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 6.5699e-04 Jy/beam
minimum 1.2126e-04 Jy/beam
mean 2.0615e-04 Jy/beam
median 1.7329e-04 Jy/beam
sigma 8.8473e-05 Jy/beam
MAD rms 4.8627e-05 Jy/beam

RMS images

VLASS1.2.sb36551200.eb36595645.58594.214120625_split.ms

VLASS1.2.ql.T11t20.J131801_033000.10.2048.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_T11t20.J131801+033000_P42274v1_2019_12_04T21_54_29.808/working/VLASS1.2.sb36551200.eb36595645.58594.214120625_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T11t20.J131801+033000_P42274v1_2019_12_04T21_54_29.808/working
Start time
2019-12-05 10:34:46.123
End
2019-12-05 10:35:55.957
Duration
0:01:09.833
Note, WebLog generation is not included in the time.

CASA logs for stage 6