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 5.7398e-04 Jy/beam
minimum 1.0819e-04 Jy/beam
mean 1.7321e-04 Jy/beam
median 1.3258e-04 Jy/beam
sigma 8.4509e-05 Jy/beam
MAD rms 1.4958e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J205915_443000.10.2048.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.J205915+443000_P33747v1_2019_02_07T17_04_25.354/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J205915+443000_P33747v1_2019_02_07T17_04_25.354/working
Start time
2019-02-09 10:38:39.696
End
2019-02-09 10:40:55.608
Duration
0:02:15.912
Note, WebLog generation is not included in the time.

CASA logs for stage 6