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