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 2.1518e-03 Jy/beam
minimum 1.2781e-04 Jy/beam
mean 2.0724e-04 Jy/beam
median 1.5963e-04 Jy/beam
sigma 1.0630e-04 Jy/beam
MAD rms 1.7252e-05 Jy/beam

RMS images

VLASS1.2.sb36461910.eb36513329.58566.766115624996_split.ms

VLASS1.2.ql.T15t05.J030616_173000.10.2048.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_T15t05.J030616+173000_P37145v1_2019_04_01T22_41_40.409/working/VLASS1.2.sb36461910.eb36513329.58566.766115624996_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t05.J030616+173000_P37145v1_2019_04_01T22_41_40.409/working
Start time
2019-04-04 02:10:22.111
End
2019-04-04 02:12:26.559
Duration
0:02:04.448
Note, WebLog generation is not included in the time.

CASA logs for stage 6