.6_acm_sci.fits 0.662 0.623 53 29.52 52.83 0.27081 216.497 90.669 20170906T072326.3_acm_sci.fits 0.494 0.399 59 22.58 42.63 0.27042 226.777 90.593 20170906T074533.8_acm_sci.fits 0.695 1.090 26 347.18 334.25 0.27032 295.085 90.667 20170906T091636.0_acm_sci.fits I have a table file: 20170906.table I can make plots: xyplotter_auto 20170906 AZ TZ 1 xyplotter_auto 20170906 AZ pscal 2
On 20171108 I took a lot of bias and dark images. I had a dark dome, the FCU head deployed, and the acm mirror was out. I combined images using the folowing steps:
To process 60sec darks ls -1 /home/sco/HET_work/acm_nights/20171108/acm/20*fits > list.all fits_review list.all N fits_review_table N xyplotter_auto fits_review imgnum exptime 1 cut_by_line cut_by_line list.all 832 878 list.dark60 acm_stack list.dark60 9 mv Big_Stack.fits dark60_raw.fits ds9_open 900 900 ds9_view dark60_raw.fits zscale n 1 In ./bias I used the same methods to stack 225 bias image to get Mbias1.fits To make a bias subtracted dark for 60 sec: clip_imarith.sh dark60_raw.fits - ../bias/Mbias1.fits dark60.fits