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 5.9426e-04 Jy/beam
minimum 1.1975e-04 Jy/beam
mean 1.8466e-04 Jy/beam
median 1.4620e-04 Jy/beam
sigma 7.7918e-05 Jy/beam
MAD rms 1.6515e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J224349_623000.10.2048.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.J224349+623000_P33125v1_2019_03_06T00_14_01.242/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J224349+623000_P33125v1_2019_03_06T00_14_01.242/working
Start time
2019-03-08 06:00:34.272
End
2019-03-08 06:02:40.678
Duration
0:02:06.406
Note, WebLog generation is not included in the time.

CASA logs for stage 6