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 6.7858e-04 Jy/beam
minimum 1.1165e-04 Jy/beam
mean 1.7934e-04 Jy/beam
median 1.3524e-04 Jy/beam
sigma 8.5940e-05 Jy/beam
MAD rms 1.5346e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J013405_054235.10.2048.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_SGC2E_0.J013405+054235_P30409v1_2019_02_09T00_47_49.016/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J013405+054235_P30409v1_2019_02_09T00_47_49.016/working
Start time
2019-02-11 06:41:53.940
End
2019-02-11 06:43:55.472
Duration
0:02:01.532
Note, WebLog generation is not included in the time.

CASA logs for stage 6