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 8.3651e-04 Jy/beam
minimum 1.2624e-04 Jy/beam
mean 2.0757e-04 Jy/beam
median 1.6302e-04 Jy/beam
sigma 9.8860e-05 Jy/beam
MAD rms 1.7301e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J175701_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.J175701-293000_P33198v1_2019_01_31T17_48_18.596/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J175701-293000_P33198v1_2019_01_31T17_48_18.596/working
Start time
2019-02-02 07:40:31.212
End
2019-02-02 07:42:33.312
Duration
0:02:02.101
Note, WebLog generation is not included in the time.

CASA logs for stage 6