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 6.4353e-04 Jy/beam
minimum 1.1416e-04 Jy/beam
mean 1.7728e-04 Jy/beam
median 1.3816e-04 Jy/beam
sigma 8.0622e-05 Jy/beam
MAD rms 1.4364e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J014210_064235.10.2048.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.J014210+064235_P30421v1_2019_02_09T00_48_09.022/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J014210+064235_P30421v1_2019_02_09T00_48_09.022/working
Start time
2019-02-11 13:15:58.993
End
2019-02-11 13:18:09.585
Duration
0:02:10.593
Note, WebLog generation is not included in the time.

CASA logs for stage 6