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 3.6498e-03 Jy/beam
minimum 1.0711e-04 Jy/beam
mean 2.0916e-04 Jy/beam
median 1.5630e-04 Jy/beam
sigma 1.1977e-04 Jy/beam
MAD rms 4.9187e-05 Jy/beam

RMS images

TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms

Pilot.ql.Cygnus_e2.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_e2.J202431+373000_P33751v1_2019_02_11T18_02_36.289/working/TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e2.J202431+373000_P33751v1_2019_02_11T18_02_36.289/working
Start time
2019-02-18 12:29:09.644
End
2019-02-18 12:30:08.219
Duration
0:00:58.575
Note, WebLog generation is not included in the time.

CASA logs for stage 6