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 8.5297e-04 Jy/beam
minimum 1.3601e-04 Jy/beam
mean 2.0941e-04 Jy/beam
median 1.6268e-04 Jy/beam
sigma 9.2243e-05 Jy/beam
MAD rms 1.6732e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_0.J210248_124236.10.2048.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.J210248+124236_P30776v1_2019_03_06T17_26_47.934/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_0.J210248+124236_P30776v1_2019_03_06T17_26_47.934/working
Start time
2019-03-07 22:57:15.208
End
2019-03-07 22:58:47.168
Duration
0:01:31.961
Note, WebLog generation is not included in the time.

CASA logs for stage 6