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 1.6132e-03 Jy/beam
minimum 3.5776e-04 Jy/beam
mean 5.9499e-04 Jy/beam
median 4.9250e-04 Jy/beam
sigma 2.2626e-04 Jy/beam
MAD rms 1.3245e-04 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101800_013000.10.2048.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_COSMOS_e1.J101800+013000_P27832v1_2019_02_04T17_05_59.076/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101800+013000_P27832v1_2019_02_04T17_05_59.076/working
Start time
2019-02-07 06:31:44.699
End
2019-02-07 06:33:08.661
Duration
0:01:23.961
Note, WebLog generation is not included in the time.

CASA logs for stage 6