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 6.8317e-04 Jy/beam
minimum 1.1473e-04 Jy/beam
mean 1.8938e-04 Jy/beam
median 1.4329e-04 Jy/beam
sigma 9.4025e-05 Jy/beam
MAD rms 1.7222e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J203932_373000.10.2048.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.J203932+373000_P33671v1_2019_02_07T15_27_56.166/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203932+373000_P33671v1_2019_02_07T15_27_56.166/working
Start time
2019-02-08 17:35:55.139
End
2019-02-08 17:37:35.725
Duration
0:01:40.586
Note, WebLog generation is not included in the time.

CASA logs for stage 6