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 8.4349e-04 Jy/beam
minimum 1.1530e-04 Jy/beam
mean 1.8003e-04 Jy/beam
median 1.3808e-04 Jy/beam
sigma 8.8928e-05 Jy/beam
MAD rms 1.3036e-05 Jy/beam

RMS images

VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms

VLASS1.2.ql.T15t20.J142530_183000.10.2048.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_T15t20.J142530+183000_P39160v1_2019_04_04T15_20_41.762/working/VLASS1.2.sb36492430.eb36542481.58573.39361230324_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t20.J142530+183000_P39160v1_2019_04_04T15_20_41.762/working
Start time
2019-04-06 04:36:49.159
End
2019-04-06 04:38:54.714
Duration
0:02:05.555
Note, WebLog generation is not included in the time.

CASA logs for stage 6