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 1.5034e-03 Jy/beam
minimum 1.1019e-04 Jy/beam
mean 1.9186e-04 Jy/beam
median 1.4713e-04 Jy/beam
sigma 9.7673e-05 Jy/beam
MAD rms 3.2920e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J204733_433000.10.2048.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.J204733+433000_P33735v1_2019_02_11T23_20_42.179/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J204733+433000_P33735v1_2019_02_11T23_20_42.179/working
Start time
2019-02-13 05:48:22.713
End
2019-02-13 05:49:43.613
Duration
0:01:20.900
Note, WebLog generation is not included in the time.

CASA logs for stage 6