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 9.9428e-04 Jy/beam
minimum 1.2652e-04 Jy/beam
mean 2.0954e-04 Jy/beam
median 1.6054e-04 Jy/beam
sigma 1.0330e-04 Jy/beam
MAD rms 2.3974e-05 Jy/beam

RMS images

TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms

Pilot.ql.SgrA_e3.J175605_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.J175605-263000_P33316v1_2019_01_18T00_16_58.774/working/TSKY0001.sb32503898.eb32530404.57613.06443417824_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SgrA_e3.J175605-263000_P33316v1_2019_01_18T00_16_58.774/working
Start time
2019-01-21 09:52:16.256
End
2019-01-21 09:54:14.756
Duration
0:01:58.500
Note, WebLog generation is not included in the time.

CASA logs for stage 6