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 1.2256e-03 Jy/beam
minimum 1.3403e-04 Jy/beam
mean 2.2874e-04 Jy/beam
median 1.7282e-04 Jy/beam
sigma 1.1105e-04 Jy/beam
MAD rms 3.5084e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_1.J215944_094236.10.2048.v2.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_1.J215944+094236_P30696v2_2019_03_13T21_40_50.064/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_1.J215944+094236_P30696v2_2019_03_13T21_40_50.064/working
Start time
2019-03-14 10:37:32.133
End
2019-03-14 10:38:43.334
Duration
0:01:11.201
Note, WebLog generation is not included in the time.

CASA logs for stage 6