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 5.9806e-04 Jy/beam
minimum 1.1819e-04 Jy/beam
mean 1.8703e-04 Jy/beam
median 1.4613e-04 Jy/beam
sigma 8.1920e-05 Jy/beam
MAD rms 1.6823e-05 Jy/beam

RMS images

TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms

Pilot.ql.Stripe82A_1_e2.J205000_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_1_e2.J205000-004235_P28001v1_2019_02_04T17_37_18.404/working/TSKY0001.sb32448102.eb32462094.57589.39807837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_1_e2.J205000-004235_P28001v1_2019_02_04T17_37_18.404/working
Start time
2019-02-05 21:39:31.912
End
2019-02-05 21:41:42.828
Duration
0:02:10.916
Note, WebLog generation is not included in the time.

CASA logs for stage 6