https://github.com/RadioAstronomySoftwareGroup/pyuvdata
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Tip revision: b86f3ea682d8441fc6d368a1c323ae8d7f166929 authored by jburba on 01 March 2018, 15:08:13 UTC
Updating plotting output
Tip revision: b86f3ea
history
CORR-DACQ: created file.
/usr/local/bin/correct_psa128.py zen.2456865.60537.xy.uv
/usr/local/bin/xrfi_simple.py -a 1 --df=6 -c 0_65,377_388,510,770,840,852,913,921_922,932_934,942_1023 --combine -t 80 zen.2456865.60537.xy.uvc
/usr/local/bin/xrfi_simple.py -a all --combine -t 80 --from_npz=zen.2456865.60537.xy.uvcRE.npz zen.2456865.60537.xy.uvcR
DDR FILTER, DDR:/usr/local/bin/ddr_filter_coarse.py -a all -p xx,xy,yx,yy --maxbl=301 --clean=1e-3 --output=ddr --nsections=20 zen.2456865.59841.xy.uvcR zen.2456865.60537.xy.uvcRR zen.2456865.61232.xy.uvcR
PULL CHANS:/Users/djacobs/scripts/pull_chans.py -c 100_110 zen.2456865.60537.xy.uvcRRE
PULL ANTPOLS:/Users/djacobs/scripts/pull_antpols.py -a (0,1,2,3,4,5)_(0,1,2,3,4,5) zen.2456865.60537.xy.uvcRREA
  Read/written with pyuvdata version: 1.4.2.  Git origin: https://github.com/RadioAstronomySoftwareGroup/pyuvdata.git.  Git hash: 3e18b8b4b8fab07067857d6025700df5367334e7.  Git branch: new_version.  Git description: v1.4-532-g3e18b8b4-dirty.  Downselected to specific times using pyuvdata.  Downselected to specific frequencies using pyuvdata.
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