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 6.5025e-04 Jy/beam
minimum 1.2775e-04 Jy/beam
mean 2.0474e-04 Jy/beam
median 1.5908e-04 Jy/beam
sigma 9.0129e-05 Jy/beam
MAD rms 2.0953e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82A_1_e3.J211800_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_1_e3.J211800+001724_P32145v1_2019_01_31T18_17_47.907/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_1_e3.J211800+001724_P32145v1_2019_01_31T18_17_47.907/working
Start time
2019-02-01 18:43:45.077
End
2019-02-01 18:45:41.126
Duration
0:01:56.049
Note, WebLog generation is not included in the time.

CASA logs for stage 6