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 9.2118e-04 Jy/beam
minimum 1.2092e-04 Jy/beam
mean 1.9704e-04 Jy/beam
median 1.5739e-04 Jy/beam
sigma 9.0294e-05 Jy/beam
MAD rms 2.5395e-05 Jy/beam

RMS images

TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms

Pilot.ql.SGC1C_0.J225801_024235.10.2048.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_SGC1C_0.J225801+024235_P28218v1_2019_02_05T17_45_17.699/working/TSKY0001.sb32461178.eb32478431.57591.43888707176_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC1C_0.J225801+024235_P28218v1_2019_02_05T17_45_17.699/working
Start time
2019-02-07 12:01:06.177
End
2019-02-07 12:03:23.912
Duration
0:02:17.736
Note, WebLog generation is not included in the time.

CASA logs for stage 6