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 6.3641e-04 Jy/beam
minimum 1.1873e-04 Jy/beam
mean 2.0008e-04 Jy/beam
median 1.4891e-04 Jy/beam
sigma 1.0016e-04 Jy/beam
MAD rms 2.3630e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_1.J235341_094236.10.2048.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_SGC3B_1.J235341+094236_P30534v1_2019_01_23T21_00_12.007/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J235341+094236_P30534v1_2019_01_23T21_00_12.007/working
Start time
2019-01-25 00:36:56.198
End
2019-01-25 00:38:06.344
Duration
0:01:10.146
Note, WebLog generation is not included in the time.

CASA logs for stage 6