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 6.1563e-04 Jy/beam
minimum 1.1527e-04 Jy/beam
mean 1.9374e-04 Jy/beam
median 1.5643e-04 Jy/beam
sigma 8.7485e-05 Jy/beam
MAD rms 3.7147e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J221815_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.J221815+623000_P33122v1_2019_03_13T21_41_31.896/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J221815+623000_P33122v1_2019_03_13T21_41_31.896/working
Start time
2019-03-15 15:26:52.613
End
2019-03-15 15:28:40.696
Duration
0:01:48.083
Note, WebLog generation is not included in the time.

CASA logs for stage 6