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 6.7289e-04 Jy/beam
minimum 1.1457e-04 Jy/beam
mean 2.0808e-04 Jy/beam
median 1.5651e-04 Jy/beam
sigma 1.0213e-04 Jy/beam
MAD rms 3.3762e-05 Jy/beam

RMS images

TSKY0001.sb32433643.eb32445263.57584.55763373843_split.ms

Pilot.ql.CDFS_e1.J035335_223000.10.2048.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.J035335-223000_P33665v1_2019_02_04T17_20_53.324/working/TSKY0001.sb32433643.eb32445263.57584.55763373843_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_CDFS_e1.J035335-223000_P33665v1_2019_02_04T17_20_53.324/working
Start time
2019-02-05 07:46:17.279
End
2019-02-05 07:47:30.791
Duration
0:01:13.512
Note, WebLog generation is not included in the time.

CASA logs for stage 6