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 8.4275e-04 Jy/beam
minimum 1.1362e-04 Jy/beam
mean 1.8762e-04 Jy/beam
median 1.4710e-04 Jy/beam
sigma 8.5810e-05 Jy/beam
MAD rms 2.2312e-05 Jy/beam

RMS images

TSKY0001.sb32503337.eb32660293.57632.412079305555_split.ms

Pilot.ql.CDFS_e3.J032918_233000.10.2048.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_CDFS_e3.J032918-233000_P33483v1_2019_01_31T20_10_43.952/working/TSKY0001.sb32503337.eb32660293.57632.412079305555_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_CDFS_e3.J032918-233000_P33483v1_2019_01_31T20_10_43.952/working
Start time
2019-02-02 23:16:20.433
End
2019-02-02 23:18:12.501
Duration
0:01:52.068
Note, WebLog generation is not included in the time.

CASA logs for stage 6