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 1.2014e-03 Jy/beam
minimum 1.1884e-04 Jy/beam
mean 1.9621e-04 Jy/beam
median 1.4874e-04 Jy/beam
sigma 9.3688e-05 Jy/beam
MAD rms 2.4198e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J230737_613000.10.2048.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.J230737+613000_P33117v1_2019_03_11T16_12_49.851/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J230737+613000_P33117v1_2019_03_11T16_12_49.851/working
Start time
2019-03-12 10:12:07.648
End
2019-03-12 10:13:21.896
Duration
0:01:14.249
Note, WebLog generation is not included in the time.

CASA logs for stage 6