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 6.0880e-04 Jy/beam
minimum 1.1511e-04 Jy/beam
mean 1.8211e-04 Jy/beam
median 1.4005e-04 Jy/beam
sigma 8.8231e-05 Jy/beam
MAD rms 1.6836e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_0.J012602_044235.10.2048.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.J012602+044235_P29903v1_2019_02_07T17_51_56.511/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_0.J012602+044235_P29903v1_2019_02_07T17_51_56.511/working
Start time
2019-02-09 11:40:44.696
End
2019-02-09 11:43:04.226
Duration
0:02:19.530
Note, WebLog generation is not included in the time.

CASA logs for stage 6