New Constraints on variations of the fine structure constant from CMB anisotropies (2009)
Menegoni, Eloisa, Galli, Silvia, Bartlett, James, Melchiorri, Alessandro
We demonstrate that recent measurements of Cosmic Microwave Background temperature and polarization anisotropy made by the ACBAR, QUAD and BICEP experiments substantially improve the cosmological...
Observing the Evolution of the Universe (2009)
Aguirre, James, Amblard, Alexandre, Ashoorioon, Amjad, Baccigalupi, Carlo, Balbi, Amedeo, Bartlett, James, ...
How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the universe. Through detailed...
Constraints On Cosmological Parameters From Current Cmb Data (2007)
James Bartlett, Alain Blanchard, Marian Douspis, Morvan Le Dour
. We discuss the constraints one can place on cosmological parameters using current cosmic microwave background data. A standard Ø 2 -- minimization over band--power estimates is first presented,...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien C., Lumb, David H., Bartlett, James, Romer, A. K., ...
We study the gas mass fraction, $f\_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f\_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien, Lumb, David, Bartlett, James, Romer, A.K., ...
We study the gas mass fraction, $f_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien, Lumb, David, Bartlett, James, Romer, A.K., ...
We study the gas mass fraction, $f_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien, Lumb, David, Bartlett, James, Romer, A.K., ...
We study the gas mass fraction, $f_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien, Lumb, David, Bartlett, James, Romer, A.K., ...
We study the gas mass fraction, $f_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters (2005)
Sadat, Rachida, Blanchard, Alain, Vauclair, Sebastien, Lumb, David, Bartlett, James, Romer, A.K., ...
We study the gas mass fraction, $f_{\rm gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f_{\rm gas}$ shape of high redshift galaxy clusters follows the global shape inferred at low...
Cosmological implications from the observed properties ofCMB. (2003)
Blanchard, Alain, Bartlett, James, Douspis, Marian
Observations of the cosmic microwave background represent a remarkable source of information for modern cosmology. Besides providing impressive support for the Big Bang model itself, they quantify...
Cosmological implications from the observed properties of CMB. (2003)
Blanchard, Alain, Bartlett, James, Douspis, Marian
Observations of the cosmic microwave background represent a remarkable source of information for modern cosmology. Besides providing impressive support for the Big Bang model itself, they quantify...
Cosmological implications from the observed properties of CMB. (2003)
Blanchard, Alain, Bartlett, James, Douspis, Marian
Observations of the cosmic microwave background represent a remarkable source of information for modern cosmology. Besides providing impressive support for the Big Bang model itself, they quantify...
Cosmological implications from the observed properties of CMB. (2003)
Blanchard, Alain, Bartlett, James, Douspis, Marian
Observations of the cosmic microwave background represent a remarkable source of information for modern cosmology. Besides providing impressive support for the Big Bang model itself, they quantify...
Cosmological implications from the observed properties of CMB. (2003)
Blanchard, Alain, Bartlett, James, Douspis, Marian
Observations of the cosmic microwave background represent a remarkable source of information for modern cosmology. Besides providing impressive support for the Big Bang model itself, they quantify...