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 6.9400e-04 Jy/beam
minimum 1.1838e-04 Jy/beam
mean 1.8939e-04 Jy/beam
median 1.4373e-04 Jy/beam
sigma 9.1824e-05 Jy/beam
MAD rms 1.4516e-05 Jy/beam

RMS images

VLASS1.2.sb36567355.eb36772922.58643.48209619213_split.ms

VLASS1.2.ql.T19t03.J021605_323000.10.2048.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_T19t03.J021605+323000_P45526v1_2019_06_16T18_56_42.369/working/VLASS1.2.sb36567355.eb36772922.58643.48209619213_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T19t03.J021605+323000_P45526v1_2019_06_16T18_56_42.369/working
Start time
2019-06-18 05:32:22.919
End
2019-06-18 05:34:09.258
Duration
0:01:46.339
Note, WebLog generation is not included in the time.

CASA logs for stage 6