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 7.6367e-04 Jy/beam
minimum 1.4908e-04 Jy/beam
mean 2.4152e-04 Jy/beam
median 1.8565e-04 Jy/beam
sigma 1.1293e-04 Jy/beam
MAD rms 2.6696e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101804_053000.10.2048.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.J101804+053000_P27872v1_2019_02_04T17_08_25.937/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101804+053000_P27872v1_2019_02_04T17_08_25.937/working
Start time
2019-02-05 16:48:28.768
End
2019-02-05 16:50:18.471
Duration
0:01:49.703
Note, WebLog generation is not included in the time.

CASA logs for stage 6