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 6.7270e-04 Jy/beam
minimum 1.1533e-04 Jy/beam
mean 1.7741e-04 Jy/beam
median 1.3666e-04 Jy/beam
sigma 8.5002e-05 Jy/beam
MAD rms 1.1531e-05 Jy/beam

RMS images

VLASS1.2.sb36518823.eb36595674.58595.435916689814_split.ms

VLASS1.2.ql.T15t29.J213533_173000.10.2048.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_T15t29.J213533+173000_P43827v1_2019_05_12T19_50_17.847/working/VLASS1.2.sb36518823.eb36595674.58595.435916689814_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t29.J213533+173000_P43827v1_2019_05_12T19_50_17.847/working
Start time
2019-05-15 04:56:17.094
End
2019-05-15 04:58:22.223
Duration
0:02:05.129
Note, WebLog generation is not included in the time.

CASA logs for stage 6