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 6.0126e-04 Jy/beam
minimum 1.1949e-04 Jy/beam
mean 1.8442e-04 Jy/beam
median 1.4412e-04 Jy/beam
sigma 8.4783e-05 Jy/beam
MAD rms 1.4009e-05 Jy/beam

RMS images

TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms

Pilot.ql.SGC2C_1.J010214_074236.10.2048.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.J010214+074236_P29473v1_2019_02_06T00_48_01.295/working/TSKY0001.sb32476919.eb32479828.57594.43471144676_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC2C_1.J010214+074236_P29473v1_2019_02_06T00_48_01.295/working
Start time
2019-02-07 07:32:10.266
End
2019-02-07 07:33:52.107
Duration
0:01:41.841
Note, WebLog generation is not included in the time.

CASA logs for stage 6