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 2.4183e-03 Jy/beam
minimum 1.1088e-04 Jy/beam
mean 1.9958e-04 Jy/beam
median 1.5809e-04 Jy/beam
sigma 9.8714e-05 Jy/beam
MAD rms 4.0644e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J204136_423000.10.2048.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.J204136+423000_P33724v1_2019_02_19T17_04_33.615/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J204136+423000_P33724v1_2019_02_19T17_04_33.615/working
Start time
2019-03-03 20:56:31.592
End
2019-03-03 20:58:11.580
Duration
0:01:39.988
Note, WebLog generation is not included in the time.

CASA logs for stage 6