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 9.0643e-04 Jy/beam
minimum 1.2072e-04 Jy/beam
mean 1.8758e-04 Jy/beam
median 1.4570e-04 Jy/beam
sigma 8.8261e-05 Jy/beam
MAD rms 1.5174e-05 Jy/beam

RMS images

VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms

VLASS1.2.ql.T24t05.J043633_533000.10.2048.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_T24t05.J043633+533000_P35428v1_2019_03_13T21_14_08.906/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T24t05.J043633+533000_P35428v1_2019_03_13T21_14_08.906/working
Start time
2019-03-16 00:00:10.809
End
2019-03-16 00:02:18.973
Duration
0:02:08.164
Note, WebLog generation is not included in the time.

CASA logs for stage 6