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 6.4811e-04 Jy/beam
minimum 1.2832e-04 Jy/beam
mean 2.0138e-04 Jy/beam
median 1.5830e-04 Jy/beam
sigma 9.1702e-05 Jy/beam
MAD rms 1.4346e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_0.J205429_104236.10.2048.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_SGC3A_0.J205429+104236_P30753v1_2019_03_06T17_24_05.906/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_0.J205429+104236_P30753v1_2019_03_06T17_24_05.906/working
Start time
2019-03-08 06:24:58.517
End
2019-03-08 06:26:41.196
Duration
0:01:42.679
Note, WebLog generation is not included in the time.

CASA logs for stage 6