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 7.2414e-04 Jy/beam
minimum 1.1413e-04 Jy/beam
mean 1.8407e-04 Jy/beam
median 1.3943e-04 Jy/beam
sigma 9.6281e-05 Jy/beam
MAD rms 1.3563e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t01.J002509_293000.10.2048.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.J002509+293000_P37598v1_2019_04_02T21_42_39.217/working/VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t01.J002509+293000_P37598v1_2019_04_02T21_42_39.217/working
Start time
2019-04-05 00:24:58.798
End
2019-04-05 00:27:12.353
Duration
0:02:13.555
Note, WebLog generation is not included in the time.

CASA logs for stage 6