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 5.6931e-04 Jy/beam
minimum 1.0362e-04 Jy/beam
mean 1.6841e-04 Jy/beam
median 1.3067e-04 Jy/beam
sigma 7.9112e-05 Jy/beam
MAD rms 1.4376e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_0.J213113_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_0.J213113+114236_P30593v1_2019_01_22T17_39_14.575/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_0.J213113+114236_P30593v1_2019_01_22T17_39_14.575/working
Start time
2019-01-24 16:53:36.699
End
2019-01-24 16:55:48.204
Duration
0:02:11.505
Note, WebLog generation is not included in the time.

CASA logs for stage 6