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M48 HR data linearity | by Mickut
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M48 HR data linearity

Scatter plot and linear fit of star flux based raw magnitude vs Tycho catalog magnitude based on Messier 48 open cluster image B and G channel data.


This data is utilized in my Hertzsprung-Russell diagram of M48.


Tycho catalog B and V magnitudes were used, which accounts for small discrepancies since my filters are not photometric.


I also wrote a blog posting about the process.

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Uploaded on January 17, 2015