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 6.3045e-04 Jy/beam
minimum 1.2085e-04 Jy/beam
mean 2.0825e-04 Jy/beam
median 1.7332e-04 Jy/beam
sigma 8.9439e-05 Jy/beam
MAD rms 4.9791e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_0.J235801_054235.10.2048.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_0.J235801+054235_P33913v1_2019_02_12T20_18_41.484/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_0.J235801+054235_P33913v1_2019_02_12T20_18_41.484/working
Start time
2019-02-13 21:46:02.741
End
2019-02-13 21:47:55.698
Duration
0:01:52.956
Note, WebLog generation is not included in the time.

CASA logs for stage 6