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 1.1606e-03 Jy/beam
minimum 1.1432e-04 Jy/beam
mean 1.9404e-04 Jy/beam
median 1.3976e-04 Jy/beam
sigma 1.0547e-04 Jy/beam
MAD rms 1.9226e-05 Jy/beam

RMS images

VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms

VLASS1.2.ql.T18t10.J070051_283000.10.2048.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_T18t10.J070051+283000_P41882v1_2019_05_20T21_06_04.791/working/VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t10.J070051+283000_P41882v1_2019_05_20T21_06_04.791/working
Start time
2019-05-23 04:56:32.263
End
2019-05-23 04:57:50.514
Duration
0:01:18.251
Note, WebLog generation is not included in the time.

CASA logs for stage 6