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 7.4673e-04 Jy/beam
minimum 1.3029e-04 Jy/beam
mean 2.1566e-04 Jy/beam
median 1.6437e-04 Jy/beam
sigma 1.0547e-04 Jy/beam
MAD rms 1.9718e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J172920_253000.10.2048.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_SgrA_e2.J172920-253000_P33236v1_2019_01_31T02_59_07.350/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J172920-253000_P33236v1_2019_01_31T02_59_07.350/working
Start time
2019-02-01 02:03:02.889
End
2019-02-01 02:04:42.521
Duration
0:01:39.631
Note, WebLog generation is not included in the time.

CASA logs for stage 6