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 1.7642e-03 Jy/beam
minimum 1.0886e-04 Jy/beam
mean 1.8796e-04 Jy/beam
median 1.4718e-04 Jy/beam
sigma 9.6581e-05 Jy/beam
MAD rms 2.6372e-05 Jy/beam

RMS images

TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms

Pilot.ql.SGC2E_0.J011802_074236.10.2048.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.J011802+074236_P30425v1_2019_02_09T00_48_15.636/working/TSKY0001.sb32511750.eb32521454.57607.51894731482_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2E_0.J011802+074236_P30425v1_2019_02_09T00_48_15.636/working
Start time
2019-02-12 14:51:02.887
End
2019-02-12 14:52:55.708
Duration
0:01:52.821
Note, WebLog generation is not included in the time.

CASA logs for stage 6