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 6.4487e-04 Jy/beam
minimum 1.2001e-04 Jy/beam
mean 2.0657e-04 Jy/beam
median 1.5501e-04 Jy/beam
sigma 9.8982e-05 Jy/beam
MAD rms 2.6146e-05 Jy/beam

RMS images

VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms

VLASS1.2.ql.T24t05.J045954_533000.10.2048.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_T24t05.J045954+533000_P35432v1_2019_09_27T15_32_22.386/working/VLASS1.2.sb36398499.eb36445182.58547.81841561342_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T24t05.J045954+533000_P35432v1_2019_09_27T15_32_22.386/working
Start time
2019-09-28 08:12:23.445
End
2019-09-28 08:13:35.868
Duration
0:01:12.423
Note, WebLog generation is not included in the time.

CASA logs for stage 6