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 6.4461e-04 Jy/beam
minimum 1.1467e-04 Jy/beam
mean 1.9521e-04 Jy/beam
median 1.4081e-04 Jy/beam
sigma 1.0317e-04 Jy/beam
MAD rms 1.8915e-05 Jy/beam

RMS images

VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms

VLASS1.2.ql.T18t05.J031126_293000.10.2048.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_T18t05.J031126+293000_P37635v1_2019_04_05T16_05_45.770/working/VLASS1.2.sb36467167.eb36536584.58571.64133251157_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t05.J031126+293000_P37635v1_2019_04_05T16_05_45.770/working
Start time
2019-04-06 10:46:23.221
End
2019-04-06 10:47:35.993
Duration
0:01:12.772
Note, WebLog generation is not included in the time.

CASA logs for stage 6