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 7.3136e-04 Jy/beam
minimum 1.5251e-04 Jy/beam
mean 2.3154e-04 Jy/beam
median 1.8205e-04 Jy/beam
sigma 1.0234e-04 Jy/beam
MAD rms 1.8353e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J100207_063000.10.2048.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.J100207+063000_P27878v1_2019_02_04T17_08_47.972/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J100207+063000_P27878v1_2019_02_04T17_08_47.972/working
Start time
2019-02-06 01:13:01.072
End
2019-02-06 01:15:17.015
Duration
0:02:15.943
Note, WebLog generation is not included in the time.

CASA logs for stage 6