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 7.9004e-04 Jy/beam
minimum 1.3893e-04 Jy/beam
mean 2.2056e-04 Jy/beam
median 1.6818e-04 Jy/beam
sigma 1.0810e-04 Jy/beam
MAD rms 1.9411e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_0.J205405_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_SGC2A_0.J205405+054235_P30037v1_2019_02_09T00_18_43.283/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_0.J205405+054235_P30037v1_2019_02_09T00_18_43.283/working
Start time
2019-02-10 12:48:17.028
End
2019-02-10 12:50:15.039
Duration
0:01:58.010
Note, WebLog generation is not included in the time.

CASA logs for stage 6