Zobrazeno 1 - 10
of 354
pro vyhledávání: '"Hatton, S."'
Publikováno v:
Mon.Not.Roy.Astron.Soc. 361 (2005) 369-384
High-resolution N-body re-simulations of 15 massive (10^{14}-10^{15} Msun) dark matter haloes have been combined with the hybrid galaxy formation model GalICS (Hatton et al. 2003), to study the formation and evolution of galaxies in clusters, within
Externí odkaz:
http://arxiv.org/abs/astro-ph/0502490
Publikováno v:
Mon.Not.Roy.Astron.Soc.352:571,2004
This paper illustrates how mock observational samples of high-redshift galaxies with sophisticated selection criteria can be extracted from the predictions of GALICS, a hybrid model of hierarchical galaxy formation that couples the outputs of large c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310071
Autor:
Blaizot, J., Wadadekar, Y., Guiderdoni, B., Colombi, S., Bertin, E., Bouchet, F. R., Devriendt, J. E. G., Hatton, S.
Publikováno v:
Mon.Not.Roy.Astron.Soc.360:159-175,2005
We present the Mock Map Facility, a powerful tool to generate mock catalogues or images from semi-analytically post-processed snapshots of cosmological N-body simulations. The paper describes in detail an efficient technique to create such mocks from
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309305
Publikováno v:
Proc. of `The Promise of FIRST' symposium, 12--15 December 2000, Toledo, Spain (G.L.Pilbratt, J.Cernicharo, A.M. Heras, T. Prusti, & R. Harris eds., ESA SP-460, 2001)
The next generation of submillimetre/millimetre instruments will provide us with a deeper insight into the mechanisms that rule galaxy formation. As the brightest starbursts are thought to be heavily obscured at optical wavelengths, the opening of th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0102086
Autor:
Hatton, S. J.
Recent results from a number of redshift surveys suggest that the Universe is well described by an inhomogeneous, fractal distribution on the largest scales probed. This distribution has been found to have fractal dimension, D, approximately equal to
Externí odkaz:
http://arxiv.org/abs/astro-ph/9906085
Autor:
Hatton, S. J., Cole, S.
Given the failure of existing models for redshift-space distortions to provide a highly accurate measure of the beta-parameter, and the ability of forthcoming surveys to obtain data with very low random errors, it becomes necessary to develop better
Externí odkaz:
http://arxiv.org/abs/astro-ph/9905186
Autor:
Hatton, S. J., Cole, S.
Publikováno v:
Mon.Not.Roy.Astron.Soc.296:10-20,1998
We use a set of large, high-resolution cosmological N-body simulations to examine the redshift-space distortions of galaxy clustering on scales of order 10-200h^{-1} Mpc. Galaxy redshift surveys currently in progress will, on completion, allow us to
Externí odkaz:
http://arxiv.org/abs/astro-ph/9707186
Akademický článek
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Akademický článek
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Autor:
Abbas, J. R., Bertram‐Ralph, E., Hatton, S., Garth, T., Doherty, C., Bruce, I. A., McGrath, B. A.
Publikováno v:
Anaesthesia Reports; Jan-Jun2024, Vol. 12 Issue 1, p1-8, 8p
