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 8.8138e-04 Jy/beam
minimum 1.1909e-04 Jy/beam
mean 1.8962e-04 Jy/beam
median 1.4591e-04 Jy/beam
sigma 9.0529e-05 Jy/beam
MAD rms 1.5696e-05 Jy/beam

RMS images

VLASS1.2.sb36477997.eb36584946.58590.244118518516_split.ms

VLASS1.2.ql.T14t19.J122246_153000.10.2048.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_T14t19.J122246+153000_P37036v1_2019_05_02T19_25_45.199/working/VLASS1.2.sb36477997.eb36584946.58590.244118518516_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t19.J122246+153000_P37036v1_2019_05_02T19_25_45.199/working
Start time
2019-05-04 18:51:23.839
End
2019-05-04 18:53:19.409
Duration
0:01:55.570
Note, WebLog generation is not included in the time.

CASA logs for stage 6