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 8.9199e-04 Jy/beam
minimum 1.1857e-04 Jy/beam
mean 2.1302e-04 Jy/beam
median 1.6774e-04 Jy/beam
sigma 9.5926e-05 Jy/beam
MAD rms 3.3689e-05 Jy/beam

RMS images

TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms

Pilot.ql.SGC2D_0.J003004_054235.10.2048.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_SGC2D_0.J003004+054235_P33921v1_2019_02_12T20_18_59.753/working/TSKY0001.sb32477510.eb32481415.57595.330938541665_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2D_0.J003004+054235_P33921v1_2019_02_12T20_18_59.753/working
Start time
2019-02-14 03:11:41.496
End
2019-02-14 03:13:16.157
Duration
0:01:34.661
Note, WebLog generation is not included in the time.

CASA logs for stage 6