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 5.8175e-04 Jy/beam
minimum 1.1558e-04 Jy/beam
mean 1.8540e-04 Jy/beam
median 1.4325e-04 Jy/beam
sigma 8.3005e-05 Jy/beam
MAD rms 1.8026e-05 Jy/beam

RMS images

TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms

Pilot.ql.SGC1E_1.J024200_014235.10.2048.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.J024200+014235_P29912v1_2019_02_07T17_11_03.306/working/TSKY0001.sb32468630.eb32488498.57599.53490315972_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1E_1.J024200+014235_P29912v1_2019_02_07T17_11_03.306/working
Start time
2019-02-08 18:13:49.101
End
2019-02-08 18:15:46.437
Duration
0:01:57.336
Note, WebLog generation is not included in the time.

CASA logs for stage 6