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 6.1727e-04 Jy/beam
minimum 1.1515e-04 Jy/beam
mean 1.7852e-04 Jy/beam
median 1.3663e-04 Jy/beam
sigma 8.8922e-05 Jy/beam
MAD rms 1.2456e-05 Jy/beam

RMS images

VLASS2.1.sb38694041.eb38838729.59146.565794803246_split.ms

VLASS2.1.ql.T03t19.J123418_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/VLASS2.1_T03t19.J123418-293000_P73255v1_2020_10_24T18_49_50.663/working/VLASS2.1.sb38694041.eb38838729.59146.565794803246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS2.1_T03t19.J123418-293000_P73255v1_2020_10_24T18_49_50.663/working
Start time
2020-11-18 22:33:33.553
End
2020-11-18 22:35:15.051
Duration
0:01:41.499
Note, WebLog generation is not included in the time.

CASA logs for stage 6