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 8.8133e-04 Jy/beam
minimum 1.2638e-04 Jy/beam
mean 2.0981e-04 Jy/beam
median 1.5932e-04 Jy/beam
sigma 1.0219e-04 Jy/beam
MAD rms 2.2051e-05 Jy/beam

RMS images

TSKY0001.sb32295801.eb32296475.57549.31722762731_split.ms

Pilot.ql.Stripe82A_0_e1.J200200_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_Stripe82A_0_e1.J200200+001724_P27518v1_2019_01_23T00_39_09.122/working/TSKY0001.sb32295801.eb32296475.57549.31722762731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_0_e1.J200200+001724_P27518v1_2019_01_23T00_39_09.122/working
Start time
2019-01-24 20:09:39.732
End
2019-01-24 20:11:08.331
Duration
0:01:28.599
Note, WebLog generation is not included in the time.

CASA logs for stage 6