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 9.6508e-04 Jy/beam
minimum 1.3002e-04 Jy/beam
mean 2.2729e-04 Jy/beam
median 1.7193e-04 Jy/beam
sigma 1.1013e-04 Jy/beam
MAD rms 3.3752e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_1.J221011_084236.10.2048.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_1.J221011+084236_P30106v1_2019_02_13T22_36_57.760/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_1.J221011+084236_P30106v1_2019_02_13T22_36_57.760/working
Start time
2019-02-14 13:58:10.411
End
2019-02-14 13:59:27.819
Duration
0:01:17.409
Note, WebLog generation is not included in the time.

CASA logs for stage 6