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 7.4510e-04 Jy/beam
minimum 1.0864e-04 Jy/beam
mean 1.6956e-04 Jy/beam
median 1.2982e-04 Jy/beam
sigma 8.2910e-05 Jy/beam
MAD rms 1.1405e-05 Jy/beam

RMS images

VLASS1.2.sb36633416.eb36641475.58607.36298261574_split.ms

VLASS1.2.ql.T21t17.J160804_423000.10.2048.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_T21t17.J160804+423000_P49403v1_2019_05_07T22_37_42.507/working/VLASS1.2.sb36633416.eb36641475.58607.36298261574_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t17.J160804+423000_P49403v1_2019_05_07T22_37_42.507/working
Start time
2019-05-11 02:21:46.397
End
2019-05-11 02:24:26.018
Duration
0:02:39.621
Note, WebLog generation is not included in the time.

CASA logs for stage 6