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tests:astropars:challenge1 [2014/10/31 15:02] – randraetests:astropars:challenge1 [2022/10/24 12:26] (current) – external edit 127.0.0.1
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 (Zuckerman & Song 2004) around the solar peculiar motion. (Zuckerman & Song 2004) around the solar peculiar motion.
  
 +{{:tests:uv_groups.png|}}
  
 Unlike open clusters, association members are very sparse, with their nearest Unlike open clusters, association members are very sparse, with their nearest
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 not always apparent in some projections: not always apparent in some projections:
  
-{{:tests:groupc_uwmemb_.png|}}+
 {{:tests:groupc_uw_.png|}} {{:tests:groupc_uw_.png|}}
 +{{:tests:groupc_uwmemb_.png|}}
  
 This could obviously be automated with well-known clustering methods.  This could obviously be automated with well-known clustering methods. 
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 over the background field stars.  over the background field stars. 
  
-{{:tests:cmd_groups.png|}}+
  
 Young stars are typically several magnitudes above the main sequence and well Young stars are typically several magnitudes above the main sequence and well
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-{{:tests:uv_groups.png|}}+
  
  
  
tests/astropars/challenge1.1414767765.txt.gz · Last modified: 2022/10/24 12:26 (external edit)