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 5.8802e-04 Jy/beam
minimum 1.1233e-04 Jy/beam
mean 1.7423e-04 Jy/beam
median 1.3313e-04 Jy/beam
sigma 8.4354e-05 Jy/beam
MAD rms 1.2323e-05 Jy/beam

RMS images

VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms

VLASS1.2.ql.T17t26.J185602_253000.10.2048.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_T17t26.J185602+253000_P48894v1_2019_05_23T23_42_10.090/working/VLASS1.2.sb36627706.eb36662063.58620.307527881945_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.2_T17t26.J185602+253000_P48894v1_2019_05_23T23_42_10.090/working
Start time
2019-05-26 06:27:19.182
End
2019-05-26 06:29:28.398
Duration
0:02:09.215
Note, WebLog generation is not included in the time.

CASA logs for stage 6