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 8.0929e-04 Jy/beam
minimum 1.2082e-04 Jy/beam
mean 2.0258e-04 Jy/beam
median 1.6385e-04 Jy/beam
sigma 9.2164e-05 Jy/beam
MAD rms 3.3264e-05 Jy/beam

RMS images

TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms

Pilot.ql.Stripe82D_0_e3.J023800_004235.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_0_e3.J023800-004235_P32773v1_2019_03_06T17_47_11.926/working/TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_0_e3.J023800-004235_P32773v1_2019_03_06T17_47_11.926/working
Start time
2019-03-08 00:22:40.481
End
2019-03-08 00:24:49.397
Duration
0:02:08.916
Note, WebLog generation is not included in the time.

CASA logs for stage 6