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 7.3959e-04 Jy/beam
minimum 1.1031e-04 Jy/beam
mean 1.9541e-04 Jy/beam
median 1.6715e-04 Jy/beam
sigma 8.5467e-05 Jy/beam
MAD rms 5.4845e-05 Jy/beam

RMS images

VLASS1.2.sb36484370.eb36574402.58585.3477416088_split.ms

VLASS1.2.ql.T15t18.J124706_193000.10.2048.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_T15t18.J124706+193000_P38723v1_2019_12_09T17_38_11.217/working/VLASS1.2.sb36484370.eb36574402.58585.3477416088_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t18.J124706+193000_P38723v1_2019_12_09T17_38_11.217/working
Start time
2019-12-10 05:06:28.976
End
2019-12-10 05:07:30.991
Duration
0:01:02.015
Note, WebLog generation is not included in the time.

CASA logs for stage 6