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 1.3036e-03 Jy/beam
minimum 1.2102e-04 Jy/beam
mean 2.0432e-04 Jy/beam
median 1.5676e-04 Jy/beam
sigma 1.0719e-04 Jy/beam
MAD rms 1.8439e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J174255_273000.10.2048.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.J174255-273000_P33217v1_2019_01_31T02_52_22.755/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J174255-273000_P33217v1_2019_01_31T02_52_22.755/working
Start time
2019-02-02 01:17:29.130
End
2019-02-02 01:19:44.794
Duration
0:02:15.664
Note, WebLog generation is not included in the time.

CASA logs for stage 6