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 7.6694e-04 Jy/beam
minimum 1.2801e-04 Jy/beam
mean 2.0977e-04 Jy/beam
median 1.6373e-04 Jy/beam
sigma 9.2784e-05 Jy/beam
MAD rms 2.2750e-05 Jy/beam

RMS images

TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms

Pilot.ql.Stripe82D_2_e2.J035800_001724.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_2_e2.J035800+001724_P28363v2_2019_03_05T15_23_17.925/working/TSKY0001.sb32458590.eb32483782.57597.441518437496_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_2_e2.J035800+001724_P28363v2_2019_03_05T15_23_17.925/working
Start time
2019-03-06 08:31:04.951
End
2019-03-06 08:32:58.015
Duration
0:01:53.064
Note, WebLog generation is not included in the time.

CASA logs for stage 6