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 6.1667e-04 Jy/beam
minimum 1.3371e-04 Jy/beam
mean 2.1033e-04 Jy/beam
median 1.6944e-04 Jy/beam
sigma 8.4365e-05 Jy/beam
MAD rms 1.9942e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_1.J222413_114236.10.2048.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.J222413+114236_P30724v1_2019_03_06T17_21_54.306/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_1.J222413+114236_P30724v1_2019_03_06T17_21_54.306/working
Start time
2019-03-08 04:34:18.750
End
2019-03-08 04:36:12.651
Duration
0:01:53.901
Note, WebLog generation is not included in the time.

CASA logs for stage 6