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 7.2017e-04 Jy/beam
minimum 1.4098e-04 Jy/beam
mean 2.1984e-04 Jy/beam
median 1.6998e-04 Jy/beam
sigma 1.0393e-04 Jy/beam
MAD rms 1.6273e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_0.J204203_064235.10.2048.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_SGC2A_0.J204203+064235_P30044v1_2019_02_09T00_18_55.746/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_0.J204203+064235_P30044v1_2019_02_09T00_18_55.746/working
Start time
2019-02-10 16:17:05.524
End
2019-02-10 16:19:13.404
Duration
0:02:07.881
Note, WebLog generation is not included in the time.

CASA logs for stage 6