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 8.9104e-04 Jy/beam
minimum 1.1232e-04 Jy/beam
mean 1.7944e-04 Jy/beam
median 1.3814e-04 Jy/beam
sigma 8.4516e-05 Jy/beam
MAD rms 1.5929e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms

Pilot.ql.Cepheus_e3.J232200_603000.10.2048.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_Cepheus_e3.J232200+603000_P33108v1_2019_03_06T00_05_15.301/working/TSKY0001.sb32360679.eb32488742.57601.2146350463_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e3.J232200+603000_P33108v1_2019_03_06T00_05_15.301/working
Start time
2019-03-08 05:26:31.825
End
2019-03-08 05:28:12.993
Duration
0:01:41.167
Note, WebLog generation is not included in the time.

CASA logs for stage 6