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 6.3231e-04 Jy/beam
minimum 1.1475e-04 Jy/beam
mean 1.8081e-04 Jy/beam
median 1.3819e-04 Jy/beam
sigma 8.7373e-05 Jy/beam
MAD rms 1.2803e-05 Jy/beam

RMS images

VLASS1.2.sb36624415.eb36765605.58641.29728032407_split.ms

VLASS1.2.ql.T19t30.J235300_343000.10.2048.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_T19t30.J235300+343000_P48777v1_2019_06_14T18_19_37.029/working/VLASS1.2.sb36624415.eb36765605.58641.29728032407_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T19t30.J235300+343000_P48777v1_2019_06_14T18_19_37.029/working
Start time
2019-06-16 03:54:19.482
End
2019-06-16 03:55:57.557
Duration
0:01:38.075
Note, WebLog generation is not included in the time.

CASA logs for stage 6