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 8.2532e-04 Jy/beam
minimum 1.2704e-04 Jy/beam
mean 2.2981e-04 Jy/beam
median 1.8051e-04 Jy/beam
sigma 1.0765e-04 Jy/beam
MAD rms 4.1104e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J180623_303000.10.2048.v2.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_e2.J180623-303000_P33190v2_2019_03_15T18_56_49.798/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J180623-303000_P33190v2_2019_03_15T18_56_49.798/working
Start time
2019-03-16 12:22:45.140
End
2019-03-16 12:24:11.777
Duration
0:01:26.637
Note, WebLog generation is not included in the time.

CASA logs for stage 6