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 7.3867e-04 Jy/beam
minimum 1.3278e-04 Jy/beam
mean 2.3276e-04 Jy/beam
median 1.8711e-04 Jy/beam
sigma 1.0840e-04 Jy/beam
MAD rms 5.3611e-05 Jy/beam

RMS images

TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms

Pilot.ql.SGC1D_0.J000200_014235.10.2048.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_SGC1D_0.J000200+014235_P33874v1_2019_02_09T01_05_59.329/working/TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1D_0.J000200+014235_P33874v1_2019_02_09T01_05_59.329/working
Start time
2019-02-10 23:58:09.910
End
2019-02-10 23:59:55.230
Duration
0:01:45.320
Note, WebLog generation is not included in the time.

CASA logs for stage 6