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 9.3850e-04 Jy/beam
minimum 1.2853e-04 Jy/beam
mean 2.1511e-04 Jy/beam
median 1.6423e-04 Jy/beam
sigma 9.9485e-05 Jy/beam
MAD rms 2.5444e-05 Jy/beam

RMS images

TSKY0001.sb32552567.eb32560928.57621.309616342594_split.ms

Pilot.ql.Stripe82A_0_e3.J200200_004235.10.2048.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.J200200-004235_P27407v1_2019_01_30T21_59_22.510/working/TSKY0001.sb32552567.eb32560928.57621.309616342594_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_0_e3.J200200-004235_P27407v1_2019_01_30T21_59_22.510/working
Start time
2019-01-31 16:17:32.123
End
2019-01-31 16:19:07.315
Duration
0:01:35.192
Note, WebLog generation is not included in the time.

CASA logs for stage 6