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 2.2692e-03 Jy/beam
minimum 1.1805e-04 Jy/beam
mean 2.1968e-04 Jy/beam
median 1.6752e-04 Jy/beam
sigma 1.1829e-04 Jy/beam
MAD rms 4.2420e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J203551_413000.10.2048.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.J203551+413000_P33713v1_2019_02_11T18_51_32.889/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J203551+413000_P33713v1_2019_02_11T18_51_32.889/working
Start time
2019-02-13 06:13:17.811
End
2019-02-13 06:14:28.025
Duration
0:01:10.214
Note, WebLog generation is not included in the time.

CASA logs for stage 6