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 6.2279e-04 Jy/beam
minimum 1.1506e-04 Jy/beam
mean 1.8503e-04 Jy/beam
median 1.4217e-04 Jy/beam
sigma 8.6062e-05 Jy/beam
MAD rms 1.7288e-05 Jy/beam

RMS images

TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms

Pilot.ql.SGC2B_1.J231803_084236.10.2048.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_SGC2B_1.J231803+084236_P29315v1_2019_02_05T17_51_09.349/working/TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2B_1.J231803+084236_P29315v1_2019_02_05T17_51_09.349/working
Start time
2019-02-07 02:04:13.570
End
2019-02-07 02:06:13.133
Duration
0:01:59.563
Note, WebLog generation is not included in the time.

CASA logs for stage 6