Visualization of structures and cosmic flows in the ... - CLUES-Project
Visualization of structures and cosmic flows in the ... - CLUES-Project
Visualization of structures and cosmic flows in the ... - CLUES-Project
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Galaxy color is set<br />
aga<strong>in</strong>st <strong>the</strong> FilamentID<br />
• <strong>the</strong> histogram shows <strong>the</strong> distribution<br />
<strong>of</strong> this variable<br />
• <strong>the</strong> color palette shown <strong>in</strong> <strong>the</strong><br />
background <strong>of</strong> <strong>the</strong> histogram is used to<br />
provide <strong>the</strong> colors to <strong>the</strong> galaxies<br />
• this palette can be tuned us<strong>in</strong>g a<br />
dedicated <strong>in</strong>terface<br />
• a subsample <strong>of</strong> galaxies can be<br />
selected aga<strong>in</strong>st this FilamentID<br />
distribution by sett<strong>in</strong>g a m<strong>in</strong> <strong>and</strong> a max<br />
• this can be done by click<strong>in</strong>g directly on<br />
<strong>the</strong> histogram or fill<strong>in</strong>g <strong>the</strong> m<strong>in</strong> <strong>and</strong><br />
max fields<br />
• <strong>the</strong> color palette can ei<strong>the</strong>r be<br />
stretched between <strong>the</strong> m<strong>in</strong> <strong>and</strong> <strong>the</strong><br />
max or kept locked<br />
• variables o<strong>the</strong>r tha FilamentID can be<br />
used, for example <strong>the</strong> Mabs