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Professor Carlos Frenk's Outputs (19)

Large-scale structure from 2dFGRS (2005)
Presentation / Conference Contribution
Peacock, J., Colless, M., Baldry, I., Baugh, C., Bland-Hawthorn, J., Bridges, T., Cannon, R., Cole, S., Collins, C., Couch, W., Dalton, G., De Propris, R., Driver, S., Efstathiou, G., Ellis, R., Frenk, C., Glazebrook, K., Jackson, C., Lahav, O., Lewis, I., …Taylor, K. (2005, December). Large-scale structure from 2dFGRS

Effects of feedback on the morphology of galaxy discs (2005)
Journal Article
Okamoto, T., Eke, V., Frenk, C., & Jenkins, A. (2005). Effects of feedback on the morphology of galaxy discs. Monthly Notices of the Royal Astronomical Society, 363(4), 1299-1314. https://doi.org/10.1111/j.1365-2966.2005.09525.x

We have performed hydrodynamic simulations of galaxy formation in a cold dark matter (ΛCDM) universe. We have followed galaxy formation in a dark matter halo, chosen to have a relatively quiet recent merger history, using different models for star fo... Read More about Effects of feedback on the morphology of galaxy discs.

Theoretical models of the halo occupation distribution : separating central and satellite galaxies (2005)
Journal Article
Zheng, Z., Berlind, A., Weinberg, D., Benson, A., Baugh, C., Cole, S., …Lacey, C. (2005). Theoretical models of the halo occupation distribution : separating central and satellite galaxies. Astrophysical Journal, 633(2), 791-809. https://doi.org/10.1086/466510

The halo occupation distribution (HOD) describes the relation between galaxies and dark matter at the level of individual dark matter halos. The properties of galaxies residing at the centers of halos differ from those of satellite galaxies because o... Read More about Theoretical models of the halo occupation distribution : separating central and satellite galaxies.

The first generation of star-forming haloes. (2005)
Journal Article
Reed, D., Bower, R., Frenk, C., Gao, L., Jenkins, A., Theuns, T., & White, S. (2005). The first generation of star-forming haloes. Monthly Notices of the Royal Astronomical Society, 363(2), 393-404. https://doi.org/10.1111/j.1365-2966.2005.09416.x

We model gas cooling in high-resolution N-body simulations in order to investigate the formation of the first generation of stars. We follow a region of a Lambda cold dark matter (ΛCDM) universe especially selected to contain a rich cluster by the pr... Read More about The first generation of star-forming haloes..

The distribution of satellite galaxies: the great pancake. (2005)
Journal Article
Libeskind, N. I., Frenk, C. S., Cole, S., Helly, J. C., Jenkins, A., Navarro, J. F., & Power, C. (2005). The distribution of satellite galaxies: the great pancake. Monthly Notices of the Royal Astronomical Society, 363(1), 146-152. https://doi.org/10.1111/j.1365-2966.2005.09425.x

The 11 known satellite galaxies within 250 kpc of the Milky Way lie close to a great circle on the sky. We use high-resolution N-body simulations of galactic dark matter haloes to test if this remarkable property can be understood within the context... Read More about The distribution of satellite galaxies: the great pancake..

The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey (2005)
Journal Article
Hilton, M., Collins, C., De Propris, R., Baldry, I., Baugh, C., Bland-Hawthorn, J., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey. Monthly Notices of the Royal Astronomical Society, 363(2), 661-674. https://doi.org/10.1111/j.1365-2966.2005.09470.x

The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest, homogeneous X-ray selected cluster catalogue and completed g... Read More about The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey.

Early structure in Lambda CDM (2005)
Journal Article
Gao, L., White, S., Jenkins, A., Frenk, C., & Springel, V. (2005). Early structure in Lambda CDM. Monthly Notices of the Royal Astronomical Society, 363(2), 379-392. https://doi.org/10.1111/j.1365-2966.2005.09509.x

We use a novel technique to simulate the growth of one of the most massive progenitors of a supercluster region from redshift z 80, when its mass was about 10 M, until the present day. Our nested sequence of N-body resimulations allows us to study in... Read More about Early structure in Lambda CDM.

