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 8.6124e-04 Jy/beam
minimum 1.5187e-04 Jy/beam
mean 2.5185e-04 Jy/beam
median 1.9994e-04 Jy/beam
sigma 1.0758e-04 Jy/beam
MAD rms 2.9491e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101000_003000.10.2048.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.J101000+003000_P27820v1_2019_02_04T17_05_29.179/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101000+003000_P27820v1_2019_02_04T17_05_29.179/working
Start time
2019-02-05 20:26:30.019
End
2019-02-05 20:28:25.311
Duration
0:01:55.292
Note, WebLog generation is not included in the time.

CASA logs for stage 6