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 5.9721e-04 Jy/beam
minimum 1.0690e-04 Jy/beam
mean 1.7671e-04 Jy/beam
median 1.3675e-04 Jy/beam
sigma 8.6037e-05 Jy/beam
MAD rms 1.8563e-05 Jy/beam

RMS images

TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms

Pilot.ql.SGC3C_0.J230059_124236.10.2048.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_0.J230059+124236_P30903v1_2019_01_22T20_37_30.783/working/TSKY0001.sb32513487.eb32527959.57611.25701277777_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3C_0.J230059+124236_P30903v1_2019_01_22T20_37_30.783/working
Start time
2019-01-24 12:10:52.801
End
2019-01-24 12:12:51.476
Duration
0:01:58.675
Note, WebLog generation is not included in the time.

CASA logs for stage 6