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 6.2086e-04 Jy/beam
minimum 1.2139e-04 Jy/beam
mean 1.9904e-04 Jy/beam
median 1.5511e-04 Jy/beam
sigma 9.0225e-05 Jy/beam
MAD rms 1.9072e-05 Jy/beam

RMS images

TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms

Pilot.ql.Stripe82A_1_e3.J205800_004235.10.2048.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_Stripe82A_1_e3.J205800-004235_P32130v1_2019_01_31T18_17_26.727/working/TSKY0001.sb32553261.eb32562856.57622.31784837963_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Stripe82A_1_e3.J205800-004235_P32130v1_2019_01_31T18_17_26.727/working
Start time
2019-02-01 16:58:30.627
End
2019-02-01 16:59:57.033
Duration
0:01:26.406
Note, WebLog generation is not included in the time.

CASA logs for stage 6