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Published byHerman Irawan Modified over 6 years ago
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Jon Purnell Heidi Jo Newberg Malik Magdon-Ismail
Probabilistic Approach to Finding Geometric Objects in Spatial Datasets of the Milky Way Jon Purnell Heidi Jo Newberg Malik Magdon-Ismail Rensselaer Polytechnic Institute ISMIS 2005
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Motivation Simultaneously fit multiple geometric distributions
Use distributions with varying complexity Automatic parameter optimization No need to filter data
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Real Data Applied algorithm to 2.5 degree wide wedge along the celestial equator from SDSS dataset.
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Galactic (Background) Distribution
Power Law Hernquist Equation
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Tidal Stream Distribution
An ellipse with a 2-d Gaussian cross-section
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Model Distribution Mixture of Background and Stream distributions
Numerical Integration over wedge
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Data Efficiency Efficiency – ratio of the number of stars in dataset to the actual number of stars in the galaxy
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Parameter Optimization
Reduce parameter set Unconstrain parameters Conjugate gradients
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Synthetic Data Generate data using mixture model
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Synthetic Data Results
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Real Data Applied algorithm to 2.5 degree wide wedge along the celestial equator from SDSS dataset.
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Real Data Results
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Future Plans Apply different distributions for halo stars
Search for multiple streams Search for other structures Search over multiple ‘wedges’ simultaneously
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Questions ?
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