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 2.2641e-03 Jy/beam
minimum 1.2717e-04 Jy/beam
mean 2.1032e-04 Jy/beam
median 1.5744e-04 Jy/beam
sigma 1.1062e-04 Jy/beam
MAD rms 2.3124e-05 Jy/beam

RMS images

TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms

Pilot.ql.SGC2C_0.J231011_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_SGC2C_0.J231011+084236_P29525v1_2019_02_06T00_51_12.286/working/TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2C_0.J231011+084236_P29525v1_2019_02_06T00_51_12.286/working
Start time
2019-02-07 19:51:41.067
End
2019-02-07 19:53:15.930
Duration
0:01:34.863
Note, WebLog generation is not included in the time.

CASA logs for stage 6