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 7.7118e-04 Jy/beam
minimum 1.4513e-04 Jy/beam
mean 2.4569e-04 Jy/beam
median 1.8729e-04 Jy/beam
sigma 1.1211e-04 Jy/beam
MAD rms 3.5216e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82B_1_e3.J231800_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.J231800-004235_P32155v1_2019_02_04T18_17_21.852/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_1_e3.J231800-004235_P32155v1_2019_02_04T18_17_21.852/working
Start time
2019-02-05 20:46:22.787
End
2019-02-05 20:47:38.373
Duration
0:01:15.586
Note, WebLog generation is not included in the time.

CASA logs for stage 6