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 6.1963e-04 Jy/beam
minimum 1.0905e-04 Jy/beam
mean 1.7401e-04 Jy/beam
median 1.3308e-04 Jy/beam
sigma 8.2510e-05 Jy/beam
MAD rms 1.4352e-05 Jy/beam

RMS images

VLASS1.2.sb36469888.eb36489419.58557.72455666667_split.ms

VLASS1.2.ql.T17t05.J033809_273000.10.2048.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_T17t05.J033809+273000_P37308v1_2019_03_20T18_11_34.839/working/VLASS1.2.sb36469888.eb36489419.58557.72455666667_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t05.J033809+273000_P37308v1_2019_03_20T18_11_34.839/working
Start time
2019-03-22 01:00:28.665
End
2019-03-22 01:02:14.538
Duration
0:01:45.872
Note, WebLog generation is not included in the time.

CASA logs for stage 6