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 8.5102e-04 Jy/beam
minimum 1.5704e-04 Jy/beam
mean 2.4833e-04 Jy/beam
median 1.9075e-04 Jy/beam
sigma 1.2123e-04 Jy/beam
MAD rms 1.8227e-05 Jy/beam

RMS images

TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms

Pilot.ql.Stripe82B_2_e3.J232600_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_2_e3.J232600-004235_P32521v1_2019_02_01T16_52_02.729/working/TSKY0001.sb32554307.eb32557640.57620.209545798614_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82B_2_e3.J232600-004235_P32521v1_2019_02_01T16_52_02.729/working
Start time
2019-02-02 08:56:44.485
End
2019-02-02 08:58:39.857
Duration
0:01:55.372
Note, WebLog generation is not included in the time.

CASA logs for stage 6