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 6.1962e-04 Jy/beam
minimum 1.1045e-04 Jy/beam
mean 1.8004e-04 Jy/beam
median 1.3983e-04 Jy/beam
sigma 8.3653e-05 Jy/beam
MAD rms 1.4824e-05 Jy/beam

RMS images

TSKY0001.sb32503337.eb32660293.57632.412079305555_split.ms

Pilot.ql.CDFS_e3.J033813_243000.10.2048.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_CDFS_e3.J033813-243000_P33474v1_2019_01_31T14_57_44.823/working/TSKY0001.sb32503337.eb32660293.57632.412079305555_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_CDFS_e3.J033813-243000_P33474v1_2019_01_31T14_57_44.823/working
Start time
2019-02-02 08:34:42.902
End
2019-02-02 08:36:46.486
Duration
0:02:03.583
Note, WebLog generation is not included in the time.

CASA logs for stage 6