RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 5.7403e-04 Jy/beam
minimum 1.0919e-04 Jy/beam
mean 1.7300e-04 Jy/beam
median 1.3116e-04 Jy/beam
sigma 8.3828e-05 Jy/beam
MAD rms 1.4315e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J203701_443000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203701+443000_P33743v1_2019_02_07T17_03_55.268/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203701+443000_P33743v1_2019_02_07T17_03_55.268/working
Start time
2019-02-09 01:41:26.812
End
2019-02-09 01:43:42.031
Duration
0:02:15.219
Note, WebLog generation is not included in the time.

CASA logs for stage 6