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 7.8696e-04 Jy/beam
minimum 1.1569e-04 Jy/beam
mean 1.9033e-04 Jy/beam
median 1.4767e-04 Jy/beam
sigma 9.1217e-05 Jy/beam
MAD rms 1.9409e-05 Jy/beam

RMS images

TSKY0001.sb32433643.eb32445263.57584.55763373843_split.ms

Pilot.ql.CDFS_e1.J032520_263000.10.2048.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_e1.J032520-263000_P33614v1_2019_02_04T17_18_24.950/working/TSKY0001.sb32433643.eb32445263.57584.55763373843_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_CDFS_e1.J032520-263000_P33614v1_2019_02_04T17_18_24.950/working
Start time
2019-02-07 02:47:15.599
End
2019-02-07 02:49:07.431
Duration
0:01:51.831
Note, WebLog generation is not included in the time.

CASA logs for stage 6