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 6.4132e-04 Jy/beam
minimum 1.1231e-04 Jy/beam
mean 1.7882e-04 Jy/beam
median 1.3531e-04 Jy/beam
sigma 9.1719e-05 Jy/beam
MAD rms 1.3480e-05 Jy/beam

RMS images

VLASS1.2.sb36566777.eb36762108.58640.463947303244_split.ms

VLASS1.2.ql.T19t05.J031423_333000.10.2048.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_T19t05.J031423+333000_P45615v1_2019_09_23T20_10_25.295/working/VLASS1.2.sb36566777.eb36762108.58640.463947303244_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T19t05.J031423+333000_P45615v1_2019_09_23T20_10_25.295/working
Start time
2019-09-24 23:32:43.064
End
2019-09-24 23:34:15.096
Duration
0:01:32.032
Note, WebLog generation is not included in the time.

CASA logs for stage 6