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 7.1385e-04 Jy/beam
minimum 1.1534e-04 Jy/beam
mean 1.9297e-04 Jy/beam
median 1.4961e-04 Jy/beam
sigma 9.1517e-05 Jy/beam
MAD rms 2.4869e-05 Jy/beam

RMS images

TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms

Pilot.ql.SGC1C_0.J231001_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.J231001+034235_P28231v1_2019_02_05T17_46_34.189/working/TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1C_0.J231001+034235_P28231v1_2019_02_05T17_46_34.189/working
Start time
2019-02-07 03:49:52.311
End
2019-02-07 03:51:50.341
Duration
0:01:58.029
Note, WebLog generation is not included in the time.

CASA logs for stage 6