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 7.9385e-04 Jy/beam
minimum 1.6460e-04 Jy/beam
mean 2.6153e-04 Jy/beam
median 2.1047e-04 Jy/beam
sigma 1.1144e-04 Jy/beam
MAD rms 3.6299e-05 Jy/beam

RMS images

TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms

Pilot.ql.SGC2A_0.J205816_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.J205816+084236_P30068v1_2019_02_09T00_19_35.696/working/TSKY0001.sb32470405.eb32492399.57602.30093894676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2A_0.J205816+084236_P30068v1_2019_02_09T00_19_35.696/working
Start time
2019-02-10 08:12:00.107
End
2019-02-10 08:13:56.480
Duration
0:01:56.373
Note, WebLog generation is not included in the time.

CASA logs for stage 6