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 6.3944e-04 Jy/beam
minimum 1.2077e-04 Jy/beam
mean 1.9263e-04 Jy/beam
median 1.5080e-04 Jy/beam
sigma 8.9226e-05 Jy/beam
MAD rms 1.5808e-05 Jy/beam

RMS images

TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms

Pilot.ql.SGC1B_0.J213001_034235.10.2048.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.J213001+034235_P31825v1_2019_02_04T17_25_52.502/working/TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1B_0.J213001+034235_P31825v1_2019_02_04T17_25_52.502/working
Start time
2019-02-06 16:37:25.941
End
2019-02-06 16:39:45.729
Duration
0:02:19.788
Note, WebLog generation is not included in the time.

CASA logs for stage 6