Digital Cosmology
Timeline
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Slices at redshift zero
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Gas Temperature Evolution
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Cold Dark Matter and Gas: Gas Temperature Evolution
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Mixed Dark Matter and Gas: Gas Density Evolution
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1. What are X-Ray clusters?
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2. How are they simulated?
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3. Simulation in a 2-D, co-moving frame
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4. Adding a third dimension
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5. From square patch to datacube
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6a. Gas density evolution (co-moving frame)
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6b. Gas density evolution (co-moving frame)
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7. Gas temperature evolution (co-moving
frame)
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8. Evolution of X-ray luminosity in 2-10Kev band (proper frame)
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9. Flythrough of Gas Density
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10. Flythrough of Gas Temperature
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11. Flythrough of X-ray luminosity
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