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 7.3119e-04 Jy/beam
minimum 1.2027e-04 Jy/beam
mean 1.9233e-04 Jy/beam
median 1.4711e-04 Jy/beam
sigma 9.7409e-05 Jy/beam
MAD rms 1.2921e-05 Jy/beam

RMS images

VLASS1.2.sb36482658.eb36556685.58578.76741302083_split.ms

VLASS1.2.ql.T15t06.J040349_173000.10.2048.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_T15t06.J040349+173000_P39419v1_2019_04_12T16_27_34.588/working/VLASS1.2.sb36482658.eb36556685.58578.76741302083_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T15t06.J040349+173000_P39419v1_2019_04_12T16_27_34.588/working
Start time
2019-04-14 01:25:56.044
End
2019-04-14 01:27:44.022
Duration
0:01:47.979
Note, WebLog generation is not included in the time.

CASA logs for stage 6