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 1.0034e-03 Jy/beam
minimum 1.4565e-04 Jy/beam
mean 2.4692e-04 Jy/beam
median 1.8810e-04 Jy/beam
sigma 1.2210e-04 Jy/beam
MAD rms 3.3216e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J094200_033000.10.2048.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.J094200+033000_P27843v1_2019_02_04T17_06_30.060/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J094200+033000_P27843v1_2019_02_04T17_06_30.060/working
Start time
2019-02-05 19:45:49.629
End
2019-02-05 19:47:37.156
Duration
0:01:47.527
Note, WebLog generation is not included in the time.

CASA logs for stage 6