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 7.9928e-04 Jy/beam
minimum 1.4648e-04 Jy/beam
mean 2.3215e-04 Jy/beam
median 1.8141e-04 Jy/beam
sigma 1.0649e-04 Jy/beam
MAD rms 2.0815e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101404_043000.10.2048.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.J101404+043000_P27861v1_2019_02_04T17_07_28.646/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101404+043000_P27861v1_2019_02_04T17_07_28.646/working
Start time
2019-02-05 20:13:54.787
End
2019-02-05 20:15:57.992
Duration
0:02:03.205
Note, WebLog generation is not included in the time.

CASA logs for stage 6