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 8.2771e-04 Jy/beam
minimum 1.2284e-04 Jy/beam
mean 2.0431e-04 Jy/beam
median 1.5857e-04 Jy/beam
sigma 9.9758e-05 Jy/beam
MAD rms 2.0482e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J175641_283000.10.2048.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.J175641-283000_P33209v1_2019_01_31T02_49_07.059/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J175641-283000_P33209v1_2019_01_31T02_49_07.059/working
Start time
2019-02-01 15:05:47.033
End
2019-02-01 15:07:34.216
Duration
0:01:47.183
Note, WebLog generation is not included in the time.

CASA logs for stage 6