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 2.3525e-03 Jy/beam
minimum 1.3051e-04 Jy/beam
mean 2.5032e-04 Jy/beam
median 1.8746e-04 Jy/beam
sigma 1.3564e-04 Jy/beam
MAD rms 4.7049e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J175549_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.J175549-253000_P33242v1_2019_02_04T16_51_28.863/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J175549-253000_P33242v1_2019_02_04T16_51_28.863/working
Start time
2019-02-06 03:08:04.552
End
2019-02-06 03:09:19.110
Duration
0:01:14.559
Note, WebLog generation is not included in the time.

CASA logs for stage 6