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 2.5214e-03 Jy/beam
minimum 1.1759e-04 Jy/beam
mean 1.9918e-04 Jy/beam
median 1.5033e-04 Jy/beam
sigma 1.1047e-04 Jy/beam
MAD rms 2.7683e-05 Jy/beam

RMS images

VLASS1.2.sb36487050.eb36572852.58584.34754221065_split.ms

VLASS1.2.ql.T14t24.J155040_123000.10.2048.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_T14t24.J155040+123000_P38350v1_2019_04_18T19_58_39.514/working/VLASS1.2.sb36487050.eb36572852.58584.34754221065_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t24.J155040+123000_P38350v1_2019_04_18T19_58_39.514/working
Start time
2019-04-19 20:02:07.207
End
2019-04-19 20:03:21.253
Duration
0:01:14.046
Note, WebLog generation is not included in the time.

CASA logs for stage 6