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 6.8341e-04 Jy/beam
minimum 1.1798e-04 Jy/beam
mean 1.9604e-04 Jy/beam
median 1.4753e-04 Jy/beam
sigma 9.1941e-05 Jy/beam
MAD rms 2.1643e-05 Jy/beam

RMS images

TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms

Pilot.ql.SGC2B_0.J213806_054235.10.2048.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_SGC2B_0.J213806+054235_P29330v1_2019_02_06T22_09_12.037/working/TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2B_0.J213806+054235_P29330v1_2019_02_06T22_09_12.037/working
Start time
2019-02-07 13:45:27.797
End
2019-02-07 13:46:30.736
Duration
0:01:02.939
Note, WebLog generation is not included in the time.

CASA logs for stage 6