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 5.8297e-03 Jy/beam
minimum 1.1990e-04 Jy/beam
mean 2.5718e-04 Jy/beam
median 1.8323e-04 Jy/beam
sigma 1.7176e-04 Jy/beam
MAD rms 6.0189e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J202431_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.J202431+373000_P33668v1_2019_03_01T23_42_47.047/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J202431+373000_P33668v1_2019_03_01T23_42_47.047/working
Start time
2019-03-07 07:45:16.543
End
2019-03-07 07:46:22.227
Duration
0:01:05.684
Note, WebLog generation is not included in the time.

CASA logs for stage 6