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 6.4113e-04 Jy/beam
minimum 1.1451e-04 Jy/beam
mean 2.0261e-04 Jy/beam
median 1.7262e-04 Jy/beam
sigma 8.7378e-05 Jy/beam
MAD rms 5.1207e-05 Jy/beam

RMS images

VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms

VLASS1.2.ql.T20t14.J102630_373000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t14.J102630+373000_P48471v1_2019_05_03T23_51_36.297/working/VLASS1.2.sb36617763.eb36631658.58606.046132268515_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t14.J102630+373000_P48471v1_2019_05_03T23_51_36.297/working
Start time
2020-01-03 06:39:33.519
End
2020-01-03 06:40:59.351
Duration
0:01:25.832
Note, WebLog generation is not included in the time.

CASA logs for stage 6