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 6.1224e-04 Jy/beam
minimum 1.1101e-04 Jy/beam
mean 1.7322e-04 Jy/beam
median 1.3674e-04 Jy/beam
sigma 7.9658e-05 Jy/beam
MAD rms 1.6421e-05 Jy/beam

RMS images

VLASS1.2.sb36487638.eb36576920.58588.434619479165_split.ms

VLASS1.2.ql.T14t28.J181018_143000.10.2048.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_T14t28.J181018+143000_P38323v1_2019_04_29T01_48_54.343/working/VLASS1.2.sb36487638.eb36576920.58588.434619479165_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t28.J181018+143000_P38323v1_2019_04_29T01_48_54.343/working
Start time
2019-05-01 21:15:48.534
End
2019-05-01 21:18:14.806
Duration
0:02:26.272
Note, WebLog generation is not included in the time.

CASA logs for stage 6