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 2.1974e-03 Jy/beam
minimum 1.5056e-04 Jy/beam
mean 2.5862e-04 Jy/beam
median 1.9942e-04 Jy/beam
sigma 1.2789e-04 Jy/beam
MAD rms 3.7000e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82C_1_e3.J010200_001724.10.2048.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_Stripe82C_1_e3.J010200+001724_P32121v1_2019_02_01T22_16_09.079/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82C_1_e3.J010200+001724_P32121v1_2019_02_01T22_16_09.079/working
Start time
2019-02-05 13:47:25.140
End
2019-02-05 13:48:46.792
Duration
0:01:21.652
Note, WebLog generation is not included in the time.

CASA logs for stage 6