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 6.2050e-04 Jy/beam
minimum 1.2040e-04 Jy/beam
mean 1.8547e-04 Jy/beam
median 1.4501e-04 Jy/beam
sigma 8.5703e-05 Jy/beam
MAD rms 1.4927e-05 Jy/beam

RMS images

VLASS1.2.sb36589288.eb36724054.58636.42679225694_split.ms

VLASS1.2.ql.T23t01.J001533_503000.10.2048.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_T23t01.J001533+503000_P46628v1_2019_06_26T19_18_05.245/working/VLASS1.2.sb36589288.eb36724054.58636.42679225694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T23t01.J001533+503000_P46628v1_2019_06_26T19_18_05.245/working
Start time
2019-06-28 20:38:03.014
End
2019-06-28 20:40:11.306
Duration
0:02:08.292
Note, WebLog generation is not included in the time.

CASA logs for stage 6