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 1.0723e-03 Jy/beam
minimum 1.1987e-04 Jy/beam
mean 2.3088e-04 Jy/beam
median 1.8827e-04 Jy/beam
sigma 1.1284e-04 Jy/beam
MAD rms 6.5216e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t13.J090217_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.J090217+293000_P41807v1_2019_04_20T23_19_21.900/working/VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t13.J090217+293000_P41807v1_2019_04_20T23_19_21.900/working
Start time
2020-01-02 03:12:39.200
End
2020-01-02 03:13:44.994
Duration
0:01:05.794
Note, WebLog generation is not included in the time.

CASA logs for stage 6