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 6.6290e-04 Jy/beam
minimum 1.2253e-04 Jy/beam
mean 1.9410e-04 Jy/beam
median 1.4510e-04 Jy/beam
sigma 9.6726e-05 Jy/beam
MAD rms 1.3669e-05 Jy/beam

RMS images

VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms

VLASS1.2.ql.T18t26.J185619_283000.10.2048.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_T18t26.J185619+283000_P50349v1_2019_06_03T23_04_15.952/working/VLASS1.2.sb36674136.eb36677242.58625.28268025463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t26.J185619+283000_P50349v1_2019_06_03T23_04_15.952/working
Start time
2019-06-05 05:25:31.546
End
2019-06-05 05:27:32.079
Duration
0:02:00.533
Note, WebLog generation is not included in the time.

CASA logs for stage 6