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 6.6373e-04 Jy/beam
minimum 1.0504e-04 Jy/beam
mean 1.6922e-04 Jy/beam
median 1.2976e-04 Jy/beam
sigma 8.1929e-05 Jy/beam
MAD rms 1.4534e-05 Jy/beam

RMS images

VLASS1.2.sb36604324.eb36612725.58599.03784488426_split.ms

VLASS1.2.ql.T20t10.J074459_383000.10.2048.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_T20t10.J074459+383000_P48153v1_2019_05_15T15_40_24.073/working/VLASS1.2.sb36604324.eb36612725.58599.03784488426_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T20t10.J074459+383000_P48153v1_2019_05_15T15_40_24.073/working
Start time
2019-05-18 08:26:53.931
End
2019-05-18 08:29:34.814
Duration
0:02:40.882
Note, WebLog generation is not included in the time.

CASA logs for stage 6