Outputs (4)

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.

Where are the stars? (2005)
Journal Article
Eke, V., Baugh, C., Cole, S., Frenk, C., King, H., & Peacock, J. (2005). Where are the stars?. Monthly Notices of the Royal Astronomical Society, 362, 1233-1246. https://doi.org/10.1111/j.1365-2966.2005.09384.x

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.

Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - II. Evolution to z ∼ 0. (2005)
Journal Article
Wilman, D., Balogh, M., Bower, R., Mulchaey, J., Oemler, A., Carlberg, R., …Whitaker, R. (2005). Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - II. Evolution to z ∼ 0. Monthly Notices of the Royal Astronomical Society, 358(1), 88-100. https://doi.org/10.1111/j.1365-2966.2005.08745.x

We compare deep Magellan spectroscopy of 26 groups at 0.3 ≤z≤ 0.55, selected from the Canadian Network for Observational Cosmology 2 field survey, with a large sample of nearby groups from the 2PIGG catalogue. We find that the fraction of group galax... Read More about Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - II. Evolution to z ∼ 0..