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 9.0900e-04 Jy/beam
minimum 1.4417e-04 Jy/beam
mean 2.3324e-04 Jy/beam
median 1.7964e-04 Jy/beam
sigma 1.1211e-04 Jy/beam
MAD rms 1.9303e-05 Jy/beam

RMS images

VLASS1.2.sb36404986.eb36465932.58552.531894976855_split.ms

VLASS1.2.ql.T08t28.J181011_113000.10.2048.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_T08t28.J181011-113000_P35750v1_2019_04_05T17_00_23.906/working/VLASS1.2.sb36404986.eb36465932.58552.531894976855_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T08t28.J181011-113000_P35750v1_2019_04_05T17_00_23.906/working
Start time
2019-04-06 19:04:02.551
End
2019-04-06 19:05:51.576
Duration
0:01:49.025
Note, WebLog generation is not included in the time.

CASA logs for stage 6