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 8.3372e-04 Jy/beam
minimum 1.4944e-04 Jy/beam
mean 2.6413e-04 Jy/beam
median 2.3015e-04 Jy/beam
sigma 1.0714e-04 Jy/beam
MAD rms 7.0483e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T14t27.J175833_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_T14t27.J175833+143000_P38166v1_2019_10_22T20_22_59.154/working/VLASS1.2.sb36488814.eb36542213.58572.48964302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T14t27.J175833+143000_P38166v1_2019_10_22T20_22_59.154/working
Start time
2019-10-23 08:42:17.222
End
2019-10-23 08:43:48.626
Duration
0:01:31.404
Note, WebLog generation is not included in the time.

CASA logs for stage 6