Cosmological Simulations on a Grid of Computers (2009)
Blaizot, Jeremy, Caron, Eddy, Courtois, Hélène, Depardon, Benjamin, Desprez, Frédéric
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations on a Grid of Computers (2009)
Blaizot, Jeremy, Caron, Eddy, Courtois, Hélène, Depardon, Benjamin, Desprez, Frédéric
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations on a Grid of Computers (2009)
Blaizot, Jeremy, Caron, Eddy, Courtois, Hélène, Depardon, Benjamin, Desprez, Frédéric
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations on a Grid of Computers (2009)
Depardon, Benjamin, Caron, Eddy, Desprez, Frédéric, Courtois, Hélène, Blaizot, Jeremy
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations on a Grid of Computers (2009)
Depardon, Benjamin, Caron, Eddy, Desprez, Frédéric, Courtois, Hélène, Blaizot, Jeremy
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations on a Grid of Computers (2009)
Depardon, Benjamin, Caron, Eddy, Desprez, Frédéric, Courtois, Hélène, Blaizot, Jeremy
The work presented in this paper aims at restricting the input parameter values of the semi-analytical model used in Galics and MoMaF, so as to derive which parameters influence the most the results,...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware. (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
(eng) Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware (2007)
Caniou, Yves, Caron, Eddy, Depardon, Benjamin, Courtois, Hélène, Teyssier, Romain
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
Cosmological Simulations using Grid Middleware (2007)
École Normale, Supérieure Lyon, Yves Caniou, Eddy Caron, Benjamin Depardon, Hélène Courtois, ...
Large problems ranging from numerical simulation can now be solved through the Internet using grid middleware. This report describes the different steps involved to make available a service in the...
The 3D skeleton of the SDSS (2006)
Sousbie, Thierry, Pichon, Christophe, Courtois, Hélène, Colombi, Stéphane, Novikov, Dmitri
The length of the three-dimensional filaments observed in the fourth public data-release of the SDSS is measured using the {\em local skeleton} method. It consists in defining the set of points where...
The abundance of Lyman-( \alpha ) emitters in hierarchical models (2005)
Le Delliou, Morgan, Lacey, Cedric, Baugh, Carlton M., Guiderdoni, Bruno, Bacon, Roland, Courtois, Hélène, ...
We present predictions for the abundance of Ly-$\alpha$ emitters in hierarchical structure formation models. We use the {\tt GALFORM} semi-analytical model to explore the impact on the predicted...
The abundance of Lyman-( \alpha ) emitters in hierarchical models (2005)
Le Delliou, Morgan, Lacey, Cedric, Baugh, Carlton M., Guiderdoni, Bruno, Bacon, Roland, Courtois, Hélène, ...
We present predictions for the abundance of Ly-$\alpha$ emitters in hierarchical structure formation models. We use the {\tt GALFORM} semi-analytical model to explore the impact on the predicted...
The abundance of Lyman-( \alpha ) emitters in hierarchical models (2005)
Le Delliou, Morgan, Lacey, Cedric, Baugh, Carlton M., Guiderdoni, Bruno, Bacon, Roland, Courtois, Hélène, ...
We present predictions for the abundance of Ly-$\alpha$ emitters in hierarchical structure formation models. We use the {\tt GALFORM} semi-analytical model to explore the impact on the predicted...
The abundance of Lyman-( \alpha ) emitters in hierarchical models (2005)
Le Delliou, Morgan, Lacey, Cedric, Baugh, Carlton M., Guiderdoni, Bruno, Bacon, Roland, Courtois, Hélène, ...
We present predictions for the abundance of Ly-$\alpha$ emitters in hierarchical structure formation models. We use the {\tt GALFORM} semi-analytical model to explore the impact on the predicted...
The abundance of Lyman-( \alpha ) emitters in hierarchical models (2005)
Le Delliou, Morgan, Lacey, Cedric, Baugh, Carlton M., Guiderdoni, Bruno, Bacon, Roland, Courtois, Hélène, ...
We present predictions for the abundance of Ly-$\alpha$ emitters in hierarchical structure formation models. We use the {\tt GALFORM} semi-analytical model to explore the impact on the predicted...
The LEDA galaxy distribution : I. Maps of the Local Universe (2004)
Courtois, Hélène, Paturel, Georges, Sousbie, Thierry, Sylos Labini, Francesco
In order to investigate the properties of large-scale structures of galaxies in the universe, we present an analysis of their spatial distribution at z$
The LEDA galaxy distribution : I. Maps of the Local Universe (2004)
Courtois, Hélène, Paturel, Georges, Sousbie, Thierry, Sylos Labini, Francesco
In order to investigate the properties of large-scale structures of galaxies in the universe, we present an analysis of their spatial distribution at z$
The LEDA galaxy distribution : I. Maps of the Local Universe (2004)
Courtois, Hélène, Paturel, Georges, Sousbie, Thierry, Sylos Labini, Francesco
In order to investigate the properties of large-scale structures of galaxies in the universe, we present an analysis of their spatial distribution at z$
The LEDA galaxy distribution : I. Maps of the Local Universe (2004)
Courtois, Hélène, Paturel, Georges, Sousbie, Thierry, Sylos Labini, Francesco
In order to investigate the properties of large-scale structures of galaxies in the universe, we present an analysis of their spatial distribution at z$