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 5.9371e-04 Jy/beam
minimum 1.0574e-04 Jy/beam
mean 1.7521e-04 Jy/beam
median 1.3324e-04 Jy/beam
sigma 8.7655e-05 Jy/beam
MAD rms 1.9873e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_1.J232116_114236.10.2048.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_SGC3B_1.J232116+114236_P30548v1_2019_01_22T18_56_30.957/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J232116+114236_P30548v1_2019_01_22T18_56_30.957/working
Start time
2019-01-24 02:52:23.191
End
2019-01-24 02:54:34.766
Duration
0:02:11.575
Note, WebLog generation is not included in the time.

CASA logs for stage 6