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 1.6548e-03 Jy/beam
minimum 3.6431e-04 Jy/beam
mean 5.8892e-04 Jy/beam
median 4.8798e-04 Jy/beam
sigma 2.1330e-04 Jy/beam
MAD rms 1.1614e-04 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101400_013000.10.2048.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.J101400+013000_P27831v1_2019_02_04T17_05_56.226/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101400+013000_P27831v1_2019_02_04T17_05_56.226/working
Start time
2019-02-07 20:19:43.133
End
2019-02-07 20:21:43.359
Duration
0:02:00.226
Note, WebLog generation is not included in the time.

CASA logs for stage 6