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 7.1527e-04 Jy/beam
minimum 1.2100e-04 Jy/beam
mean 1.8969e-04 Jy/beam
median 1.4709e-04 Jy/beam
sigma 8.7286e-05 Jy/beam
MAD rms 1.4176e-05 Jy/beam

RMS images

VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms

VLASS1.2.ql.T23t05.J044026_503000.10.2048.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_T23t05.J044026+503000_P35399v1_2019_03_13T21_33_47.065/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t05.J044026+503000_P35399v1_2019_03_13T21_33_47.065/working
Start time
2019-03-15 17:30:23.112
End
2019-03-15 17:32:38.177
Duration
0:02:15.064
Note, WebLog generation is not included in the time.

CASA logs for stage 6