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| Code Block |
|---|
| language | bash |
|---|
| theme | Midnight |
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| title | /astro/mwavcs/vcs/1323690320/hyperdrive/hyperdrive.sbatch |
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| collapse | true |
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|
#!/bin/bash -l
#SBATCH --job-name=hyp-$1
#SBATCH --output=hyperdrive.out
#SBATCH --nodes=1
#SBATCH --ntasks-per-node=40
#SBATCH --time=01:00:00
#SBATCH --clusters=garrawarla
#SBATCH --partition=gpuq
#SBATCH --account=mwavcs
#SBATCH --export=NONE
#SBATCH --gres=tmp:50g
#SBATCH --gres=gpu:1
# Load the Hyperdrive module
module use /pawsey/mwa/software/python3/modulefiles
module load hyperdrive
module load
vcsbeam
set -eux
which hyperdrive
# The location of the correlated visibility FITS files:
DATADIR=/astro/mwavcs/asvo/253001
# The path to the associated metafits filesfile
CAL_METAFITS=${DATADIR}/1323690320.metafits
OBS_METAFITS=/astro/mwavcs/asvo/253008/1323690616.metafits
# <-- This is the observation for which the calibration solution is needed
# The base source list (you shouldn't need to change this)
SRCLIST=/pawsey/mwa/software/python3/srclists/master/srclist_pumav3_EoR0aegean_fixedEoR1pietro+ForA_phase1+2.txt
# If it hasn't been done already, run Hyperdrive in "srclist-by-beam" to get just the subset of sources in the beam
if [[ ! -r srclist_1000.yaml ]]; then
hyperdrive srclist-by-beam \
-n 1000 \
-m ${CAL_METAFITS} \
/pawsey/mwa/software/python3/srclists/master/srclist_pumav3_EoR0aegean_fixedEoR1pietro+ForA_phase1+2.txt \
srclist_1000.yaml
fi
# Run Hyperdrive to generate a calibration solution
hyperdrive di-calibrate \
-s srclist_1000.yaml \
-d ${DATADIR}/*.fits \
${CAL_METAFITS} |
Run the Hyperdrive script (on Garrawarla):
| Code Block |
|---|
| language | bash |
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| theme | Midnight |
|---|
| title | Run Hyperdrive on Garrawarla |
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|
cd /astro/mwavcs/vcs/1323690320/hyperdrive
sbatch hyperdrive.sbatch |
Create VCSBeam plotting script:
| Code Block |
|---|
| language | bash |
|---|
| theme | Midnight |
|---|
| title | /astro/mwavcs/vcs/1323690320/hyperdrive/plot.sbatch |
|---|
| collapse | true |
|---|
|
#!/bin/bash -l
#SBATCH --job-name=plot_calsol
#SBATCH --output=plot_calsol.out
#SBATCH --nodes=1
#SBATCH --ntasks-per-node=2
#SBATCH --time=01:00:00
#SBATCH --clusters=garrawarla
#SBATCH --partition=gpuq
#SBATCH --account=mwavcs
#SBATCH --export=NONE
#SBATCH --gres=tmp:50g
#SBATCH --gres=gpu:1
# Load the VCSBeam module
module use /pawsey/mwa/software/python3/modulefiles
module load vcsbeam
# The location of the correlated visibility FITS files:
DATADIR=/astro/mwavcs/asvo/253001
# The paths to the associated metafits files
CAL_METAFITS=${DATADIR}/1323690320.metafits
OBS_METAFITS=/astro/mwavcs/asvo/253008/1323690616.metafits # <-- This is the observation for which the calibration solution is needed
# Use VCSBeam to plot the solutions
srun -N 1 -n 1 mwa_plot_calibration -m ${OBS_METAFITS} -c ${CAL_METAFITS} -C hyperdrive_solutions.bin -R NONE -U 0,0 -O -X -z nan > plot_data.txt
# The following will have to be done on your own computer (not on Garrawarla)
# Download
# (1) plot_calibration.py (use "which plot_calibration.py" to find out where it is)
# (2) plot_data.txt
# and then run the following
#plot_calibration.py --phases_png phases.png --amps_png amps.png plot_data.txt |
Run the Hyperdrive script (on Garrawarla)plotting script:
| Code Block |
|---|
| language | bash |
|---|
| theme | Midnight |
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| title | Run Hyperdrive VCSBeam plotting on Garrawarla |
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|
cd /astro/mwavcs/vcs/1323690320/hyperdrive
sbatch hyperdriveplot.sbatch |
Plot the calibration solutions (on your local computer, after downloading a copy of plot_calibration.py and plot_data.txt:
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