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 6.5313e-04 Jy/beam
minimum 1.2915e-04 Jy/beam
mean 2.1071e-04 Jy/beam
median 1.6064e-04 Jy/beam
sigma 9.4301e-05 Jy/beam
MAD rms 2.2181e-05 Jy/beam

RMS images

VLASS2.1.sb38460547.eb38644333.59105.33538509259_split.ms

VLASS2.1.ql.T09t05.J031808_073000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T09t05.J031808-073000_P57885v1_2020_09_13T22_52_06.947/working/VLASS2.1.sb38460547.eb38644333.59105.33538509259_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T09t05.J031808-073000_P57885v1_2020_09_13T22_52_06.947/working
Start time
2020-10-02 15:31:43.668
End
2020-10-02 15:32:55.314
Duration
0:01:11.645
Note, WebLog generation is not included in the time.

CASA logs for stage 6