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 6.2738e-04 Jy/beam
minimum 1.2157e-04 Jy/beam
mean 1.9346e-04 Jy/beam
median 1.4906e-04 Jy/beam
sigma 8.9868e-05 Jy/beam
MAD rms 1.7619e-05 Jy/beam

RMS images

VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms

VLASS1.2.ql.T24t05.J040319_533000.10.2048.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_T24t05.J040319+533000_P35423v1_2019_09_27T15_36_53.303/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T24t05.J040319+533000_P35423v1_2019_09_27T15_36_53.303/working
Start time
2019-09-28 18:21:53.584
End
2019-09-28 18:23:37.828
Duration
0:01:44.244
Note, WebLog generation is not included in the time.

CASA logs for stage 6