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 5.2612e-04 Jy/beam
minimum 1.0409e-04 Jy/beam
mean 1.6861e-04 Jy/beam
median 1.2740e-04 Jy/beam
sigma 7.8984e-05 Jy/beam
MAD rms 1.7067e-05 Jy/beam

RMS images

TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms

Pilot.ql.Cygnus_e2.J210213_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_e2.J210213+423000_P33811v1_2019_02_07T18_44_29.571/working/TSKY0001.sb32432262.eb32479371.57594.17331140046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e2.J210213+423000_P33811v1_2019_02_07T18_44_29.571/working
Start time
2019-02-09 15:20:56.953
End
2019-02-09 15:22:37.359
Duration
0:01:40.406
Note, WebLog generation is not included in the time.

CASA logs for stage 6