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 5.9777e-04 Jy/beam
minimum 1.1155e-04 Jy/beam
mean 1.7680e-04 Jy/beam
median 1.3512e-04 Jy/beam
sigma 8.4692e-05 Jy/beam
MAD rms 1.3084e-05 Jy/beam

RMS images

VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms

VLASS1.2.ql.T16t26.J190424_223000.10.2048.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_T16t26.J190424+223000_P38982v1_2019_04_02T16_42_22.433/working/VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t26.J190424+223000_P38982v1_2019_04_02T16_42_22.433/working
Start time
2019-04-04 06:14:22.855
End
2019-04-04 06:16:33.083
Duration
0:02:10.228
Note, WebLog generation is not included in the time.

CASA logs for stage 6