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 8.9390e-04 Jy/beam
minimum 1.2738e-04 Jy/beam
mean 2.1140e-04 Jy/beam
median 1.6118e-04 Jy/beam
sigma 1.1180e-04 Jy/beam
MAD rms 1.6311e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J173409_293000.10.2048.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.J173409-293000_P33278v1_2019_01_18T00_15_56.470/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J173409-293000_P33278v1_2019_01_18T00_15_56.470/working
Start time
2019-01-19 23:11:40.752
End
2019-01-19 23:13:58.130
Duration
0:02:17.378
Note, WebLog generation is not included in the time.

CASA logs for stage 6