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 7.7288e-04 Jy/beam
minimum 1.2259e-04 Jy/beam
mean 2.0243e-04 Jy/beam
median 1.5590e-04 Jy/beam
sigma 9.9743e-05 Jy/beam
MAD rms 1.8022e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J173817_263000.10.2048.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_e3.J173817-263000_P33312v1_2019_01_18T00_16_52.573/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J173817-263000_P33312v1_2019_01_18T00_16_52.573/working
Start time
2019-01-20 14:16:47.541
End
2019-01-20 14:19:01.888
Duration
0:02:14.347
Note, WebLog generation is not included in the time.

CASA logs for stage 6