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 1.0010e-03 Jy/beam
minimum 1.2312e-04 Jy/beam
mean 1.9616e-04 Jy/beam
median 1.5196e-04 Jy/beam
sigma 9.0380e-05 Jy/beam
MAD rms 1.9060e-05 Jy/beam

RMS images

TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms

Pilot.ql.SGC3A_1.J222013_124236.10.2048.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_1.J222013+124236_P30733v1_2019_03_06T17_22_26.010/working/TSKY0001.sb32514645.eb32526281.57610.24174200231_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3A_1.J222013+124236_P30733v1_2019_03_06T17_22_26.010/working
Start time
2019-03-08 03:44:47.299
End
2019-03-08 03:46:30.290
Duration
0:01:42.991
Note, WebLog generation is not included in the time.

CASA logs for stage 6