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 6.4690e-04 Jy/beam
minimum 1.2920e-04 Jy/beam
mean 1.9570e-04 Jy/beam
median 1.5291e-04 Jy/beam
sigma 8.9143e-05 Jy/beam
MAD rms 1.4255e-05 Jy/beam

RMS images

TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms

Pilot.ql.SGC3D_1.J015206_114236.10.2048.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_SGC3D_1.J015206+114236_P30223v1_2019_03_06T19_40_19.666/working/TSKY0001.sb32515804.eb32520104.57606.39461725694_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3D_1.J015206+114236_P30223v1_2019_03_06T19_40_19.666/working
Start time
2019-03-08 13:15:59.246
End
2019-03-08 13:18:16.076
Duration
0:02:16.830
Note, WebLog generation is not included in the time.

CASA logs for stage 6