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 1.1417e-03 Jy/beam
minimum 1.2601e-04 Jy/beam
mean 1.9759e-04 Jy/beam
median 1.5212e-04 Jy/beam
sigma 9.8547e-05 Jy/beam
MAD rms 1.3809e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_0.J225646_104236.10.2048.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_0.J225646+104236_P30881v1_2019_01_22T20_34_09.283/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_0.J225646+104236_P30881v1_2019_01_22T20_34_09.283/working
Start time
2019-01-24 22:57:24.324
End
2019-01-24 22:59:24.288
Duration
0:01:59.964
Note, WebLog generation is not included in the time.

CASA logs for stage 6