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 8.7212e-04 Jy/beam
minimum 1.3295e-04 Jy/beam
mean 2.2257e-04 Jy/beam
median 1.6825e-04 Jy/beam
sigma 1.0411e-04 Jy/beam
MAD rms 2.8314e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82B_1_e3.J224600_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_Stripe82B_1_e3.J224600-004235_P32147v1_2019_04_14T23_38_22.985/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_1_e3.J224600-004235_P32147v1_2019_04_14T23_38_22.985/working
Start time
2019-04-16 04:33:36.290
End
2019-04-16 04:34:47.312
Duration
0:01:11.022
Note, WebLog generation is not included in the time.

CASA logs for stage 6