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 6.1002e-04 Jy/beam
minimum 1.2041e-04 Jy/beam
mean 1.9726e-04 Jy/beam
median 1.5089e-04 Jy/beam
sigma 9.3678e-05 Jy/beam
MAD rms 2.2129e-05 Jy/beam

RMS images

VLASS1.2.sb36675323.eb36772845.58643.26662539352_split.ms

VLASS1.2.ql.T18t31.J231253_283000.10.2048.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_T18t31.J231253+283000_P50643v1_2019_11_27T15_03_58.595/working/VLASS1.2.sb36675323.eb36772845.58643.26662539352_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t31.J231253+283000_P50643v1_2019_11_27T15_03_58.595/working
Start time
2019-11-28 03:49:05.283
End
2019-11-28 03:50:08.599
Duration
0:01:03.316
Note, WebLog generation is not included in the time.

CASA logs for stage 6