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Modeling the galaxy/light-mass connection with cosmological simulations | Argyro Tasitsiomi
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11 Dec 2006 | Abstract: | I review some results on the galaxy/light-mass connection obtained by dissipationless simulations in combination with a simple, non-parametric model to connect halo circular velocity to the luminosity of the galaxy they would host. I focus on the galaxy-mass correlation and mass-to-light ratios obtained from galaxy up to cluster scales. The predictions of this simple scheme are shown to be in very good agreement with SDSS observations. | Source: | arXiv, astro-ph/0612255 | Services: | Forum | Review | PDF | Favorites |
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