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 6.1426e-04 Jy/beam
minimum 1.2303e-04 Jy/beam
mean 1.9876e-04 Jy/beam
median 1.4906e-04 Jy/beam
sigma 9.3736e-05 Jy/beam
MAD rms 1.8248e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J015011_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_0.J015011+084236_P30443v1_2019_02_09T00_48_45.703/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J015011+084236_P30443v1_2019_02_09T00_48_45.703/working
Start time
2019-02-14 03:18:31.702
End
2019-02-14 03:20:04.697
Duration
0:01:32.995
Note, WebLog generation is not included in the time.

CASA logs for stage 6