Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
- G. Hütsi
DOIAbstract
In this paper we determine the constraints on cosmological parameters using the CMB data from the Wma
In this paper we determine the constraints on cosmological parameters using the CMB data from the Wma
We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000...
We use FRIIb radio galaxy redshift–angular size data to constrain cosmological parameters in a dark ...
International audienceAims. We examine the constraints that can be obtained on standard cold dark ma...
In this paper we determine the constraints on cosmological parameters using the CMB data from the Wm...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We derive constraints on cosmological parameters using the power spectrum of galaxy clustering measu...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We extract the galaxy density and momentum power spectra from a subset of early-type galaxies in the...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data ...
Aims. We examine the constraints that can be obtained on standard cold dark matter models from the m...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data ...
We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000...
We use FRIIb radio galaxy redshift–angular size data to constrain cosmological parameters in a dark ...
International audienceAims. We examine the constraints that can be obtained on standard cold dark ma...
In this paper we determine the constraints on cosmological parameters using the CMB data from the Wm...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We derive constraints on cosmological parameters using the power spectrum of galaxy clustering measu...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We extract the galaxy density and momentum power spectra from a subset of early-type galaxies in the...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the ...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data ...
Aims. We examine the constraints that can be obtained on standard cold dark matter models from the m...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data ...
We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000...
We use FRIIb radio galaxy redshift–angular size data to constrain cosmological parameters in a dark ...
International audienceAims. We examine the constraints that can be obtained on standard cold dark ma...
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