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 5.9519e-04 Jy/beam
minimum 1.1060e-04 Jy/beam
mean 1.7625e-04 Jy/beam
median 1.3397e-04 Jy/beam
sigma 8.4017e-05 Jy/beam
MAD rms 1.3729e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J012202_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.J012202+054235_P30406v1_2019_02_09T00_47_44.035/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J012202+054235_P30406v1_2019_02_09T00_47_44.035/working
Start time
2019-02-11 07:33:56.351
End
2019-02-11 07:35:58.681
Duration
0:02:02.331
Note, WebLog generation is not included in the time.

CASA logs for stage 6