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 8.8083e-04 Jy/beam
minimum 1.2848e-04 Jy/beam
mean 2.0614e-04 Jy/beam
median 1.6055e-04 Jy/beam
sigma 9.3779e-05 Jy/beam
MAD rms 2.3899e-05 Jy/beam

RMS images

TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms

Pilot.ql.Stripe82A_2_e2.J214600_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_Stripe82A_2_e2.J214600-004235_P27160v1_2019_02_08T23_46_15.989/working/TSKY0001.sb32450678.eb32484186.57598.27566423611_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_2_e2.J214600-004235_P27160v1_2019_02_08T23_46_15.989/working
Start time
2019-02-10 10:34:17.146
End
2019-02-10 10:36:12.603
Duration
0:01:55.457
Note, WebLog generation is not included in the time.

CASA logs for stage 6