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 5.8941e-04 Jy/beam
minimum 1.1608e-04 Jy/beam
mean 2.0266e-04 Jy/beam
median 1.7078e-04 Jy/beam
sigma 8.8472e-05 Jy/beam
MAD rms 5.5602e-05 Jy/beam

RMS images

VLASS1.2.sb36486269.eb36608627.58598.318571932876_split.ms

VLASS1.2.ql.T14t20.J124203_133000.10.2048.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_T14t20.J124203+133000_P38475v1_2019_04_25T22_13_14.983/working/VLASS1.2.sb36486269.eb36608627.58598.318571932876_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t20.J124203+133000_P38475v1_2019_04_25T22_13_14.983/working
Start time
2019-12-17 09:49:33.824
End
2019-12-17 09:50:44.641
Duration
0:01:10.817
Note, WebLog generation is not included in the time.

CASA logs for stage 6