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 6.3402e-04 Jy/beam
minimum 1.1085e-04 Jy/beam
mean 1.9142e-04 Jy/beam
median 1.3877e-04 Jy/beam
sigma 1.0041e-04 Jy/beam
MAD rms 2.0816e-05 Jy/beam

RMS images

TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms

Pilot.ql.Cygnus_e3.J210344_393000.10.2048.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_Cygnus_e3.J210344+393000_P33698v1_2019_02_07T16_07_36.020/working/TSKY0001.sb32522754.eb32557595.57620.02690508102_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_Cygnus_e3.J210344+393000_P33698v1_2019_02_07T16_07_36.020/working
Start time
2019-02-08 09:42:42.139
End
2019-02-08 09:44:05.460
Duration
0:01:23.322
Note, WebLog generation is not included in the time.

CASA logs for stage 6