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rss_1.0 Otros recursos de Eisenstein, Daniel

Resultados 1 - 10 de 166 de Eisenstein, Daniel. (0,08 segundos)

Documentos:
1. (100%) Large-Scale Structure and Future Surveys - Eisenstein, Daniel
As the 2dF Galaxy Redshift Survey and Sloan Digital Sky Survey move toward completion, it is time to ...
- 26-jun-2007

2. (80%) Deprojecting Densities from Angular Cross-Correlations - Eisenstein, Daniel J.
I present a model-independent spherically symmetric density estimator to be used in the cross-correl ...
- 26-jun-2007

3. (80%) An Analytic Expression for the Growth Function in a Flat Universe with a Cosmological Constant - Eisenstein, Daniel J.
An analytic expression is given for the growth function for linear perturbations in a low-density un ...
- 27-jun-2007

4. (80%) Covariance of the One-Dimensional Mass Power Spectrum - Zhan, Hu; Eisenstein, Daniel
We analyse the covariance of the one-dimensional mass power spectrum along lines of sight. The covar ...
- 27-jun-2007

5. (80%) Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest - McDonald, Patrick; Eisenstein, Daniel
We explore the requirements for a Lyman-alpha forest (LyaF) survey designed to measure the angular d ...
- 27-jun-2007

6. (70%) Origin of Quasar Progenitors from the Collapse of Low-Spin Cosmological Perturbations - Eisenstein, Daniel J.; Loeb, Abraham
We show that seeds for quasar black holes could have originated from the initial cosmological collap ...
- 27-jun-2007

7. (70%) An Analytical Model for the Triaxial Collapse of Cosmological Perturbations - Eisenstein, Daniel J.; Loeb, Abraham
We present an analytical model for the non-spherical collapse of overdense regions out of a Gaussian ...
- 27-jun-2007

8. (70%) Probing Early Clustering with Lyman-Alpha Absorption Lines Beyond the Quasar Redshift - Loeb, Abraham; Eisenstein, Daniel J.
Groups and clusters of galaxies hosting a quasar can be found through the detection of Lyman-alpha a ...
- 27-jun-2007

9. (70%) Can the Tully-Fisher Relation be the Result of Initial Conditions? - Eisenstein, Daniel J.; Loeb, Abraham
We use Monte Carlo realizations of halo formation histories and a spherical accretion model to calcu ...
- 27-jun-2007

10. (70%) Baryonic Features in the Matter Transfer Function - Eisenstein, Daniel J.; Hu, Wayne
We provide scaling relations and fitting formulae for adiabatic cold dark matter cosmologies that ac ...
- 27-jun-2007

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