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Professor Carlton Baugh's Outputs (359)

A Wide-Field K-band Galaxy Survey: The Color and Surface Brightness Distribution of Nearby Galaxies (1997)
Journal Article
Gardner, J., Sharples, R., Frenk, C., Baugh, C., & Carrasco, B. (1997). A Wide-Field K-band Galaxy Survey: The Color and Surface Brightness Distribution of Nearby Galaxies. Bulletin of the American Astronomical Society, 29(2),

We present the results of a wide-field K band galaxy survey. We have imaged nearly 10 square degrees in two fields at high galactic latitude using linear detectors in the near-infrared K band and the optical B, V, and I bands. We have obtained spectr... Read More about A Wide-Field K-band Galaxy Survey: The Color and Surface Brightness Distribution of Nearby Galaxies.

Modelling Galaxy Formation at High Z (1997)
Presentation / Conference Contribution
Lacey, C., Baugh, C., Cole, S., & Frenk, C. (1997, December). Modelling Galaxy Formation at High Z

A Wide-Field K-band Galaxy Survey (1996)
Journal Article
Gardner, J., Sharples, R., Frenk, C., Baugh, C., & Carrasco, B. (1996). A Wide-Field K-band Galaxy Survey. Bulletin of the American Astronomical Society, 28(4),

We present the results of a wide-field K band galaxy survey. We have imaged nearly 10 square degrees in two fields at high galactic latitude using linear detectors in the near-infrared K band, and the optical B, V, and I bands. We have obtained spect... Read More about A Wide-Field K-band Galaxy Survey.

A comparison of the evolution of density fields in perturbation theory and numerical simulations - II. Counts-in-cells analysis. (1995)
Journal Article
Baugh, C., Gaztañaga, E., & Efstathiou, G. (1995). A comparison of the evolution of density fields in perturbation theory and numerical simulations - II. Counts-in-cells analysis. Monthly Notices of the Royal Astronomical Society, 274(4), 1049-1070. https://doi.org/10.1093/mnras/274.4.1049

We present a detailed comparison of the predictions of perturbation theory (PT) for the averaged J-point correlation functions, ξJξJ, with the results of numerical simulations of gravitational clustering. We carry out a systematic analysis of this me... Read More about A comparison of the evolution of density fields in perturbation theory and numerical simulations - II. Counts-in-cells analysis..

A comparison of the evolution of density fields in perturbation theory and numerical simulations – I. Non-linear evolution of the power spectrum. (1994)
Journal Article
Baugh, C., & Efstathiou, G. (1994). A comparison of the evolution of density fields in perturbation theory and numerical simulations – I. Non-linear evolution of the power spectrum. Monthly Notices of the Royal Astronomical Society, 270(1), 183-198. https://doi.org/10.1093/mnras/270.1.183

We present a detailed comparison of the predictions of second-order perturbation theory and numerical N-body simulations for the evolution of density fluctuations in a standard cold dark matter universe. The evolution of the power spectrum of density... Read More about A comparison of the evolution of density fields in perturbation theory and numerical simulations – I. Non-linear evolution of the power spectrum..