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 5.9614e-04 Jy/beam
minimum 1.0912e-04 Jy/beam
mean 1.7517e-04 Jy/beam
median 1.3508e-04 Jy/beam
sigma 8.4945e-05 Jy/beam
MAD rms 1.2937e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J205544_393000.10.2048.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_Cygnus_e3.J205544+393000_P33696v1_2019_02_07T16_00_22.815/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J205544+393000_P33696v1_2019_02_07T16_00_22.815/working
Start time
2019-02-09 08:56:37.260
End
2019-02-09 08:58:47.336
Duration
0:02:10.077
Note, WebLog generation is not included in the time.

CASA logs for stage 6