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 8.3237e-04 Jy/beam
minimum 1.1553e-04 Jy/beam
mean 2.0795e-04 Jy/beam
median 1.5485e-04 Jy/beam
sigma 1.0833e-04 Jy/beam
MAD rms 2.9043e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J204933_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.J204933+373000_P33673v1_2019_02_11T17_21_08.866/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J204933+373000_P33673v1_2019_02_11T17_21_08.866/working
Start time
2019-02-12 15:00:55.668
End
2019-02-12 15:02:11.543
Duration
0:01:15.875
Note, WebLog generation is not included in the time.

CASA logs for stage 6