Search Results - "Millennium Simulation"

The Spitzer extragalactic representative volume survey: The environments of high-z SDSS quasi-stellar objects by Falder, J., Stevens, J., Jarvis, M., Bonfield, D., Lacy, M., Farrah, D., Oliver, S., Surace, J., Mauduit, J., Vaccari, M., Marchetti, L., González-Solares, E., Afonso, J., Cava, A., Seymour, Nick

“…We compare our findings to the predictions of a semi-analytic galaxy formation model, based on the ΛCDM MILLENNIUM simulation, and find for both redshift bins that the model predictions match well the source density we have measured from the SERVS data.…”
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The influence of environment on galaxy formation by Brunino, Riccardo

“…Using the outputs of the MILLENNIUM simulation and the relative Semi Analytical galaxy catalogues produced by Croton et al. 2006, we developed an algorithm aimed at the identification of large spherical underdense regions in the simulated Large Scale Structure (LSS), at z = 0. …”
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Galaxy evolution in protoclusters by Muldrew, Stuart I., Hatch, Nina A., Cooke, Elizabeth A.

“…We investigate galaxy evolution in protoclusters using a semi-analytic model applied to the Millennium Simulation, scaled to a Planck cosmology. We show that the model reproduces the observed behaviour of the star formation history (SFH) both in protoclusters and the field. …”
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What are protoclusters? – Defining high-redshift galaxy clusters and protoclusters by Muldrew, Stuart I., Hatch, Nina A., Cooke, Elizabeth A.

“…We explore the structures of protoclusters and their relationship with high-redshift clusters using the Millennium Simulation combined with a semi-analytic model. …”
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The structure and evolution of a forming galaxy cluster at z = 1.62 by Hatch, Nina A., Muldrew, Stuart I., Cooke, Elizabeth A., Hartley, William G., Almaini, O., Simpson, C.J., Conselice, Christopher J.

“…The structure of the protocluster reveals how much mass is available for the future growth of the cluster and we use the Millennium Simulation, scaled to a Planck cosmology, to predict that Cl 0218.3−0510 will evolve into a 2.7+3.9 −1.7 × 1014M cluster by the present day.…”
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Gravitational-wave limits from pulsar timing constrain supermassive black hole evolution by Shannon, R., Ravi, V., Coles, W., Hobbs, G., Keith, M., Manchester, R., Wyithe, J., Bailes, M., Bhat, Ramesh, Burke-Spolaor, S., Khoo, J., Levin, Y., Oslowski, S., Sarkissian, J., van Straten, W., Verbiest, J., Wang, J.-B.

“…For example, the standard galaxy formation model implemented in the Millennium simulations is inconsistent with our limit with 50% probability.…”
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