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 8.0705e-04 Jy/beam
minimum 1.3405e-04 Jy/beam
mean 2.1852e-04 Jy/beam
median 1.6067e-04 Jy/beam
sigma 1.2089e-04 Jy/beam
MAD rms 1.6190e-05 Jy/beam

RMS images

VLASS1.2.sb36611554.eb36692241.58628.86010204861_split.ms

VLASS1.2.ql.T21t11.J101816_403000.10.2048.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_T21t11.J101816+403000_P47407v1_2019_06_05T22_41_40.830/working/VLASS1.2.sb36611554.eb36692241.58628.86010204861_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t11.J101816+403000_P47407v1_2019_06_05T22_41_40.830/working
Start time
2019-06-07 04:06:27.967
End
2019-06-07 04:08:10.809
Duration
0:01:42.842
Note, WebLog generation is not included in the time.

CASA logs for stage 6