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 6.7183e-04 Jy/beam
minimum 1.1758e-04 Jy/beam
mean 1.8490e-04 Jy/beam
median 1.4872e-04 Jy/beam
sigma 7.8859e-05 Jy/beam
MAD rms 2.2292e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J222646_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.J222646+623000_P33123v1_2019_03_06T00_13_52.684/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J222646+623000_P33123v1_2019_03_06T00_13_52.684/working
Start time
2019-03-08 09:31:47.892
End
2019-03-08 09:33:43.380
Duration
0:01:55.488
Note, WebLog generation is not included in the time.

CASA logs for stage 6