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 7.9977e-04 Jy/beam
minimum 1.3982e-04 Jy/beam
mean 2.2269e-04 Jy/beam
median 1.7099e-04 Jy/beam
sigma 1.0989e-04 Jy/beam
MAD rms 1.6564e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J100602_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.J100602+033000_P27849v1_2019_02_04T17_06_49.458/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J100602+033000_P27849v1_2019_02_04T17_06_49.458/working
Start time
2019-02-05 23:53:11.353
End
2019-02-05 23:55:23.544
Duration
0:02:12.191
Note, WebLog generation is not included in the time.

CASA logs for stage 6