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 6.6577e-04 Jy/beam
minimum 1.1225e-04 Jy/beam
mean 1.8836e-04 Jy/beam
median 1.4303e-04 Jy/beam
sigma 9.1044e-05 Jy/beam
MAD rms 2.2714e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J020018_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_SGC3C_1.J020018+124236_P30949v1_2019_01_22T17_27_03.769/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J020018+124236_P30949v1_2019_01_22T17_27_03.769/working
Start time
2019-01-23 22:49:23.417
End
2019-01-23 22:51:00.411
Duration
0:01:36.994
Note, WebLog generation is not included in the time.

CASA logs for stage 6