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 7.0513e-04 Jy/beam
minimum 1.3813e-04 Jy/beam
mean 2.2286e-04 Jy/beam
median 1.7754e-04 Jy/beam
sigma 9.1845e-05 Jy/beam
MAD rms 2.4393e-05 Jy/beam

RMS images

TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms

Pilot.ql.SGC1B_0.J214600_014235.10.2048.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_SGC1B_0.J214600+014235_P31809v1_2019_02_04T17_25_27.891/working/TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1B_0.J214600+014235_P31809v1_2019_02_04T17_25_27.891/working
Start time
2019-02-06 01:50:47.835
End
2019-02-06 01:52:55.244
Duration
0:02:07.409
Note, WebLog generation is not included in the time.

CASA logs for stage 6