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 5.8679e-04 Jy/beam
minimum 1.0794e-04 Jy/beam
mean 1.7514e-04 Jy/beam
median 1.3881e-04 Jy/beam
sigma 8.0673e-05 Jy/beam
MAD rms 2.1698e-05 Jy/beam

RMS images

TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms

Pilot.ql.Cygnus_e2.J201949_403000.10.2048.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_Cygnus_e2.J201949+403000_P33783v1_2019_02_07T18_26_08.352/working/TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e2.J201949+403000_P33783v1_2019_02_07T18_26_08.352/working
Start time
2019-02-10 19:06:28.165
End
2019-02-10 19:08:24.130
Duration
0:01:55.965
Note, WebLog generation is not included in the time.

CASA logs for stage 6