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 6.6182e-04 Jy/beam
minimum 1.3225e-04 Jy/beam
mean 2.0529e-04 Jy/beam
median 1.6049e-04 Jy/beam
sigma 9.1700e-05 Jy/beam
MAD rms 1.5475e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_1.J220606_074236.10.2048.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.J220606+074236_P30095v1_2019_02_09T00_20_20.726/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_1.J220606+074236_P30095v1_2019_02_09T00_20_20.726/working
Start time
2019-02-11 03:33:16.593
End
2019-02-11 03:35:38.860
Duration
0:02:22.267
Note, WebLog generation is not included in the time.

CASA logs for stage 6