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 1.2815e-03 Jy/beam
minimum 1.2071e-04 Jy/beam
mean 1.9484e-04 Jy/beam
median 1.5240e-04 Jy/beam
sigma 9.1064e-05 Jy/beam
MAD rms 1.6810e-05 Jy/beam

RMS images

TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms

Pilot.ql.SGC1D_1.J021801_024235.10.2048.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_1.J021801+024235_P33848v1_2019_02_09T01_05_01.415/working/TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1D_1.J021801+024235_P33848v1_2019_02_09T01_05_01.415/working
Start time
2019-02-11 12:45:24.896
End
2019-02-11 12:47:17.186
Duration
0:01:52.289
Note, WebLog generation is not included in the time.

CASA logs for stage 6