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 6.4710e-04 Jy/beam
minimum 1.2876e-04 Jy/beam
mean 1.9626e-04 Jy/beam
median 1.5422e-04 Jy/beam
sigma 8.5890e-05 Jy/beam
MAD rms 1.4833e-05 Jy/beam

RMS images

TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms

Pilot.ql.SGC2B_0.J213812_074236.10.2048.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_0.J213812+074236_P29350v1_2019_02_05T17_53_52.467/working/TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2B_0.J213812+074236_P29350v1_2019_02_05T17_53_52.467/working
Start time
2019-02-07 09:10:49.330
End
2019-02-07 09:12:51.515
Duration
0:02:02.185
Note, WebLog generation is not included in the time.

CASA logs for stage 6