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 6.5170e-04 Jy/beam
minimum 1.3062e-04 Jy/beam
mean 2.0908e-04 Jy/beam
median 1.6208e-04 Jy/beam
sigma 9.3827e-05 Jy/beam
MAD rms 2.3578e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_1.J223612_094236.10.2048.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_1.J223612+094236_P30705v1_2019_03_06T17_21_04.554/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_1.J223612+094236_P30705v1_2019_03_06T17_21_04.554/working
Start time
2019-03-07 19:07:11.284
End
2019-03-07 19:08:55.003
Duration
0:01:43.718
Note, WebLog generation is not included in the time.

CASA logs for stage 6