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 8.8022e-04 Jy/beam
minimum 1.1616e-04 Jy/beam
mean 1.8351e-04 Jy/beam
median 1.3839e-04 Jy/beam
sigma 9.7158e-05 Jy/beam
MAD rms 1.2714e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t05.J031609_303000.10.2048.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_T18t05.J031609+303000_P37646v1_2019_04_02T21_48_41.333/working/VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t05.J031609+303000_P37646v1_2019_04_02T21_48_41.333/working
Start time
2019-04-04 22:34:06.996
End
2019-04-04 22:36:19.473
Duration
0:02:12.477
Note, WebLog generation is not included in the time.

CASA logs for stage 6