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 6.1691e-04 Jy/beam
minimum 1.0861e-04 Jy/beam
mean 1.9562e-04 Jy/beam
median 1.6312e-04 Jy/beam
sigma 9.0153e-05 Jy/beam
MAD rms 5.2246e-05 Jy/beam

RMS images

VLASS1.2.sb36439829.eb36514324.58567.4355214699_split.ms

VLASS1.2.ql.T24t20.J190314_523000.10.2048.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_T24t20.J190314+523000_P38780v1_2019_10_21T17_46_52.204/working/VLASS1.2.sb36439829.eb36514324.58567.4355214699_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T24t20.J190314+523000_P38780v1_2019_10_21T17_46_52.204/working
Start time
2019-10-22 11:37:08.329
End
2019-10-22 11:38:27.830
Duration
0:01:19.501
Note, WebLog generation is not included in the time.

CASA logs for stage 6