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 4.8743e-04 Jy/beam
minimum 1.0051e-04 Jy/beam
mean 1.5706e-04 Jy/beam
median 1.2082e-04 Jy/beam
sigma 7.1390e-05 Jy/beam
MAD rms 1.2263e-05 Jy/beam

RMS images

TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms

Pilot.ql.Cepheus_e2.J223739_653000.10.2048.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.J223739+653000_P33070v1_2019_01_15T00_38_35.529/working/TSKY0001.sb32360679.eb32488571.57600.210124351855_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cepheus_e2.J223739+653000_P33070v1_2019_01_15T00_38_35.529/working
Start time
2019-01-16 16:36:20.435
End
2019-01-16 16:38:12.254
Duration
0:01:51.819
Note, WebLog generation is not included in the time.

CASA logs for stage 6