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 6.0934e-04 Jy/beam
minimum 1.1126e-04 Jy/beam
mean 1.7983e-04 Jy/beam
median 1.3934e-04 Jy/beam
sigma 8.6391e-05 Jy/beam
MAD rms 1.5237e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_1.J024601_034235.10.2048.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_SGC1E_1.J024601+034235_P29933v1_2019_02_07T17_28_29.511/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_1.J024601+034235_P29933v1_2019_02_07T17_28_29.511/working
Start time
2019-02-09 09:48:14.033
End
2019-02-09 09:50:42.213
Duration
0:02:28.180
Note, WebLog generation is not included in the time.

CASA logs for stage 6