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 5.2017e-04 Jy/beam
minimum 1.0291e-04 Jy/beam
mean 1.6333e-04 Jy/beam
median 1.2430e-04 Jy/beam
sigma 7.7564e-05 Jy/beam
MAD rms 1.1600e-05 Jy/beam

RMS images

TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms

Pilot.ql.Cygnus_e2.J202554_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_e2.J202554+443000_P33824v1_2019_02_07T19_01_56.065/working/TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e2.J202554+443000_P33824v1_2019_02_07T19_01_56.065/working
Start time
2019-02-10 06:38:06.259
End
2019-02-10 06:40:03.492
Duration
0:01:57.233
Note, WebLog generation is not included in the time.

CASA logs for stage 6