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 6.4965e-04 Jy/beam
minimum 1.2292e-04 Jy/beam
mean 1.9149e-04 Jy/beam
median 1.4826e-04 Jy/beam
sigma 8.8358e-05 Jy/beam
MAD rms 1.5499e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T23t05.J042800_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.J042800+503000_P35397v1_2019_03_11T21_34_02.368/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t05.J042800+503000_P35397v1_2019_03_11T21_34_02.368/working
Start time
2019-03-13 11:02:41.791
End
2019-03-13 11:04:37.202
Duration
0:01:55.410
Note, WebLog generation is not included in the time.

CASA logs for stage 6