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 6.4972e-04 Jy/beam
minimum 1.1367e-04 Jy/beam
mean 1.9158e-04 Jy/beam
median 1.4701e-04 Jy/beam
sigma 9.3754e-05 Jy/beam
MAD rms 2.0499e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J204433_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.J204433+373000_P33672v1_2019_02_07T15_31_19.395/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J204433+373000_P33672v1_2019_02_07T15_31_19.395/working
Start time
2019-02-08 21:28:02.040
End
2019-02-08 21:29:45.938
Duration
0:01:43.898
Note, WebLog generation is not included in the time.

CASA logs for stage 6