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 7.2939e-04 Jy/beam
minimum 1.2028e-04 Jy/beam
mean 2.1724e-04 Jy/beam
median 1.7662e-04 Jy/beam
sigma 1.0445e-04 Jy/beam
MAD rms 5.3130e-05 Jy/beam

RMS images

VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms

VLASS1.2.ql.T17t02.J004711_243000.10.2048.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_T17t02.J004711+243000_P37313v1_2019_11_01T20_44_01.292/working/VLASS1.2.sb36470480.eb36511597.58565.708401296295_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t02.J004711+243000_P37313v1_2019_11_01T20_44_01.292/working
Start time
2019-11-02 14:18:52.135
End
2019-11-02 14:20:11.763
Duration
0:01:19.628
Note, WebLog generation is not included in the time.

CASA logs for stage 6