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 6.8772e-04 Jy/beam
minimum 1.1926e-04 Jy/beam
mean 1.8958e-04 Jy/beam
median 1.4186e-04 Jy/beam
sigma 9.6796e-05 Jy/beam
MAD rms 1.2510e-05 Jy/beam

RMS images

VLASS1.2.sb36590526.eb36714484.58634.49575069445_split.ms

VLASS1.2.ql.T23t03.J023937_493000.10.2048.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_T23t03.J023937+493000_P46755v1_2019_06_26T15_58_16.238/working/VLASS1.2.sb36590526.eb36714484.58634.49575069445_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t03.J023937+493000_P46755v1_2019_06_26T15_58_16.238/working
Start time
2019-06-28 11:37:05.401
End
2019-06-28 11:38:43.583
Duration
0:01:38.182
Note, WebLog generation is not included in the time.

CASA logs for stage 6