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 6.6641e-04 Jy/beam
minimum 1.1143e-04 Jy/beam
mean 1.7209e-04 Jy/beam
median 1.3186e-04 Jy/beam
sigma 8.2883e-05 Jy/beam
MAD rms 1.2482e-05 Jy/beam

RMS images

VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms

VLASS1.2.ql.T17t30.J215602_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_T17t30.J215602+253000_P48938v1_2019_05_23T23_44_43.902/working/VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t30.J215602+253000_P48938v1_2019_05_23T23_44_43.902/working
Start time
2019-05-26 03:17:29.180
End
2019-05-26 03:19:23.087
Duration
0:01:53.908
Note, WebLog generation is not included in the time.

CASA logs for stage 6