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 7.0393e-04 Jy/beam
minimum 1.2253e-04 Jy/beam
mean 1.9758e-04 Jy/beam
median 1.5424e-04 Jy/beam
sigma 8.7380e-05 Jy/beam
MAD rms 1.7069e-05 Jy/beam

RMS images

TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms

Pilot.ql.SGC1D_1.J015800_044235.10.2048.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_SGC1D_1.J015800+044235_P33863v1_2019_02_09T01_05_41.091/working/TSKY0001.sb32502758.eb32530448.57615.25466265046_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1D_1.J015800+044235_P33863v1_2019_02_09T01_05_41.091/working
Start time
2019-02-11 08:05:02.411
End
2019-02-11 08:06:53.768
Duration
0:01:51.358
Note, WebLog generation is not included in the time.

CASA logs for stage 6