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 7.8163e-04 Jy/beam
minimum 1.1997e-04 Jy/beam
mean 1.9343e-04 Jy/beam
median 1.4541e-04 Jy/beam
sigma 9.6302e-05 Jy/beam
MAD rms 1.7174e-05 Jy/beam

RMS images

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

VLASS1.2.ql.T18t09.J062023_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_T18t09.J062023+283000_P41841v1_2019_05_09T21_47_38.001/working/VLASS1.2.sb36536600.eb36595636.58593.827866736116_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T18t09.J062023+283000_P41841v1_2019_05_09T21_47_38.001/working
Start time
2019-05-11 22:35:17.598
End
2019-05-11 22:37:18.109
Duration
0:02:00.511
Note, WebLog generation is not included in the time.

CASA logs for stage 6