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 6.7207e-04 Jy/beam
minimum 1.2237e-04 Jy/beam
mean 2.1693e-04 Jy/beam
median 1.8045e-04 Jy/beam
sigma 9.5621e-05 Jy/beam
MAD rms 5.5388e-05 Jy/beam

RMS images

TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms

Pilot.ql.Stripe82C_2_e2.J015800_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_2_e2.J015800+001724_P27153v1_2019_02_08T23_46_04.828/working/TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82C_2_e2.J015800+001724_P27153v1_2019_02_08T23_46_04.828/working
Start time
2019-02-10 06:56:51.396
End
2019-02-10 06:58:59.973
Duration
0:02:08.577
Note, WebLog generation is not included in the time.

CASA logs for stage 6