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 5.6469e-04 Jy/beam
minimum 1.1532e-04 Jy/beam
mean 1.7719e-04 Jy/beam
median 1.3528e-04 Jy/beam
sigma 8.5226e-05 Jy/beam
MAD rms 1.1501e-05 Jy/beam

RMS images

VLASS1.2.sb36730336.eb36770756.58641.97701479167_split.ms

VLASS1.2.ql.T17t15.J104102_253000.10.2048.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_T17t15.J104102+253000_P51432v1_2019_06_19T17_27_14.782/working/VLASS1.2.sb36730336.eb36770756.58641.97701479167_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t15.J104102+253000_P51432v1_2019_06_19T17_27_14.782/working
Start time
2019-06-21 12:24:21.207
End
2019-06-21 12:26:01.275
Duration
0:01:40.069
Note, WebLog generation is not included in the time.

CASA logs for stage 6