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 9.4974e-04 Jy/beam
minimum 1.5017e-04 Jy/beam
mean 3.2693e-04 Jy/beam
median 3.2065e-04 Jy/beam
sigma 1.3738e-04 Jy/beam
MAD rms 1.8185e-04 Jy/beam

RMS images

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

VLASS2.1.ql.T13t16.J101816_103000.10.2048.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_T13t16.J101816+103000_P62018v1_2020_07_18T15_55_25.554/working/VLASS2.1.sb38505794.eb38515224.59048.69954878472_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T13t16.J101816+103000_P62018v1_2020_07_18T15_55_25.554/working
Start time
2020-09-05 12:33:45.702
End
2020-09-05 12:35:13.213
Duration
0:01:27.511
Note, WebLog generation is not included in the time.

CASA logs for stage 6