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 6.9530e-04 Jy/beam
minimum 1.3373e-04 Jy/beam
mean 2.1718e-04 Jy/beam
median 1.7012e-04 Jy/beam
sigma 9.9439e-05 Jy/beam
MAD rms 2.0989e-05 Jy/beam

RMS images

VLASS2.1.sb38501480.eb38632936.59097.386918425924_split.ms

VLASS2.1.ql.T11t15.J093401_033000.10.2048.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_T11t15.J093401+033000_P62391v1_2020_09_05T22_03_28.852/working/VLASS2.1.sb38501480.eb38632936.59097.386918425924_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T11t15.J093401+033000_P62391v1_2020_09_05T22_03_28.852/working
Start time
2020-09-19 17:43:20.478
End
2020-09-19 17:44:41.311
Duration
0:01:20.833
Note, WebLog generation is not included in the time.

CASA logs for stage 6