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 2.9135e-03 Jy/beam
minimum 1.1345e-04 Jy/beam
mean 1.9854e-04 Jy/beam
median 1.5154e-04 Jy/beam
sigma 1.1329e-04 Jy/beam
MAD rms 2.8614e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J203529_403000.10.2048.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.J203529+403000_P33703v1_2019_02_07T16_07_53.313/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203529+403000_P33703v1_2019_02_07T16_07_53.313/working
Start time
2019-02-11 02:45:44.316
End
2019-02-11 02:47:33.073
Duration
0:01:48.757
Note, WebLog generation is not included in the time.

CASA logs for stage 6