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 1.5615e-03 Jy/beam
minimum 1.1584e-04 Jy/beam
mean 2.0394e-04 Jy/beam
median 1.4835e-04 Jy/beam
sigma 1.1609e-04 Jy/beam
MAD rms 2.5593e-05 Jy/beam

RMS images

VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms

VLASS1.2.ql.T18t01.J000659_313000.10.2048.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_T18t01.J000659+313000_P37614v1_2019_04_05T18_01_43.511/working/VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t01.J000659+313000_P37614v1_2019_04_05T18_01_43.511/working
Start time
2019-04-07 14:04:54.641
End
2019-04-07 14:05:57.601
Duration
0:01:02.960
Note, WebLog generation is not included in the time.

CASA logs for stage 6