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 6.9543e-04 Jy/beam
minimum 1.1927e-04 Jy/beam
mean 2.0583e-04 Jy/beam
median 1.5584e-04 Jy/beam
sigma 9.7041e-05 Jy/beam
MAD rms 2.9937e-05 Jy/beam

RMS images

TSKY0001.sb36463619.eb36473386.58555.315533263885_split.ms

Test_1.2.ql.T26t10.J131938_633000.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Test_T26t10.J131938+633000_P35904v1_2019_03_21T22_09_50.935/working/TSKY0001.sb36463619.eb36473386.58555.315533263885_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Test_T26t10.J131938+633000_P35904v1_2019_03_21T22_09_50.935/working
Start time
2019-03-22 12:03:41.926
End
2019-03-22 12:04:59.864
Duration
0:01:17.938
Note, WebLog generation is not included in the time.

CASA logs for stage 7