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 5.5723e-04 Jy/beam
minimum 1.1073e-04 Jy/beam
mean 1.7254e-04 Jy/beam
median 1.3068e-04 Jy/beam
sigma 8.3673e-05 Jy/beam
MAD rms 1.2186e-05 Jy/beam

RMS images

VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms

VLASS1.2.ql.T17t30.J220019_243000.10.2048.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_T17t30.J220019+243000_P48928v1_2019_05_23T23_43_51.971/working/VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t30.J220019+243000_P48928v1_2019_05_23T23_43_51.971/working
Start time
2019-05-25 19:21:03.436
End
2019-05-25 19:23:12.861
Duration
0:02:09.425
Note, WebLog generation is not included in the time.

CASA logs for stage 6