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 2.2291e-03 Jy/beam
minimum 1.3423e-04 Jy/beam
mean 2.6366e-04 Jy/beam
median 1.9085e-04 Jy/beam
sigma 1.5843e-04 Jy/beam
MAD rms 4.5590e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J173903_313000.10.2048.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.J173903-313000_P33259v1_2019_01_23T16_39_48.039/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J173903-313000_P33259v1_2019_01_23T16_39_48.039/working
Start time
2019-01-28 22:43:35.224
End
2019-01-28 22:44:42.484
Duration
0:01:07.260
Note, WebLog generation is not included in the time.

CASA logs for stage 6