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 5.3918e-04 Jy/beam
minimum 9.8164e-05 Jy/beam
mean 1.5823e-04 Jy/beam
median 1.2013e-04 Jy/beam
sigma 7.7712e-05 Jy/beam
MAD rms 1.2306e-05 Jy/beam

RMS images

VLASS1.1.sb34396276.eb34742211.58081.44143899306_split.ms

VLASS1.1.ql.T17t17.J124238_273000.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T17t17.J124238+273000_P5142v2_2017_11_24T00_36_35.971/working/VLASS1.1.sb34396276.eb34742211.58081.44143899306_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T17t17.J124238+273000_P5142v2_2017_11_24T00_36_35.971/working
Start time
2021-02-07 05:09:01.620
End
2021-02-07 05:10:25.266
Duration
0:01:23.646
Note, WebLog generation is not included in the time.

CASA logs for stage 6