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 6.6950e-04 Jy/beam
minimum 1.2721e-04 Jy/beam
mean 1.9883e-04 Jy/beam
median 1.5623e-04 Jy/beam
sigma 8.8845e-05 Jy/beam
MAD rms 1.6994e-05 Jy/beam

RMS images

TSKY0001.sb32552567.eb32560928.57621.309616342594_split.ms

Pilot.ql.Stripe82A_0_e3.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_e3.J202600+001724_P27423v1_2019_01_30T21_59_48.753/working/TSKY0001.sb32552567.eb32560928.57621.309616342594_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_0_e3.J202600+001724_P27423v1_2019_01_30T21_59_48.753/working
Start time
2019-02-01 05:11:32.572
End
2019-02-01 05:13:37.220
Duration
0:02:04.648
Note, WebLog generation is not included in the time.

CASA logs for stage 6