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 6.9780e-04 Jy/beam
minimum 1.2997e-04 Jy/beam
mean 2.0584e-04 Jy/beam
median 1.5779e-04 Jy/beam
sigma 1.0141e-04 Jy/beam
MAD rms 1.7063e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_0.J204216_094236.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_0.J204216+094236_P30739v2_2019_03_11T09_26_06.447/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_0.J204216+094236_P30739v2_2019_03_11T09_26_06.447/working
Start time
2019-03-12 12:37:45.454
End
2019-03-12 12:39:21.897
Duration
0:01:36.443
Note, WebLog generation is not included in the time.

CASA logs for stage 6