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 8.3510e-04 Jy/beam
minimum 1.2317e-04 Jy/beam
mean 2.0166e-04 Jy/beam
median 1.5314e-04 Jy/beam
sigma 9.7187e-05 Jy/beam
MAD rms 1.7825e-05 Jy/beam

RMS images

VLASS1.2.sb36478588.eb36498992.58563.30308221065_split.ms

VLASS1.2.ql.T15t21.J151024_163000.10.2048.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_T15t21.J151024+163000_P37089v1_2019_03_27T23_43_01.274/working/VLASS1.2.sb36478588.eb36498992.58563.30308221065_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t21.J151024+163000_P37089v1_2019_03_27T23_43_01.274/working
Start time
2019-03-29 02:16:17.541
End
2019-03-29 02:17:59.277
Duration
0:01:41.737
Note, WebLog generation is not included in the time.

CASA logs for stage 6