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 9.7186e-04 Jy/beam
minimum 1.1195e-04 Jy/beam
mean 1.8584e-04 Jy/beam
median 1.4220e-04 Jy/beam
sigma 9.2920e-05 Jy/beam
MAD rms 2.1956e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_1.J023803_084236.10.2048.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_1.J023803+084236_P30395v1_2019_02_09T00_47_25.719/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_1.J023803+084236_P30395v1_2019_02_09T00_47_25.719/working
Start time
2019-02-11 19:26:35.347
End
2019-02-11 19:28:11.967
Duration
0:01:36.620
Note, WebLog generation is not included in the time.

CASA logs for stage 6