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 8.4549e-04 Jy/beam
minimum 1.1861e-04 Jy/beam
mean 1.8970e-04 Jy/beam
median 1.4437e-04 Jy/beam
sigma 9.4106e-05 Jy/beam
MAD rms 1.3663e-05 Jy/beam

RMS images

VLASS1.2.sb36628294.eb36692385.58629.33235776621_split.ms

VLASS1.2.ql.T17t31.J230730_253000.10.2048.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_T17t31.J230730+253000_P48990v1_2019_06_04T18_13_47.419/working/VLASS1.2.sb36628294.eb36692385.58629.33235776621_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t31.J230730+253000_P48990v1_2019_06_04T18_13_47.419/working
Start time
2019-06-06 12:56:46.810
End
2019-06-06 12:58:55.408
Duration
0:02:08.598
Note, WebLog generation is not included in the time.

CASA logs for stage 6