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 7.8565e-04 Jy/beam
minimum 1.3599e-04 Jy/beam
mean 2.1501e-04 Jy/beam
median 1.6513e-04 Jy/beam
sigma 1.0310e-04 Jy/beam
MAD rms 1.8201e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T14t30.J195502_143000.10.2048.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_T14t30.J195502+143000_P38125v1_2019_10_22T20_23_21.015/working/VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t30.J195502+143000_P38125v1_2019_10_22T20_23_21.015/working
Start time
2019-10-23 19:44:29.684
End
2019-10-23 19:46:09.855
Duration
0:01:40.171
Note, WebLog generation is not included in the time.

CASA logs for stage 6