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 5.8482e-04 Jy/beam
minimum 1.1131e-04 Jy/beam
mean 1.8540e-04 Jy/beam
median 1.4512e-04 Jy/beam
sigma 8.4095e-05 Jy/beam
MAD rms 2.4816e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J014200_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_SGC1E_0.J014200+014235_P29877v1_2019_02_07T16_52_40.075/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J014200+014235_P29877v1_2019_02_07T16_52_40.075/working
Start time
2019-02-08 23:11:32.936
End
2019-02-08 23:13:18.891
Duration
0:01:45.955
Note, WebLog generation is not included in the time.

CASA logs for stage 6