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 5.8337e-04 Jy/beam
minimum 1.1192e-04 Jy/beam
mean 1.7504e-04 Jy/beam
median 1.3603e-04 Jy/beam
sigma 8.1851e-05 Jy/beam
MAD rms 1.4478e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_1.J015610_114236.10.2048.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.J015610+114236_P30938v1_2019_01_22T17_26_35.307/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_1.J015610+114236_P30938v1_2019_01_22T17_26_35.307/working
Start time
2019-01-24 10:56:38.763
End
2019-01-24 10:58:43.427
Duration
0:02:04.663
Note, WebLog generation is not included in the time.

CASA logs for stage 6