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 6.1000e-04 Jy/beam
minimum 1.1922e-04 Jy/beam
mean 1.8804e-04 Jy/beam
median 1.4617e-04 Jy/beam
sigma 8.8636e-05 Jy/beam
MAD rms 1.4048e-05 Jy/beam

RMS images

TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms

Pilot.ql.SGC1A_0.J205000_024235.10.2048.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_SGC1A_0.J205000+024235_P29020v1_2019_01_31T22_55_21.138/working/TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1A_0.J205000+024235_P29020v1_2019_01_31T22_55_21.138/working
Start time
2019-02-02 13:49:54.233
End
2019-02-02 13:52:21.157
Duration
0:02:26.924
Note, WebLog generation is not included in the time.

CASA logs for stage 6