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 7.7767e-04 Jy/beam
minimum 1.2098e-04 Jy/beam
mean 1.9380e-04 Jy/beam
median 1.4875e-04 Jy/beam
sigma 9.1274e-05 Jy/beam
MAD rms 1.6859e-05 Jy/beam

RMS images

TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms

Pilot.ql.SGC1A_0.J210600_014235.10.2048.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_SGC1A_0.J210600+014235_P29014v1_2019_01_31T22_55_01.417/working/TSKY0001.sb32443742.eb32465054.57590.22834526621_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1A_0.J210600+014235_P29014v1_2019_01_31T22_55_01.417/working
Start time
2019-02-02 08:05:01.398
End
2019-02-02 08:07:06.968
Duration
0:02:05.570
Note, WebLog generation is not included in the time.

CASA logs for stage 6