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 6.7101e-04 Jy/beam
minimum 1.1900e-04 Jy/beam
mean 1.9734e-04 Jy/beam
median 1.5712e-04 Jy/beam
sigma 9.0540e-05 Jy/beam
MAD rms 2.3922e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_1.J020604_064235.10.2048.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_SGC2D_1.J020604+064235_P33965v1_2019_02_12T20_20_15.693/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_1.J020604+064235_P33965v1_2019_02_12T20_20_15.693/working
Start time
2019-02-14 04:03:35.044
End
2019-02-14 04:05:14.144
Duration
0:01:39.100
Note, WebLog generation is not included in the time.

CASA logs for stage 6