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 8.8142e-04 Jy/beam
minimum 1.3847e-04 Jy/beam
mean 2.4946e-04 Jy/beam
median 1.8441e-04 Jy/beam
sigma 1.3174e-04 Jy/beam
MAD rms 3.2220e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J174839_323000.10.2048.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_e2.J174839-323000_P33166v1_2019_01_30T23_17_58.267/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J174839-323000_P33166v1_2019_01_30T23_17_58.267/working
Start time
2019-01-31 17:41:29.609
End
2019-01-31 17:42:43.680
Duration
0:01:14.071
Note, WebLog generation is not included in the time.

CASA logs for stage 6