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 6.8721e-03 Jy/beam
minimum 1.1557e-04 Jy/beam
mean 2.0800e-04 Jy/beam
median 1.5790e-04 Jy/beam
sigma 1.1590e-04 Jy/beam
MAD rms 3.4753e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J202931_373000.10.2048.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_Cygnus_e3.J202931+373000_P33669v1_2019_02_19T16_30_12.228/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J202931+373000_P33669v1_2019_02_19T16_30_12.228/working
Start time
2019-03-01 14:27:03.822
End
2019-03-01 14:28:32.353
Duration
0:01:28.530
Note, WebLog generation is not included in the time.

CASA logs for stage 6