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 6.3505e-04 Jy/beam
minimum 1.1413e-04 Jy/beam
mean 1.9031e-04 Jy/beam
median 1.4143e-04 Jy/beam
sigma 9.7444e-05 Jy/beam
MAD rms 1.8982e-05 Jy/beam

RMS images

VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms

VLASS1.2.ql.T18t10.J072439_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_T18t10.J072439+313000_P41917v1_2019_12_10T16_16_21.085/working/VLASS1.2.sb36537173.eb36600072.58595.859788263886_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t10.J072439+313000_P41917v1_2019_12_10T16_16_21.085/working
Start time
2019-12-11 11:46:35.706
End
2019-12-11 11:47:48.347
Duration
0:01:12.642
Note, WebLog generation is not included in the time.

CASA logs for stage 6