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 1.3354e-02 Jy/beam
minimum 1.3474e-04 Jy/beam
mean 3.4599e-04 Jy/beam
median 1.9796e-04 Jy/beam
sigma 3.8482e-04 Jy/beam
MAD rms 6.1282e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J174306_283000.10.2048.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.J174306-283000_P33291v1_2019_01_22T23_17_34.618/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J174306-283000_P33291v1_2019_01_22T23_17_34.618/working
Start time
2019-01-29 00:03:33.535
End
2019-01-29 00:04:41.410
Duration
0:01:07.875
Note, WebLog generation is not included in the time.

CASA logs for stage 6