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 8.1410e-04 Jy/beam
minimum 1.3709e-04 Jy/beam
mean 2.4167e-04 Jy/beam
median 1.8192e-04 Jy/beam
sigma 1.1862e-04 Jy/beam
MAD rms 3.8335e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J180828_293000.10.2048.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.J180828-293000_P33286v1_2019_01_18T00_16_09.055/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J180828-293000_P33286v1_2019_01_18T00_16_09.055/working
Start time
2019-01-18 20:26:31.828
End
2019-01-18 20:28:01.314
Duration
0:01:29.486
Note, WebLog generation is not included in the time.

CASA logs for stage 6