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 1.1925e-03 Jy/beam
minimum 1.0213e-04 Jy/beam
mean 1.5957e-04 Jy/beam
median 1.2142e-04 Jy/beam
sigma 7.7705e-05 Jy/beam
MAD rms 1.1585e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms

Pilot.ql.Cepheus_e2.J224159_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_e2.J224159+603000_P33019v1_2019_01_15T17_36_32.021/working/TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e2.J224159+603000_P33019v1_2019_01_15T17_36_32.021/working
Start time
2019-01-17 19:48:23.166
End
2019-01-17 19:50:40.498
Duration
0:02:17.332
Note, WebLog generation is not included in the time.

CASA logs for stage 6