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| The example 1 plot after the matplotlib show() routine runs. The xyplotter file is really running a python code named pxy_SM_plot.py (which you can read about in my Big List of codes). |
You can use the link here to grab the Ex1 tar file. After you have downloaded the tar file:
% cp ~sco/Downloads/Ex1.tar . # Use whatever path you need. % tar xvf Ex1.tar % cd Ex1 % cp S/* . % ls Axes d1.params d1.table d32.table d64.table dB.table List.all d16.table d1.parlab d2.table d4.table d8.table dO.table S/ % xyplotter List.all Axes N Title = 20170906 Bias and Dark (Overscan and Active Areas) X: 2.0 3.75 Xtitle = Time (hours since UT=0) Y: 1000 2000 Ytitle = Acquisition Camera Signal (adu) To see the plot: pxy_SM_plot.py STYLE 2.0 3.75 1000 2000 SHOW View plot now? (Y/N)YAfter you answer "Y" above, then you'll see the plot appear using the matplotlib show() routine. You can adjust the scaling and placement of the data, make a hard copy, etxc... The figure below shows what you should see:
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| The example 1 plot after the matplotlib show() routine runs. The xyplotter file is really running a python code named pxy_SM_plot.py (which you can read about in my Big List of codes). |
The files in the sample directory are mostly table files. The only essential part of a table file is the *.table file. Here is a sample of the files used here that were compiled using multiple runs of the fits_review routine:
% cat d1.table # Col01: image number # Col02: image name # Col03: object card value # Col04: filter name # Col05: RA in sexigecimal format # Col06: DEC in sexigecimal format # Col07: structure azimuth # Col08: parallactic angle # Col09: wcs presence # Col10: image source # Col11: time in dayas since Jan1UT=0 # Col12: time in hours since UT=0 # Col13: signal in bias area (adu) # Col14: signal in active area (adu) # Col15: exptime in seconds # Col16: flux (adu/sec) above bias # Col17: mean error in flux # data 1 20170906T021054.8_acm_sci ___ i` 01:13:04.604880 +65:36:09.864000 0.002117 0.004408 Y acm 248.091156 2.18774 1172.6884 1399.5804 227.0091 1 227.009100 2 20170906T021059.5_acm_sci ___ i` 01:13:04.916160 +65:36:09.745200 0.002117 0.004408 Y acm 248.091232 2.18955 1172.8101 1399.5564 226.9518 1 226.951800 3 20170906T021104.1_acm_sci ___ i` 01:13:05.227440 +65:36:09.630000 0.002117 0.004408 Y acm 248.091034 2.18491 1172.3223 1399.4897 226.9955 1 226.995500 4 20170906T021108.8_acm_sci ___ i` 01:13:05.538720 +65:36:09.514800 0.002117 0.004408 Y acm 248.091110 2.18672 1172.9232 1399.6877 227.0539 1 227.053900 5 20170906T021113.4_acm_sci ___ i` 01:13:05.836560 +65:36:09.403200 0.002117 0.004408 Y acm 248.091187 2.18849 1172.8722 1399.5879 226.9421 1 226.942100 6 20170906T021118.1_acm_sci ___ i` 01:13:06.147840 +65:36:09.288000 0.002117 0.004408 Y acm 248.091263 2.19029 1172.8505 1399.5830 226.9458 1 226.945800 7 20170906T021122.7_acm_sci ___ i` 01:13:06.459120 +65:36:09.172800 0.002117 0.004408 Y acm 248.091339 2.19206 1172.6592 1399.5503 226.9690 1 226.969000 8 20170906T021127.3_acm_sci ___ i` 01:13:06.770400 +65:36:09.057600 0.002117 0.004408 Y acm 248.091415 2.19383 1172.8846 1399.5699 226.9350 1 226.935000 9 20170906T021132.0_acm_sci ___ i` 01:13:07.081440 +65:36:08.942400 0.002117 0.004408 Y acm 248.091492 2.19564 1172.8358 1399.4679 226.8533 1 226.853300 10 20170906T021136.6_acm_sci ___ i` 01:13:07.392960 +65:36:08.823600 0.002117 0.004408 Y acm 248.091553 2.19741 1172.8313 1399.4053 226.7877 1 226.787700 11 20170906T021141.3_acm_sci ___ i` 01:13:07.70400 +65:36:08.708400 0.002117 0.004408 Y acm 248.091629 2.19922 1172.6782 1399.3777 226.7746 1 226.774600 12 20170906T021145.9_acm_sci ___ i` 01:13:08.015280 +65:36:08.593200 0.002117 0.004408 Y acm 248.091705 2.20099 1172.3564 1399.4358 226.9464 1 226.946400 13 20170906T021150.6_acm_sci ___ i` 01:13:08.326560 +65:36:08.481600 0.002117 0.004408 Y acm 248.091782 2.20280 1173.0643 1399.3932 225.9452 1 225.945200 