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 6.3085e-04 Jy/beam
minimum 1.1937e-04 Jy/beam
mean 1.9069e-04 Jy/beam
median 1.4826e-04 Jy/beam
sigma 8.9016e-05 Jy/beam
MAD rms 1.4099e-05 Jy/beam

RMS images

VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms

VLASS1.2.ql.T15t26.J191229_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_T15t26.J191229+193000_P39039v1_2019_04_04T17_32_31.731/working/VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t26.J191229+193000_P39039v1_2019_04_04T17_32_31.731/working
Start time
2019-04-07 16:24:42.231
End
2019-04-07 16:26:29.099
Duration
0:01:46.868
Note, WebLog generation is not included in the time.

CASA logs for stage 6