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 5.0318e-03 Jy/beam
minimum 1.6526e-04 Jy/beam
mean 4.0154e-04 Jy/beam
median 3.2498e-04 Jy/beam
sigma 2.2048e-04 Jy/beam
MAD rms 1.4381e-04 Jy/beam

RMS images

VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms

VLASS1.2.ql.T14t30.J192203_143000.10.2048.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_T14t30.J192203+143000_P38117v1_2019_10_22T20_23_17.219/working/VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t30.J192203+143000_P38117v1_2019_10_22T20_23_17.219/working
Start time
2019-10-25 13:26:02.158
End
2019-10-25 13:26:49.120
Duration
0:00:46.963
Note, WebLog generation is not included in the time.

CASA logs for stage 6