14 20170906T021155.3_acm_sci ___ i` 01:13:08.637840 +65:36:08.362800 0.002117 0.004408 Y acm 248.091858 2.20460 1172.8717 1399.3685 226.7629 1 226.762900 15 20170906T021159.9_acm_sci ___ i` 01:13:08.949120 +65:36:08.247600 0.002117 0.004408 Y acm 248.091934 2.20637 1172.4292 1399.3552 226.8556 1 226.855600 16 20170906T021204.5_acm_sci ___ i` 01:13:09.260400 +65:36:08.136000 0.002117 0.004408 Y acm 248.091736 2.20173 1172.8682 1399.5303 226.9226 1 226.922600 17 20170906T021209.2_acm_sci ___ i` 01:13:09.571680 +65:36:08.017200 0.002117 0.004408 Y acm 248.091812 2.20354 1172.5969 1399.3293 226.7527 1 226.752700 18 20170906T021213.9_acm_sci ___ i` 01:13:09.882960 +65:36:07.902000 0.002117 0.004408 Y acm 248.091888 2.20535 1172.9689 1399.4453 226.8151 1 226.815100 19 20170906T021218.5_acm_sci ___ i` 01:13:10.194240 +65:36:07.783200 0.002117 0.004408 Y acm 248.091965 2.20712 1173.0444 1399.4113 225.9697 1 225.969700 20 20170906T021223.2_acm_sci ___ i` 01:13:10.505520 +65:36:07.671600 0.002117 0.004408 Y acm 248.092041 2.20892 1173.0453 1399.3038 225.8610 1 225.861000 21 20170906T021227.8_acm_sci ___ i` 01:13:10.816800 +65:36:07.556400 0.002117 0.004408 Y acm 248.092117 2.21069 1172.6267 1399.2246 226.6286 1 226.628600 22 20170906T021232.4_acm_sci ___ i` 01:13:11.128080 +65:36:07.441200 0.002117 0.004408 Y acm 248.092178 2.21246 1172.8282 1399.3958 226.8018 1 226.801800 23 20170906T021237.1_acm_sci ___ i` 01:13:11.439360 +65:36:07.322400 0.002117 0.004408 Y acm 248.092255 2.21427 1173.4150 1399.3811 225.9047 1 225.904700 24 20170906T021241.7_acm_sci ___ i` 01:13:11.750640 +65:36:07.207200 0.002117 0.004408 Y acm 248.092331 2.21604 1172.8212 1399.3511 226.7411 1 226.741100 25 20170906T021246.4_acm_sci ___ i` 01:13:12.048480 +65:36:07.095600 0.002117 0.004408 Y acm 248.092407 2.21785 1173.4043 1399.3923 225.8988 1 225.898800 26 20170906T021251.1_acm_sci ___ i` 01:13:12.373200 +65:36:06.973200 0.002117 0.004408 Y acm 248.092484 2.21965 1172.4883 1399.1281 226.6314 1 226.631400 27 20170906T021255.7_acm_sci ___ i` 01:13:12.684480 +65:36:06.861600 0.002117 0.004408 Y acm 248.092560 2.22142 1172.4528 1399.2069 226.7122 1 226.712200This file is not teribbly easy to read, but I have a lot of tools to read and cutup such files. Some of these tool take advantage of supplemental files like these:
% cat d1.params imgnum fitsname object filter RAsex DECsex AZ parang wcsp imgtype days hours bias signal exptime flux fluxerr % cat d1.parlab imgnum Image number fitsname Name of FITS image object Object Name filter Filter RAsex RA (J2000.0) DECsex DEC (J2000.0) AZ HET Structure Azimuth (degrees) parang HET Parallactic Angle (degrees) wcsp WCS presence imgtype Image Source days Time (days since Jan1 UT=0) hours Time (hours since UT=0) bias Bias (adu) signal Signal (adu) in active area exptime Exposure time (seconds) flux Flux (ADU/sec) above bias fluxerr Flux errorI have only included the params and parlab files for the d1 table file. You could run just the d1 data through xyplotter using a very simple command like:
% xyplotter_auto d1 hours signal 1You can read about xyplotter_auto. It will handle building the Axis and List files. Then you can add more lines to the List file to add more data sets to your plot. Let's take a final look at the List.1 file in our example:
% cat List.all dO.table 12 13 0 0 point r o 30 Over dB.table 12 14 0 0 pointopen r . 50 A Bias d1.table 12 14 0 0 pointopen b 1 50 A 1 d2.table 12 14 0 0 pointopen g 2 50 A 2 d4.table 12 14 0 0 pointopen m 3 50 A 4 d8.table 12 14 0 0 pointopen r 4 50 A 8 d16.table 12 14 0 0 pointopen b 8 50 A 16 d32.table 12 14 0 0 pointopen g + 50 A 32 d64.table 12 14 0 0 pointopen m s 50 A 64The contents of these lines are explained elsewhere, but a brief reminder is given here:
column 1 = name of the table file to get X,Y data from columns 2-5 = column numbers of X,Y,Xerr,Yerr column 6 = type of marker to plot column 7 = color symbol column 8 = plot symbol column 9 = symbol size column 10 = name of data set for plot legend