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 9.7652e-04 Jy/beam
minimum 1.3303e-04 Jy/beam
mean 2.2354e-04 Jy/beam
median 1.6676e-04 Jy/beam
sigma 1.1539e-04 Jy/beam
MAD rms 2.5310e-05 Jy/beam

RMS images

VLASS1.2.sb36439263.eb36692177.58628.395548472225_split.ms

VLASS1.2.ql.T21t24.J234629_433000.10.2048.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_T21t24.J234629+433000_P44274v1_2019_06_10T19_15_59.228/working/VLASS1.2.sb36439263.eb36692177.58628.395548472225_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T21t24.J234629+433000_P44274v1_2019_06_10T19_15_59.228/working
Start time
2019-06-11 20:35:55.511
End
2019-06-11 20:37:10.843
Duration
0:01:15.332
Note, WebLog generation is not included in the time.

CASA logs for stage 6