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 6.8116e-04 Jy/beam
minimum 1.1599e-04 Jy/beam
mean 1.8022e-04 Jy/beam
median 1.3843e-04 Jy/beam
sigma 8.7247e-05 Jy/beam
MAD rms 1.2409e-05 Jy/beam

RMS images

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

VLASS2.1.ql.T25t17.J214710_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.J214710+593000_P63820v1_2020_09_06T19_32_44.959/working/VLASS2.1.sb38523814.eb38632964.59098.28982543982_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T25t17.J214710+593000_P63820v1_2020_09_06T19_32_44.959/working
Start time
2020-09-18 05:40:22.909
End
2020-09-18 05:42:07.412
Duration
0:01:44.503
Note, WebLog generation is not included in the time.

CASA logs for stage 6