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 9.4343e-04 Jy/beam
minimum 1.3673e-04 Jy/beam
mean 2.2159e-04 Jy/beam
median 1.7781e-04 Jy/beam
sigma 1.0118e-04 Jy/beam
MAD rms 3.3367e-05 Jy/beam

RMS images

TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms

Pilot.ql.Stripe82D_0_e1.J023800_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_0_e1.J023800-004235_P31607v1_2019_02_01T22_11_00.530/working/TSKY0001.sb32298423.eb32347173.57564.53262469907_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82D_0_e1.J023800-004235_P31607v1_2019_02_01T22_11_00.530/working
Start time
2019-02-02 19:02:28.688
End
2019-02-02 19:04:19.191
Duration
0:01:50.503
Note, WebLog generation is not included in the time.

CASA logs for stage 6