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 1.1780e-03 Jy/beam
minimum 1.0727e-04 Jy/beam
mean 1.7853e-04 Jy/beam
median 1.4053e-04 Jy/beam
sigma 8.3681e-05 Jy/beam
MAD rms 2.3092e-05 Jy/beam

RMS images

TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms

Pilot.ql.Cygnus_e2.J203016_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.J203016+403000_P33785v1_2019_02_07T18_26_12.580/working/TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e2.J203016+403000_P33785v1_2019_02_07T18_26_12.580/working
Start time
2019-02-11 18:32:45.317
End
2019-02-11 18:34:47.067
Duration
0:02:01.751
Note, WebLog generation is not included in the time.

CASA logs for stage 6