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 1.2297e-03 Jy/beam
minimum 1.3124e-04 Jy/beam
mean 2.3565e-04 Jy/beam
median 1.7097e-04 Jy/beam
sigma 1.2860e-04 Jy/beam
MAD rms 2.9814e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J175721_303000.10.2048.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.J175721-303000_P33273v1_2019_01_23T16_30_54.294/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J175721-303000_P33273v1_2019_01_23T16_30_54.294/working
Start time
2019-01-26 16:19:07.385
End
2019-01-26 16:20:09.578
Duration
0:01:02.194
Note, WebLog generation is not included in the time.

CASA logs for stage 6