1. (100%) Observational Constraints on the Self Interacting Dark Matter Scenario and the Growth of Supermassive Black Holes - Hennawi, Joseph F.; Ostriker, Jeremiah P.
We consider the consequences of SIDM for a velocity dependent cross section per unit mass. Accretion ...
- 26-jun-2007

2. (100%) Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering - Hennawi, Joseph F.; Spergel, David N.
We study the potential of weak lensing surveys to detect clusters of galaxies, using a fast Particle ...
- 27-jun-2007

3. (100%) Statistics of Quasars Multiply Imaged by Galaxy Clusters - Hennawi, Joseph F.; Dalal, Neal; Bode, Paul
We compute the expected number of quasars multiply imaged by cluster size dark halos for current wid ...
- 27-jun-2007

4. (100%) Quasars Probing Quasars II: The Anisotropic Clustering of Optically Thick Absorbers around Quasars - Hennawi, Joseph F.; Prochaska, Jason X.
With close pairs of quasars at different redshifts, a background quasar sightline can be used to stu ...
- 27-jun-2007

5. (83%) Gravitational Radiation Evolution of Accreting Neutron Stars - Wagoner, Robert V.; Hennawi, Joseph F.; Liu, Jingsong
The gravitational-wave and accretion driven evolution of neutron stars in low mass X-ray binaries an ...
- 26-jun-2007

6. (83%) Beyond the Damping Tail: Cross-Correlating the Kinetic Sunyaev-Zel'dovich Effect with Cosmic Shear - Doré, Olivier; Hennawi, Joseph F.; Spergel, David N.
Secondary anisotropies of the CMB have the potential to reveal intricate details about the history o ...
- 26-jun-2007

7. (83%) Characterizing the Cluster Lens Population - Hennawi, Joseph F.; Dalal, Neal; Bode, Paul; Ostriker, Jeremiah P.
We present a detailed investigation into which properties of CDM halos make them effective strong gr ...
- 27-jun-2007

8. (83%) The SDSS-DR5 Survey for Proximate Damped Lya Systems - Prochaska, Jason X.; Hennawi, Joseph F.; Herbert-Fort, Stephane
a sample of 111 PDLAs, we measure the HI frequency distribution f(N), incidence, and gas mass density of ... density of PDLAs at z~3 is approximately twice that of intervening DLAs, but at z<2.5 and z>3.5 the f(N
- 27-jun-2007

9. (67%) Coincident, 100 kpc-scale damped Lyman alpha absorption towards a binary QSO: how large are galaxies at z ~ 3? - Ellison, Sara L.; Hennawi, Joseph F.; Martin, Crystal L.; Sommer-Larsen, Jesper
the DLA at z = 2.94 we also infer an approximately solar ratio of alpha-to-Fe peak elements from [S ... of log f(H_2)< -5.5.
- 25-jun-2007

10. (67%) The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1 - Coil, Alison L.; Hennawi, Joseph F.; Newman, Jeffrey A.; Cooper, Michael C.; Davis, Marc
We present the clustering of DEEP2 galaxies at 0.7...
- 27-jun-2007

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