Changes between Version 18 and Version 19 of Notes/ExampleReduction


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Timestamp:
03/31/09 12:42:29 (15 years ago)
Author:
JamieStevens
Comment:

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  • Notes/ExampleReduction

    v18 v19  
    190190band only.
    191191
    192 Now we are ready to image the source.
     192Now we are ready to image the source. In the DAC method, there are three ways to make images of the source
     193without recombining the UV data first. We will attempt all three methods:
     1941. invert using the MFS option as normal, then clean and restor
     1951. invert using both the MFS option and the SDB option, then use mfsclean and restor
     1961. invert making a cube of all channels, then clean, restor and then make a moment map
     197
     198The first way is the way most familiar to MIRIAD users doing continuum reduction. We can make images of all
     199the individual datasets in the following way:
     200
     201dac_repeat.pl --task invert --repeat vis --repeat-freq rnovalmc --repeat map --repeat-freq rnovalmc_%f.map --repeat beam --repeat-freq rnovalmc_%f.beam "select=-auto,-ant(6)" stokes=ii options=double,mfs slop=1
     202
     203This makes 16 each of the .map and .beam files. Let's get an idea of the RMS noise of each of the maps using
     204imstat. Using kvis we can identify a region (xmin,ymin,xmax,ymax)=(39,0,65,22) that contains no emission.
     205Using dac_repeat.pl we can run imstat on each set:
     206
     207./dac_repeat.pl --task imstat --repeat in --repeat-freq rnovalmc_%f.map "region=boxes(39,0,65,22)" axes=ra,dec
     208
     209From this we find that the RMS noise values are:
     210|| f (MHz) || RMS (uJy) ||
     211|| 4540    || 246       ||
     212|| 4668    || 214       ||
     213|| 4796    || 294       ||
     214|| 4924    || 385       ||
     215|| 5052    || 340       ||
     216|| 5180    || 426       ||
     217|| 5308    || 351       ||
     218|| 5436    || 343       ||
     219|| 5564    || 561       ||
     220|| 5692    || 386       ||
     221|| 5820    || 355       ||
     222|| 5948    || 336       ||
     223|| 6076    || 444       ||
     224|| 6204    || 340       ||
     225|| 6332    || 203       ||
     226|| 6460    || 179       ||
     227
     228This gives us an average RMS of 338 uJy. We can use this value when cleaning:
     229
     230./dac_repeat.pl --task clean --repeat map --repeat-freq rnovalmc_%f.map --repeat beam --repeat-freq rnovalmc_%f.beam --repeat out --repeat-freq rnovalmc_%f.clean cutoff=0.001014
     231
     232And restor:
     233
     234./dac_repeat.pl --task restor --repeat model --repeat-freq rnovalmc_%f.clean --repeat beam --repeat-freq rnovalmc_%f.beam --repeat map --repeat-freq rnovalmc_%f.map --repeat out --repeat-freq rnovalmc_%f.restor
     235