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 6.3316e-04 Jy/beam
minimum 1.1229e-04 Jy/beam
mean 1.7937e-04 Jy/beam
median 1.3957e-04 Jy/beam
sigma 8.4467e-05 Jy/beam
MAD rms 1.6482e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J201957_413000.10.2048.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.J201957+413000_P33710v1_2019_02_07T16_12_08.861/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J201957+413000_P33710v1_2019_02_07T16_12_08.861/working
Start time
2019-02-09 12:39:46.854
End
2019-02-09 12:42:00.197
Duration
0:02:13.343
Note, WebLog generation is not included in the time.

CASA logs for stage 6