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 7.9948e-04 Jy/beam
minimum 1.6891e-04 Jy/beam
mean 2.6275e-04 Jy/beam
median 2.1244e-04 Jy/beam
sigma 1.0940e-04 Jy/beam
MAD rms 3.3060e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_0.J210621_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_0.J210621+084236_P30070v1_2019_02_09T00_19_38.958/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_0.J210621+084236_P30070v1_2019_02_09T00_19_38.958/working
Start time
2019-02-10 17:28:37.571
End
2019-02-10 17:30:41.206
Duration
0:02:03.635
Note, WebLog generation is not included in the time.

CASA logs for stage 6