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 6.8019e-04 Jy/beam
minimum 1.1531e-04 Jy/beam
mean 1.8815e-04 Jy/beam
median 1.3940e-04 Jy/beam
sigma 1.0044e-04 Jy/beam
MAD rms 1.3888e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t01.J001619_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.J001619+313000_P37616v1_2019_04_02T21_44_45.187/working/VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t01.J001619+313000_P37616v1_2019_04_02T21_44_45.187/working
Start time
2019-04-04 05:26:03.911
End
2019-04-04 05:27:44.292
Duration
0:01:40.381
Note, WebLog generation is not included in the time.

CASA logs for stage 6