VCSBeam version
Required: >= v2.18.1.
# On Garrawarla, test vcsbeam version $ module use /pawsey/mwa/software/python3/modulefiles $ module load vcsbeam MWA Beamformer v2.18.1_e79c6bd
Calibration
Offline FinePFB
$ cd /astro/mwavcs/vcs/1318345216/combined
$ for freq in {109..120}
do
sed "s/FREQ/${freq}/" < make_legacy.sbatch > make_legacy_ch${freq}.sbatch
sbatch make_legacy_ch${freq}.sbatch
done
Offline Correlator
$ cd /astro/mwavcs/vcs/1318345216/cal/1318345216/vis
$ for freq in {109..120}
do
sed "s/FREQ/${freq}/" < offline_correlate.sbatch > offline_correlate_${freq}.sbatch
sbatch offline_correlate_${freq}.sbatch
done
RTS
Create source list
$ cd /astro/mwavcs/vcs/1318345216/cal/1318345216
$ module load srclists/v1.0.0
$ srclist_by_beam.py -m /astro/mwavcs/vcs/1318345216/1318345216_metafits_ppds.fits -n 1000 -s ${SRCLISTS_DIR}/srclist_pumav3_EoR0aegean_EoR1pietro+ForA.txt
Set up flagged tiles
To find which tiles need to be flagged, find the broken tiles by going to the observation status page (http://ws.mwatelescope.org/observation/obs/?obs_id=1318345216). In the section "Tile errors and flags", you will find the "TileNames" for any tiles that should be flagged. Then, in the metafits file for the observation, you will find the "Input" numbers associated with the X and Y polarisations of each tile. The numbers you need to put in the "flagged_tiles.txt" are the Input numbers divided by two (and possibly rounded down). For example, in 1318345216, Tile064 is listed as broken, and in the metafits file, that tile's polarisations are associated with inputs 144 & 145. This means that the number that goes into flagged_tiles.txt for this tile is 72. In this way, the following list is constructed for this observation.
1 12 45 51 60 72 93 94 112
Set up flagged channels
Setting up the flagged channels is more straightforward. As a rule, we always flag the edge channels (80 kHz worth on either side) and the centre channel. Since we have averaged up to 40 kHz when we did the offline correlation step above, that means we will be flagging the outer two channels on either side (as 2 x 40 kHz = 80 kHz) and the single centre channel. Since there are 32 channels in this case, the final list of flagged channels is:
0 1 16 30 31
Extra flags
After running the RTS (see below) and checking the solutions (using the python scripts supplied in VCSTools), I found that I also had to add 14 to the list of flagged channels, and 52, 53 and 59 to the list of flagged tiles.
Run the RTS
$ cd /astro/mwavcs/vcs/1318345216/cal/1318345216/rts $ sbatch /astro/mwavcs/vcs/1318345216/batch/RTS_1318345216.batch
Make a "calibration" metafits
In order to be able to use this calibration solution for beamforming, mwalib has to be "tricked" into getting the frequency resolution right (i.e. whatever we set during the offline correlation step). To do this, make a copy of the metafits file and change
FINECHAN → 40 (kHz)
NCHANS → 768
MODE → 'HWLFILES'
I then saved this file to /astro/mwavcs/vcs/1318345216/cal/1318345216_cal.metafits.
(MEMO TO SELF: write a utility script to do this for you.)
Beamform
For the time being, we have to "trick" the beamformer into thinking this is a legacy VCS observation, instead of an MWAX VCS observation. I did this by creating a copy of the metafits file and changing the "MODE" and "NCHANS" fields to 'VOLTAGE_START' and 3072, respectively. [MEMO TO SELF: add an option to "force" the beamformer to treat it as a legacy obs, if you want to beamform from the .dat files produced by the offline PFB.]
Transfer the flagged tiles from the RTS
$ cd /astro/mwavcs/vcs/1318345216/vcsbeam $ /PATH/TO/rts_flag_ant_to_tilenames.py 1318345216_cal.metafits flagged_tiles.txt > flagged_tilenames.txt
$ cd /astro/mwavcs/vcs/1318345216/vcsbeam $ echo "00:34:08.8703 -07:21:53.409" > pointings.txt $ sbatch vcsbeam.sbatch