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 1.6954e-03 Jy/beam
minimum 1.2831e-04 Jy/beam
mean 2.3269e-04 Jy/beam
median 1.7361e-04 Jy/beam
sigma 1.2633e-04 Jy/beam
MAD rms 3.4232e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J173853_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_e2.J173853-303000_P33184v1_2019_02_01T22_15_06.153/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J173853-303000_P33184v1_2019_02_01T22_15_06.153/working
Start time
2019-02-03 05:41:31.358
End
2019-02-03 05:42:55.761
Duration
0:01:24.403
Note, WebLog generation is not included in the time.

CASA logs for stage 6