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 7.0563e-04 Jy/beam
minimum 1.3856e-04 Jy/beam
mean 2.1382e-04 Jy/beam
median 1.6711e-04 Jy/beam
sigma 9.2712e-05 Jy/beam
MAD rms 1.8144e-05 Jy/beam

RMS images

TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms

Pilot.ql.SGC2B_0.J213816_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_0.J213816+084236_P29360v1_2019_02_05T17_54_56.326/working/TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2B_0.J213816+084236_P29360v1_2019_02_05T17_54_56.326/working
Start time
2019-02-07 03:11:09.020
End
2019-02-07 03:13:10.683
Duration
0:02:01.664
Note, WebLog generation is not included in the time.

CASA logs for stage 6