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 8.3825e-04 Jy/beam
minimum 1.2719e-04 Jy/beam
mean 2.1891e-04 Jy/beam
median 1.6588e-04 Jy/beam
sigma 1.0681e-04 Jy/beam
MAD rms 2.7749e-05 Jy/beam

RMS images

TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms

Pilot.ql.SGC1A_1.J215400_014235.10.2048.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_1.J215400+014235_P28966v1_2019_01_31T22_53_03.630/working/TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1A_1.J215400+014235_P28966v1_2019_01_31T22_53_03.630/working
Start time
2019-02-01 14:15:24.191
End
2019-02-01 14:16:34.369
Duration
0:01:10.177
Note, WebLog generation is not included in the time.

CASA logs for stage 6