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 7.6323e-04 Jy/beam
minimum 1.1732e-04 Jy/beam
mean 1.9216e-04 Jy/beam
median 1.5220e-04 Jy/beam
sigma 8.6815e-05 Jy/beam
MAD rms 2.6193e-05 Jy/beam

RMS images

TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms

Pilot.ql.SGC1C_0.J224601_034235.10.2048.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_SGC1C_0.J224601+034235_P28225v1_2019_02_08T15_19_45.757/working/TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1C_0.J224601+034235_P28225v1_2019_02_08T15_19_45.757/working
Start time
2019-02-13 09:43:35.723
End
2019-02-13 09:45:49.223
Duration
0:02:13.500
Note, WebLog generation is not included in the time.

CASA logs for stage 6