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 7.5017e-04 Jy/beam
minimum 1.1894e-04 Jy/beam
mean 2.1998e-04 Jy/beam
median 1.6121e-04 Jy/beam
sigma 1.1693e-04 Jy/beam
MAD rms 3.2871e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J180751_263000.10.2048.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.J180751-263000_P33319v1_2019_01_18T00_17_03.630/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J180751-263000_P33319v1_2019_01_18T00_17_03.630/working
Start time
2019-01-19 00:15:28.005
End
2019-01-19 00:16:57.858
Duration
0:01:29.853
Note, WebLog generation is not included in the time.

CASA logs for stage 6