Resolved Spectroscopy of a z = 5 Gravitationally Lensed Galaxy with the VIMOS IFU
(2005)
Journal Article
Swinbank, M., Bower, R., Smail, I., Morris, S., & Smith, G. (2005). Resolved Spectroscopy of a z = 5 Gravitationally Lensed Galaxy with the VIMOS IFU
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.xAcoustic 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.
Can a photometric redshift code reliably determine dust extinction? (2005)
Journal Article
Babbedge, T., Whitaker, R., & Morris, S. (2005). Can a photometric redshift code reliably determine dust extinction?. Monthly Notices of the Royal Astronomical Society, 361, 437-450. https://doi.org/10.1111/j.1365-2966.2005.09168.x
The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3 (2005)
Journal Article
Wilman, R., Gerssen, J., Bower, R., Morris, S., Bacon, R., de Zeeuw, P., & Davies, R. (2005). The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3. Nature, 436(7048), 227-229. https://doi.org/10.1038/nature03718High-velocity galactic outflows, driven by intense bursts of star formation and black hole accretion, are processes invoked by current theories of galaxy formation to terminate star formation in the most massive galaxies and to deposit heavy elements... Read More about The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3.
Galaxy groups at 0.3 \textless=z\textless= 0.55 - II. Evolution to z\textasciitilde 0 (2005)
Journal Article
Wilman, D., Balogh, M., Bower, R., Mulchaey, J., Oemler, A., Carlberg, R., …Whitaker, R. (2005). Galaxy groups at 0.3 \textless=z\textless= 0.55 - II. Evolution to z\textasciitilde 0. Monthly Notices of the Royal Astronomical Society, 358, 88-100
Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - I. Group properties. (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 - I. Group properties. Monthly Notices of the Royal Astronomical Society, 358(1), 71-87. https://doi.org/10.1111/j.1365-2966.2005.08744.xThe evolution of galaxies in groups may have important implications for the evolution of the star formation history of the Universe, since many processes which operate in groups may suppress star formation and the fraction of galaxies in bound groups... Read More about Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - I. Group properties..
The abundance of Lyα emitters in hierarchical models (2005)
Journal Article
Le Delliou, M., Lacey, C., Baugh, C., Guiderdoni, B., Bacon, R., Courtois, H., …Morris, S. (2005). The abundance of Lyα emitters in hierarchical models. Monthly Notices of the Royal Astronomical Society, 357(1), L11-L15. https://doi.org/10.1111/j.1745-3933.2005.00007.xWe present predictions for the abundance of Lyα emitters in hierarchical structure formation models. We use the GALFORM semi-analytical model of galaxy formation to explore the impact on the predicted counts of varying assumptions about the escape fr... Read More about The abundance of Lyα emitters in hierarchical models.