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 7.5410e-04 Jy/beam
minimum 1.1099e-04 Jy/beam
mean 1.8984e-04 Jy/beam
median 1.4621e-04 Jy/beam
sigma 9.3857e-05 Jy/beam
MAD rms 2.2197e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J012333_104236.10.2048.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_SGC3C_1.J012333+104236_P30919v1_2019_01_22T20_46_16.564/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J012333+104236_P30919v1_2019_01_22T20_46_16.564/working
Start time
2019-01-24 10:54:10.083
End
2019-01-24 10:56:18.414
Duration
0:02:08.331
Note, WebLog generation is not included in the time.

CASA logs for stage 6