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 1.5814e-03 Jy/beam
minimum 1.1498e-04 Jy/beam
mean 1.9758e-04 Jy/beam
median 1.5563e-04 Jy/beam
sigma 9.3645e-05 Jy/beam
MAD rms 2.9663e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J202503_403000.10.2048.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.J202503+403000_P33701v1_2019_02_07T16_07_49.720/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J202503+403000_P33701v1_2019_02_07T16_07_49.720/working
Start time
2019-02-11 06:28:07.180
End
2019-02-11 06:29:50.512
Duration
0:01:43.332
Note, WebLog generation is not included in the time.

CASA logs for stage 6