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 1.1929e-03 Jy/beam
minimum 1.2325e-04 Jy/beam
mean 1.9468e-04 Jy/beam
median 1.5258e-04 Jy/beam
sigma 8.8885e-05 Jy/beam
MAD rms 1.4966e-05 Jy/beam

RMS images

TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms

Pilot.ql.SGC1D_1.J022201_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.J022201+024235_P33849v1_2019_02_09T01_05_03.036/working/TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1D_1.J022201+024235_P33849v1_2019_02_09T01_05_03.036/working
Start time
2019-02-11 07:29:56.797
End
2019-02-11 07:31:43.775
Duration
0:01:46.978
Note, WebLog generation is not included in the time.

CASA logs for stage 6