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 6.3504e-04 Jy/beam
minimum 1.1003e-04 Jy/beam
mean 1.7661e-04 Jy/beam
median 1.3516e-04 Jy/beam
sigma 8.3385e-05 Jy/beam
MAD rms 1.4887e-05 Jy/beam

RMS images

TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms

Pilot.ql.SGC2C_0.J225004_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_SGC2C_0.J225004+054235_P29490v1_2019_02_06T00_48_28.410/working/TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2C_0.J225004+054235_P29490v1_2019_02_06T00_48_28.410/working
Start time
2019-02-07 05:32:45.687
End
2019-02-07 05:34:30.282
Duration
0:01:44.595
Note, WebLog generation is not included in the time.

CASA logs for stage 6