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 2.2828e-03 Jy/beam
minimum 1.3533e-04 Jy/beam
mean 2.4864e-04 Jy/beam
median 1.8211e-04 Jy/beam
sigma 1.4105e-04 Jy/beam
MAD rms 3.5879e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J175226_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_e2.J175226-293000_P33197v1_2019_02_04T16_26_21.349/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J175226-293000_P33197v1_2019_02_04T16_26_21.349/working
Start time
2019-02-05 13:21:20.317
End
2019-02-05 13:22:30.937
Duration
0:01:10.620
Note, WebLog generation is not included in the time.

CASA logs for stage 6