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 6.6216e-04 Jy/beam
minimum 1.2458e-04 Jy/beam
mean 2.0032e-04 Jy/beam
median 1.5687e-04 Jy/beam
sigma 9.4285e-05 Jy/beam
MAD rms 1.7808e-05 Jy/beam

RMS images

TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms

Pilot.ql.Stripe82D_1_e3.J025400_001724.10.2048.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_1_e3.J025400+001724_P32737v1_2019_03_06T17_46_16.518/working/TSKY0001.sb32554861.eb32626144.57628.33101865741_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_1_e3.J025400+001724_P32737v1_2019_03_06T17_46_16.518/working
Start time
2019-03-08 05:48:27.542
End
2019-03-08 05:50:28.779
Duration
0:02:01.237
Note, WebLog generation is not included in the time.

CASA logs for stage 6