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 1.0224e-03 Jy/beam
minimum 1.0726e-04 Jy/beam
mean 1.8511e-04 Jy/beam
median 1.3729e-04 Jy/beam
sigma 9.5795e-05 Jy/beam
MAD rms 2.6331e-05 Jy/beam

RMS images

VLASS1.2.sb36507182.eb36649330.58612.33337462963_split.ms

VLASS1.2.ql.T23t21.J203413_503000.10.2048.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_T23t21.J203413+503000_P43212v1_2019_05_31T20_49_51.087/working/VLASS1.2.sb36507182.eb36649330.58612.33337462963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t21.J203413+503000_P43212v1_2019_05_31T20_49_51.087/working
Start time
2019-06-02 11:58:06.000
End
2019-06-02 11:59:21.963
Duration
0:01:15.963
Note, WebLog generation is not included in the time.

CASA logs for stage 6