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 1.3349e-03 Jy/beam
minimum 1.2322e-04 Jy/beam
mean 2.1229e-04 Jy/beam
median 1.6520e-04 Jy/beam
sigma 1.0159e-04 Jy/beam
MAD rms 3.2291e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J180522_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.J180522-273000_P33222v1_2019_01_31T02_52_26.629/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J180522-273000_P33222v1_2019_01_31T02_52_26.629/working
Start time
2019-02-03 03:03:26.749
End
2019-02-03 03:05:06.210
Duration
0:01:39.461
Note, WebLog generation is not included in the time.

CASA logs for stage 6