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 5.5718e-04 Jy/beam
minimum 1.0827e-04 Jy/beam
mean 1.7940e-04 Jy/beam
median 1.3770e-04 Jy/beam
sigma 8.1575e-05 Jy/beam
MAD rms 2.2033e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J233351_653000.10.2048.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_e3.J233351+653000_P33160v1_2019_03_06T00_30_19.919/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J233351+653000_P33160v1_2019_03_06T00_30_19.919/working
Start time
2019-03-06 20:45:16.330
End
2019-03-06 20:46:50.005
Duration
0:01:33.676
Note, WebLog generation is not included in the time.

CASA logs for stage 6