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 5.8148e-04 Jy/beam
minimum 1.0888e-04 Jy/beam
mean 1.6911e-04 Jy/beam
median 1.2925e-04 Jy/beam
sigma 8.3961e-05 Jy/beam
MAD rms 1.1292e-05 Jy/beam

RMS images

VLASS1.2.sb36531292.eb36576618.58587.88283292824_split.ms

VLASS1.2.ql.T16t11.J074459_213000.10.2048.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_T16t11.J074459+213000_P41631v1_2019_04_29T01_09_46.745/working/VLASS1.2.sb36531292.eb36576618.58587.88283292824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t11.J074459+213000_P41631v1_2019_04_29T01_09_46.745/working
Start time
2019-05-01 02:46:41.004
End
2019-05-01 02:48:55.483
Duration
0:02:14.479
Note, WebLog generation is not included in the time.

CASA logs for stage 6