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 8.7359e-04 Jy/beam
minimum 1.1945e-04 Jy/beam
mean 1.9545e-04 Jy/beam
median 1.4621e-04 Jy/beam
sigma 9.9825e-05 Jy/beam
MAD rms 1.8126e-05 Jy/beam

RMS images

VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms

VLASS1.2.ql.T18t13.J092926_283000.10.2048.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_T18t13.J092926+283000_P41803v1_2019_05_09T21_45_51.374/working/VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t13.J092926+283000_P41803v1_2019_05_09T21_45_51.374/working
Start time
2019-05-11 22:31:11.333
End
2019-05-11 22:33:15.355
Duration
0:02:04.023
Note, WebLog generation is not included in the time.

CASA logs for stage 6