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 8.1912e-04 Jy/beam
minimum 1.0753e-04 Jy/beam
mean 1.8088e-04 Jy/beam
median 1.4026e-04 Jy/beam
sigma 9.2831e-05 Jy/beam
MAD rms 2.6432e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T19t26.J201155_333000.10.2048.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_T19t26.J201155+333000_P48718v1_2019_06_19T14_40_28.136/working/VLASS1.2.sb36624415.eb36765605.58641.29728032407_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T19t26.J201155+333000_P48718v1_2019_06_19T14_40_28.136/working
Start time
2019-06-26 18:18:28.157
End
2019-06-26 18:20:39.388
Duration
0:02:11.231
Note, WebLog generation is not included in the time.

CASA logs for stage 6