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 8.6988e-04 Jy/beam
minimum 1.1419e-04 Jy/beam
mean 1.8065e-04 Jy/beam
median 1.3741e-04 Jy/beam
sigma 9.0466e-05 Jy/beam
MAD rms 1.2275e-05 Jy/beam

RMS images

VLASS2.1.sb38523814.eb38632964.59098.28982543982_split.ms

VLASS2.1.ql.T25t17.J221814_593000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T25t17.J221814+593000_P63824v1_2020_09_06T19_32_45.053/working/VLASS2.1.sb38523814.eb38632964.59098.28982543982_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T25t17.J221814+593000_P63824v1_2020_09_06T19_32_45.053/working
Start time
2020-09-18 15:41:47.639
End
2020-09-18 15:43:30.222
Duration
0:01:42.583
Note, WebLog generation is not included in the time.

CASA logs for stage 6