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 7.4236e-04 Jy/beam
minimum 1.4504e-04 Jy/beam
mean 2.3922e-04 Jy/beam
median 1.8705e-04 Jy/beam
sigma 1.1052e-04 Jy/beam
MAD rms 3.2876e-05 Jy/beam

RMS images

TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms

Pilot.ql.Stripe82D_2_e1.J035800_004235.10.2048.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_Stripe82D_2_e1.J035800-004235_P31627v1_2019_02_01T17_13_30.381/working/TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_2_e1.J035800-004235_P31627v1_2019_02_01T17_13_30.381/working
Start time
2019-02-02 15:11:16.741
End
2019-02-02 15:12:55.877
Duration
0:01:39.137
Note, WebLog generation is not included in the time.

CASA logs for stage 6