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 5.9605e-04 Jy/beam
minimum 1.1119e-04 Jy/beam
mean 1.7469e-04 Jy/beam
median 1.3516e-04 Jy/beam
sigma 8.1988e-05 Jy/beam
MAD rms 1.2746e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T16t26.J190416_213000.10.2048.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.J190416+213000_P38971v1_2019_04_02T16_37_01.187/working/VLASS1.2.sb36493574.eb36520029.58568.39485275463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T16t26.J190416+213000_P38971v1_2019_04_02T16_37_01.187/working
Start time
2019-04-04 13:27:11.191
End
2019-04-04 13:29:07.086
Duration
0:01:55.894
Note, WebLog generation is not included in the time.

CASA logs for stage 6