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 1.5612e-03 Jy/beam
minimum 1.1931e-04 Jy/beam
mean 2.2096e-04 Jy/beam
median 1.6981e-04 Jy/beam
sigma 1.1854e-04 Jy/beam
MAD rms 4.6546e-05 Jy/beam

RMS images

TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms

Pilot.ql.SGC2B_0.J213004_054235.10.2048.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.J213004+054235_P29328v1_2019_02_12T21_04_09.261/working/TSKY0001.sb32476325.eb32479241.57593.34503652778_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2B_0.J213004+054235_P29328v1_2019_02_12T21_04_09.261/working
Start time
2019-02-15 13:29:54.293
End
2019-02-15 13:31:11.264
Duration
0:01:16.971
Note, WebLog generation is not included in the time.

CASA logs for stage 6