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 5.9811e-04 Jy/beam
minimum 1.1183e-04 Jy/beam
mean 1.8027e-04 Jy/beam
median 1.3678e-04 Jy/beam
sigma 8.4621e-05 Jy/beam
MAD rms 1.8562e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J221746_583000.10.2048.v4.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J221746+583000_P33077v4_2019_03_05T22_20_41.434/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J221746+583000_P33077v4_2019_03_05T22_20_41.434/working
Start time
2019-03-07 00:13:41.593
End
2019-03-07 00:15:11.242
Duration
0:01:29.650
Note, WebLog generation is not included in the time.

CASA logs for stage 6