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 7.0736e-04 Jy/beam
minimum 1.1548e-04 Jy/beam
mean 2.1443e-04 Jy/beam
median 1.7712e-04 Jy/beam
sigma 9.3452e-05 Jy/beam
MAD rms 5.0491e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_0.J000203_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_0.J000203+064235_P33924v1_2019_02_12T20_19_05.050/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_0.J000203+064235_P33924v1_2019_02_12T20_19_05.050/working
Start time
2019-02-13 18:30:51.331
End
2019-02-13 18:32:55.254
Duration
0:02:03.923
Note, WebLog generation is not included in the time.

CASA logs for stage 6