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 9.7228e-04 Jy/beam
minimum 1.1532e-04 Jy/beam
mean 1.8669e-04 Jy/beam
median 1.4475e-04 Jy/beam
sigma 9.1472e-05 Jy/beam
MAD rms 1.7857e-05 Jy/beam

RMS images

TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms

Pilot.ql.SGC2C_1.J010210_064235.10.2048.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_SGC2C_1.J010210+064235_P29463v1_2019_02_06T00_47_45.655/working/TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2C_1.J010210+064235_P29463v1_2019_02_06T00_47_45.655/working
Start time
2019-02-07 20:56:28.128
End
2019-02-07 20:59:07.317
Duration
0:02:39.189
Note, WebLog generation is not included in the time.

CASA logs for stage 6