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 6.0520e-04 Jy/beam
minimum 1.0401e-04 Jy/beam
mean 1.6968e-04 Jy/beam
median 1.2871e-04 Jy/beam
sigma 8.1447e-05 Jy/beam
MAD rms 1.7872e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms

Pilot.ql.Cepheus_e2.J221746_583000.10.2048.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_Cepheus_e2.J221746+583000_P32993v1_2019_01_15T17_34_20.268/working/TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e2.J221746+583000_P32993v1_2019_01_15T17_34_20.268/working
Start time
2019-01-16 15:05:53.540
End
2019-01-16 15:07:12.697
Duration
0:01:19.157
Note, WebLog generation is not included in the time.

CASA logs for stage 6