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 6.2320e-04 Jy/beam
minimum 1.1617e-04 Jy/beam
mean 1.9472e-04 Jy/beam
median 1.4816e-04 Jy/beam
sigma 9.2309e-05 Jy/beam
MAD rms 2.1198e-05 Jy/beam

RMS images

TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms

Pilot.ql.SGC2C_1.J003401_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_SGC2C_1.J003401+084236_P29476v1_2019_02_06T00_48_06.419/working/TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2C_1.J003401+084236_P29476v1_2019_02_06T00_48_06.419/working
Start time
2019-02-06 21:18:35.573
End
2019-02-06 21:20:14.246
Duration
0:01:38.673
Note, WebLog generation is not included in the time.

CASA logs for stage 6