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 6.8846e-04 Jy/beam
minimum 1.0875e-04 Jy/beam
mean 1.7451e-04 Jy/beam
median 1.3400e-04 Jy/beam
sigma 8.2214e-05 Jy/beam
MAD rms 1.8353e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J221752_593000.10.2048.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.J221752+593000_P33089v1_2019_03_05T23_48_00.127/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J221752+593000_P33089v1_2019_03_05T23_48_00.127/working
Start time
2019-03-07 06:26:00.371
End
2019-03-07 06:27:53.315
Duration
0:01:52.944
Note, WebLog generation is not included in the time.

CASA logs for stage 6