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 8.5154e-04 Jy/beam
minimum 1.5528e-04 Jy/beam
mean 2.5359e-04 Jy/beam
median 1.9971e-04 Jy/beam
sigma 1.1126e-04 Jy/beam
MAD rms 3.0643e-05 Jy/beam

RMS images

TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms

Pilot.ql.COSMOS_e1.J101400_003000.10.2048.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_COSMOS_e1.J101400+003000_P27821v1_2019_02_04T17_05_30.716/working/TSKY0001.sb32331132.eb32347267.57564.798545428246_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_COSMOS_e1.J101400+003000_P27821v1_2019_02_04T17_05_30.716/working
Start time
2019-02-05 20:34:19.515
End
2019-02-05 20:36:17.287
Duration
0:01:57.772
Note, WebLog generation is not included in the time.

CASA logs for stage 6