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 8.1068e-04 Jy/beam
minimum 1.3088e-04 Jy/beam
mean 2.0631e-04 Jy/beam
median 1.5816e-04 Jy/beam
sigma 9.7927e-05 Jy/beam
MAD rms 1.4983e-05 Jy/beam

RMS images

VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms

VLASS1.2.ql.T14t27.J173838_153000.10.2048.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_T14t27.J173838+153000_P38171v1_2019_04_04T22_43_39.103/working/VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t27.J173838+153000_P38171v1_2019_04_04T22_43_39.103/working
Start time
2019-04-06 20:27:35.947
End
2019-04-06 20:29:23.029
Duration
0:01:47.082
Note, WebLog generation is not included in the time.

CASA logs for stage 6