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 7.8488e-04 Jy/beam
minimum 1.4460e-04 Jy/beam
mean 2.3331e-04 Jy/beam
median 1.7603e-04 Jy/beam
sigma 1.1564e-04 Jy/beam
MAD rms 1.9087e-05 Jy/beam

RMS images

TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms

Pilot.ql.Stripe82A_2_e3.J215800_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_2_e3.J215800+001724_P32519v1_2019_02_01T16_51_56.073/working/TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_2_e3.J215800+001724_P32519v1_2019_02_01T16_51_56.073/working
Start time
2019-02-02 11:48:17.369
End
2019-02-02 11:49:52.976
Duration
0:01:35.607
Note, WebLog generation is not included in the time.

CASA logs for stage 6