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 7.8808e-04 Jy/beam
minimum 1.2713e-04 Jy/beam
mean 2.1768e-04 Jy/beam
median 1.6221e-04 Jy/beam
sigma 1.1527e-04 Jy/beam
MAD rms 2.0576e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J172501_303000.10.2048.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_SgrA_e3.J172501-303000_P33266v1_2019_01_18T15_38_20.763/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J172501-303000_P33266v1_2019_01_18T15_38_20.763/working
Start time
2019-01-19 10:09:57.345
End
2019-01-19 10:11:21.242
Duration
0:01:23.897
Note, WebLog generation is not included in the time.

CASA logs for stage 6