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 1.1415e-03 Jy/beam
minimum 1.2563e-04 Jy/beam
mean 2.0420e-04 Jy/beam
median 1.5913e-04 Jy/beam
sigma 1.0003e-04 Jy/beam
MAD rms 2.2137e-05 Jy/beam

RMS images

TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms

Pilot.ql.SGC1B_1.J234202_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_1.J234202+034235_P31788v1_2019_02_04T17_24_56.086/working/TSKY0001.sb32444332.eb32455291.57585.22032424768_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1B_1.J234202+034235_P31788v1_2019_02_04T17_24_56.086/working
Start time
2019-02-07 01:22:43.062
End
2019-02-07 01:24:44.556
Duration
0:02:01.494
Note, WebLog generation is not included in the time.

CASA logs for stage 6