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 8.6831e-04 Jy/beam
minimum 1.2619e-04 Jy/beam
mean 2.2331e-04 Jy/beam
median 1.7435e-04 Jy/beam
sigma 1.0896e-04 Jy/beam
MAD rms 3.4695e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J175244_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_e2.J175244-303000_P33187v1_2019_01_30T23_49_54.106/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J175244-303000_P33187v1_2019_01_30T23_49_54.106/working
Start time
2019-02-01 06:26:46.402
End
2019-02-01 06:28:18.203
Duration
0:01:31.800
Note, WebLog generation is not included in the time.

CASA logs for stage 6