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 6.9930e-04 Jy/beam
minimum 1.2833e-04 Jy/beam
mean 2.1729e-04 Jy/beam
median 1.6982e-04 Jy/beam
sigma 1.0149e-04 Jy/beam
MAD rms 3.0040e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_0.J211448_104236.10.2048.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_SGC3A_0.J211448+104236_P30758v1_2019_03_06T17_24_34.683/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_0.J211448+104236_P30758v1_2019_03_06T17_24_34.683/working
Start time
2019-03-07 18:37:48.257
End
2019-03-07 18:39:29.615
Duration
0:01:41.358
Note, WebLog generation is not included in the time.

CASA logs for stage 6