The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications (2005)
Journal Article
Cole, S., Percival, W., Peacock, J., Norberg, P., Baugh, C., Frenk, C., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications. Monthly Notices of the Royal Astronomical Society, 362(2), 505-534. https://doi.org/10.1111/j.1365-2966.2005.09318.x

We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We investigate in detail the modelling of the sample selecti... Read More about The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications.

Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters (2005)
Journal Article
Angulo, R., Baugh, C., Frenk, C., Bower, R., Jenkins, A., & Morris, S. (2005). Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters. Monthly Notices of the Royal Astronomical Society, 362(1), L25-L29. https://doi.org/10.1111/j.1745-3933.2005.00067.x

Acoustic oscillations in the baryon–photon fluid leave a signature in the matter power spectrum. The overall shape of the spectrum and the wavelength of the oscillations depend upon the sound horizon scale at recombination. Using the Λ cold dark matt... Read More about Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters.

Simulations of the formation, evolution and clustering of galaxies and quasars (2005)
Journal Article
Springel, V., White, S., Jenkins, A., Frenk, C., Yoshida, N., Gao, L., …Pearce, F. (2005). Simulations of the formation, evolution and clustering of galaxies and quasars. Nature, 435(7042), 629-636. https://doi.org/10.1038/nature03597

The cold dark matter model has become the leading theoretical picture for the formation of structure in the Universe. This model, together with the theory of cosmic inflation, makes a clear prediction for the initial conditions for structure formatio... Read More about Simulations of the formation, evolution and clustering of galaxies and quasars.

The metal enrichment of the intracluster medium in hierarchical galaxy formation models (2005)
Journal Article
Nagashima, M., Lacey, C., Baugh, C., Frenk, C., & Cole, S. (2005). The metal enrichment of the intracluster medium in hierarchical galaxy formation models. Monthly Notices of the Royal Astronomical Society, 358(4), 1247-1266. https://doi.org/10.1111/j.1365-2966.2005.08766.x

We investigate the metal enrichment of the intracluster medium (ICM) within the framework of hierarchical models of galaxy formation. We calculate the formation and evolution of galaxies and clusters using a semi-analytical model which includes the e... Read More about The metal enrichment of the intracluster medium in hierarchical galaxy formation models.

The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations (2005)
Journal Article
Wild, V., Peacock, J., Lahav, O., Conway, E., Maddox, S., Baldry, I., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations. Monthly Notices of the Royal Astronomical Society, 356(1), 247-269. https://doi.org/10.1111/j.1365-2966.2004.08447.x

It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complicates the inference of cosmological parameters from galaxy redshift surveys, and is a challenge to theories of galaxy formation and evolution. In this p... Read More about The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations.

The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type (2005)
Journal Article
Croton, D., Farrar, G., Norberg, P., Colless, M., Peacock, J., Baldry, I., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type. Monthly Notices of the Royal Astronomical Society, 356(3), 1155-1167. https://doi.org/10.1111/j.1365-2966.2004.08546.x

We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8 h−1 Mpc, and on spectral type, determined from principal componen... Read More about The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type.

The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type (2005)
Journal Article
Conway, E., Maddox, S., Wild, V., Peacock, J., Hawkins, E., Norberg, P., …Taylor, K. (2005). The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type. Monthly Notices of the Royal Astronomical Society, 356(2), 456-474. https://doi.org/10.1111/j.1365-2966.2004.08446.x

We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which quantifies the spectral type of galaxies in the survey... Read More about The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type.

Can the faint submillimetre galaxies be explained in the Λ cold dark matter model? (2005)
Journal Article
Baugh, C., Lacey, C., Frenk, C., Granato, G., Silva, L., Bressan, A., …Cole, S. (2005). Can the faint submillimetre galaxies be explained in the Λ cold dark matter model?. Monthly Notices of the Royal Astronomical Society, 356(3), 1191-1200. https://doi.org/10.1111/j.1365-2966.2004.08553.x

We present predictions for the abundance of submillimetre galaxies (SMGs) and Lyman-break galaxies (LBGs) in the Λ cold dark matter cosmology. A key feature of our model is the self-consistent calculation of the absorption and emission of radiation b... Read More about Can the faint submillimetre galaxies be explained in the Λ cold dark matter model?.