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 7.3333e-04 Jy/beam
minimum 1.1539e-04 Jy/beam
mean 1.9811e-04 Jy/beam
median 1.5024e-04 Jy/beam
sigma 9.7118e-05 Jy/beam
MAD rms 1.9813e-05 Jy/beam

RMS images

TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms

Pilot.ql.SGC1B_1.J231400_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_1.J231400+024235_P31771v1_2019_02_04T17_24_15.674/working/TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1B_1.J231400+024235_P31771v1_2019_02_04T17_24_15.674/working
Start time
2019-02-05 18:25:58.768
End
2019-02-05 18:27:47.862
Duration
0:01:49.094
Note, WebLog generation is not included in the time.

CASA logs for stage 6