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 6.5116e-04 Jy/beam
minimum 1.1007e-04 Jy/beam
mean 1.8902e-04 Jy/beam
median 1.4328e-04 Jy/beam
sigma 9.4163e-05 Jy/beam
MAD rms 2.2397e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_1.J235744_094236.10.2048.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.J235744+094236_P30535v1_2019_01_22T18_56_07.476/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J235744+094236_P30535v1_2019_01_22T18_56_07.476/working
Start time
2019-01-24 19:08:38.399
End
2019-01-24 19:10:24.370
Duration
0:01:45.972
Note, WebLog generation is not included in the time.

CASA logs for stage 6