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 7.8411e-04 Jy/beam
minimum 1.3545e-04 Jy/beam
mean 2.4520e-04 Jy/beam
median 1.7887e-04 Jy/beam
sigma 1.2829e-04 Jy/beam
MAD rms 3.4041e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms

Pilot.ql.SgrA_e2.J172504_323000.10.2048.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.J172504-323000_P33161v1_2019_01_31T17_44_24.668/working/TSKY0001.sb32503898.eb32516384.57605.08926986111_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e2.J172504-323000_P33161v1_2019_01_31T17_44_24.668/working
Start time
2019-02-01 03:41:34.120
End
2019-02-01 03:42:35.849
Duration
0:01:01.729
Note, WebLog generation is not included in the time.

CASA logs for stage 6