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 6.8927e-04 Jy/beam
minimum 1.1908e-04 Jy/beam
mean 1.8763e-04 Jy/beam
median 1.4458e-04 Jy/beam
sigma 9.0420e-05 Jy/beam
MAD rms 1.6096e-05 Jy/beam

RMS images

VLASS1.2.sb36769900.eb36829520.58666.363394201384_split.ms

VLASS1.1.ql.T03t36.J234509_293000.10.2048.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_T03t36.J234509-293000_P55462v1_2019_07_12T18_10_39.361/working/VLASS1.2.sb36769900.eb36829520.58666.363394201384_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T03t36.J234509-293000_P55462v1_2019_07_12T18_10_39.361/working
Start time
2019-07-18 01:43:05.353
End
2019-07-18 01:45:26.364
Duration
0:02:21.012
Note, WebLog generation is not included in the time.

CASA logs for stage 6