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 6.9415e-04 Jy/beam
minimum 1.3344e-04 Jy/beam
mean 2.1689e-04 Jy/beam
median 1.6859e-04 Jy/beam
sigma 9.8916e-05 Jy/beam
MAD rms 1.9392e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_1.J220202_054235.10.2048.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_SGC2A_1.J220202+054235_P30074v1_2019_02_09T00_19_46.269/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_1.J220202+054235_P30074v1_2019_02_09T00_19_46.269/working
Start time
2019-02-10 10:55:35.795
End
2019-02-10 10:57:27.968
Duration
0:01:52.173
Note, WebLog generation is not included in the time.

CASA logs for stage 6