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 6.6225e-04 Jy/beam
minimum 1.2431e-04 Jy/beam
mean 1.9903e-04 Jy/beam
median 1.5695e-04 Jy/beam
sigma 9.0576e-05 Jy/beam
MAD rms 1.8992e-05 Jy/beam

RMS images

TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms

Pilot.ql.SGC1D_1.J020200_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.J020200+024235_P33844v1_2019_02_09T01_04_54.907/working/TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1D_1.J020200+024235_P33844v1_2019_02_09T01_04_54.907/working
Start time
2019-02-11 09:42:59.401
End
2019-02-11 09:44:48.698
Duration
0:01:49.297
Note, WebLog generation is not included in the time.

CASA logs for stage 6