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 9.3031e-04 Jy/beam
minimum 1.2382e-04 Jy/beam
mean 1.9832e-04 Jy/beam
median 1.5521e-04 Jy/beam
sigma 9.0666e-05 Jy/beam
MAD rms 1.9265e-05 Jy/beam

RMS images

TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms

Pilot.ql.SGC1B_0.J214601_024235.10.2048.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.J214601+024235_P31819v1_2019_02_04T17_25_43.504/working/TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1B_0.J214601+024235_P31819v1_2019_02_04T17_25_43.504/working
Start time
2019-02-07 01:14:59.322
End
2019-02-07 01:17:02.904
Duration
0:02:03.582
Note, WebLog generation is not included in the time.

CASA logs for stage 6