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 8.1028e-04 Jy/beam
minimum 1.3923e-04 Jy/beam
mean 2.2520e-04 Jy/beam
median 1.7925e-04 Jy/beam
sigma 1.0719e-04 Jy/beam
MAD rms 2.6209e-05 Jy/beam

RMS images

TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms

Pilot.ql.Stripe82B_2_e3.J234200_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_Stripe82B_2_e3.J234200+001724_P32535v1_2019_02_01T16_52_48.133/working/TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_2_e3.J234200+001724_P32535v1_2019_02_01T16_52_48.133/working
Start time
2019-02-02 20:17:49.856
End
2019-02-02 20:19:28.086
Duration
0:01:38.230
Note, WebLog generation is not included in the time.

CASA logs for stage 6