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 6.2840e-04 Jy/beam
minimum 1.1888e-04 Jy/beam
mean 2.2368e-04 Jy/beam
median 1.8614e-04 Jy/beam
sigma 9.8486e-05 Jy/beam
MAD rms 5.8900e-05 Jy/beam

RMS images

VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms

VLASS1.2.ql.T15t20.J145839_193000.10.2048.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_T15t20.J145839+193000_P39179v1_2019_10_22T20_58_46.178/working/VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t20.J145839+193000_P39179v1_2019_10_22T20_58_46.178/working
Start time
2019-10-23 13:10:57.293
End
2019-10-23 13:11:48.069
Duration
0:00:50.776
Note, WebLog generation is not included in the time.

CASA logs for stage 6