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 9.9761e-04 Jy/beam
minimum 1.3136e-04 Jy/beam
mean 2.2080e-04 Jy/beam
median 1.6974e-04 Jy/beam
sigma 1.1161e-04 Jy/beam
MAD rms 2.3416e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J180223_313000.10.2048.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.J180223-313000_P33179v2_2019_03_15T19_01_21.647/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J180223-313000_P33179v2_2019_03_15T19_01_21.647/working
Start time
2019-03-17 01:14:23.226
End
2019-03-17 01:16:10.255
Duration
0:01:47.029
Note, WebLog generation is not included in the time.

CASA logs for stage 6