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 8.0130e-04 Jy/beam
minimum 1.5110e-04 Jy/beam
mean 2.4215e-04 Jy/beam
median 1.9951e-04 Jy/beam
sigma 1.0237e-04 Jy/beam
MAD rms 2.9101e-05 Jy/beam

RMS images

VLASS2.1.sb38505794.eb38515224.59048.69954878472_split.ms

VLASS2.1.ql.T13t12.J073007_093000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T13t12.J073007+093000_P61926v1_2020_07_18T16_55_51.230/working/VLASS2.1.sb38505794.eb38515224.59048.69954878472_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T13t12.J073007+093000_P61926v1_2020_07_18T16_55_51.230/working
Start time
2020-09-18 03:13:06.329
End
2020-09-18 03:14:45.323
Duration
0:01:38.993
Note, WebLog generation is not included in the time.

CASA logs for stage 6