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 8.3456e-04 Jy/beam
minimum 1.2534e-04 Jy/beam
mean 2.3317e-04 Jy/beam
median 1.7787e-04 Jy/beam
sigma 1.1674e-04 Jy/beam
MAD rms 4.5182e-05 Jy/beam

RMS images

TSKY0001.sb32431120.eb32481709.57596.1060375_split.ms

Pilot.ql.SgrA_e1.J180158_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_e1.J180158-303000_P29812v1_2019_02_07T16_37_28.312/working/TSKY0001.sb32431120.eb32481709.57596.1060375_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e1.J180158-303000_P29812v1_2019_02_07T16_37_28.312/working
Start time
2019-02-09 01:17:53.183
End
2019-02-09 01:20:03.643
Duration
0:02:10.460
Note, WebLog generation is not included in the time.

CASA logs for stage 6