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 5.2283e-04 Jy/beam
minimum 9.9464e-05 Jy/beam
mean 1.6629e-04 Jy/beam
median 1.3051e-04 Jy/beam
sigma 7.5873e-05 Jy/beam
MAD rms 1.8399e-05 Jy/beam

RMS images

VLASS1.1.sb34671004.eb34701330.58075.89221989583_split.ms

VLASS1.1.ql.T26t18.J224407_613000.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T26t18.J224407+613000_P17399v2_2017_11_18T18_32_21.710/working/VLASS1.1.sb34671004.eb34701330.58075.89221989583_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/VLASS1.1_T26t18.J224407+613000_P17399v2_2017_11_18T18_32_21.710/working
Start time
2020-02-13 07:39:17.359
End
2020-02-13 07:40:34.529
Duration
0:01:17.170
Note, WebLog generation is not included in the time.

CASA logs for stage 6