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 7.6337e-04 Jy/beam
minimum 1.2207e-04 Jy/beam
mean 1.9398e-04 Jy/beam
median 1.4993e-04 Jy/beam
sigma 9.5343e-05 Jy/beam
MAD rms 1.4410e-05 Jy/beam

RMS images

TSKY0001.sb32295801.eb32296475.57549.31722762731_split.ms

Pilot.ql.Stripe82A_0_e1.J202600_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.J202600+001724_P27524v1_2019_01_23T00_39_19.139/working/TSKY0001.sb32295801.eb32296475.57549.31722762731_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_0_e1.J202600+001724_P27524v1_2019_01_23T00_39_19.139/working
Start time
2019-01-25 10:14:06.301
End
2019-01-25 10:15:58.254
Duration
0:01:51.953
Note, WebLog generation is not included in the time.

CASA logs for stage 6