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 3.9476e-03 Jy/beam
minimum 1.1921e-04 Jy/beam
mean 2.7009e-04 Jy/beam
median 1.8451e-04 Jy/beam
sigma 2.2018e-04 Jy/beam
MAD rms 6.7615e-05 Jy/beam

RMS images

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

VLASS2.1.ql.T25t18.J232242_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_T25t18.J232242+593000_P63910v1_2020_09_06T20_35_13.519/working/VLASS2.1.sb38523814.eb38632964.59098.28982543982_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T25t18.J232242+593000_P63910v1_2020_09_06T20_35_13.519/working
Start time
2020-11-02 14:38:26.680
End
2020-11-02 14:39:20.754
Duration
0:00:54.074
Note, WebLog generation is not included in the time.

CASA logs for stage 6