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 7.9385e-04 Jy/beam
minimum 1.2015e-04 Jy/beam
mean 1.9172e-04 Jy/beam
median 1.4613e-04 Jy/beam
sigma 9.5983e-05 Jy/beam
MAD rms 1.5340e-05 Jy/beam

RMS images

VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms

VLASS1.2.ql.T18t13.J090651_293000.10.2048.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_T18t13.J090651+293000_P41808v1_2019_05_09T21_46_08.203/working/VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t13.J090651+293000_P41808v1_2019_05_09T21_46_08.203/working
Start time
2019-05-13 01:37:54.805
End
2019-05-13 01:40:33.538
Duration
0:02:38.733
Note, WebLog generation is not included in the time.

CASA logs for stage 6