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 8.1140e-04 Jy/beam
minimum 1.2517e-04 Jy/beam
mean 2.0991e-04 Jy/beam
median 1.5850e-04 Jy/beam
sigma 1.0436e-04 Jy/beam
MAD rms 2.0039e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J174234_253000.10.2048.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.J174234-253000_P33324v1_2019_01_18T00_17_11.564/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J174234-253000_P33324v1_2019_01_18T00_17_11.564/working
Start time
2019-01-19 08:41:07.572
End
2019-01-19 08:42:44.495
Duration
0:01:36.923
Note, WebLog generation is not included in the time.

CASA logs for stage 6