 Analysis of the diffuse near-IR emission from 2MASS deep integration data: foregrounds vs the cosmic infrared background |
| Analysis of the Diffuse Near-Infrared Emission from Two-Micron All-Sky Survey Deep Integration Data: Foregrounds versus the Cosmic Infrared Background |
| Clustering of Diffuse Infrared Background Light |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE maps. I. $C(0)$ and limits on the near-IR background |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE maps. III. Power spectrum analysis and excess isotropic component of fluctuations |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE maps. An all-sky survey of $C(0)$ |
| Clustering of DIRBE Light and IR Background |
| Clustering in COBE/DIRBE Maps and the Cosmic Infrared Background |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE Maps: an All-Sky Survey of C(0) |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE Maps. III. Power Spectrum Analysis and Excess Isotropic Component of Fluctuations |
| Clustering of Diffuse Infrared Background Light |
| Clustering of DIRBE Light and IR Background |
| Clustering of the Diffuse Infrared Light from the COBE DIRBE Maps. I. C(0) and Limits on the Near-Infrared Background |
| COBE Educational Resources (1993) |
| Constraints on the power spectrum of the primordial density field from large-scale data - Microwave background and predictions of inflation |
| Cosmic Infrared Background and clustering of the diffuse light in COBE/DIRBE maps |
| Determining cosmic microwave background structure from its peak distribution |
| Determining $\Omega$ from cluster correlation function |
| Detection of small scale fluctuations in the near-IR cosmic infrared background from long exposure 2MASS fields |
| Detection of Small-Scale Fluctuations in the Near-Infrared Cosmic Infrared Background from Long-Exposure 2MASS Fields |
| Determining Cosmic Microwave Background Structure from Its Peak Distribution |
| Determining Omega from the cluster correlation function |
| Dynamical friction and galaxy rotation - Should mergers lead to slow rotation? |
| Dynamical friction in rotating systems - Application to clusters and galaxies |
| Dynamical friction and evolution of the luminosity function in clusters of galaxies |
| Effects of mass segregation in rotating clusters of galaxies |
| Fluctuations in the near-IR cosmic infrared background from COBE DIRBE maps |
| Formation of cosmological hierarchies and constraints on the primordial power spectrum |
| Formation of galaxies in haloes |
| Formation and evolution of clusters of galaxies |
| Formation of population III stars and pregalactic evolution |
| Formation of elliptical and spiral galaxies in rotating haloes |
| Formation of Galaxies in Haloes |
| Galaxy Evolution, Deep Galaxy Counts and the Near-IR Cosmic Infrared Background |
| Galaxy Evolution, Deep Galaxy Counts, and the Near-Infrared Cosmic Infrared Background |
| Galaxy formation, clustering and the 'hidden mass' |
| Gravitational clustering and the origin of the correlation function of clusters of galaxies |
| Gravitational clustering of Gaussian density fluctuations and the origin of hierarchy correlations |
| High-z objects and cold-dark-matter cosmogonies: the case of 53W091 |
| High-z Objects and Cold-Dark-Matter Cosmogonies: the Case of 53W091 |
| High-z objects and cold dark matter cosmogonies - Constraints on the primordial power spectrum on small scales |
| Large-Scale Data, Microwave Background, and Inflation |
| Large-scale structure in the universe |
| Large scale peculiar velocities and gravitational clustering |
| Large-scale data, microwave background and inflation |
| Large-Scale Peculiar Velocities and Gravitational Clustering |
| Latest COBE results, large-scale structure and predictions of inflation |
| Latest COBE results, large-scale data, and predictions of inflation |
| Limits on the cosmic infrared background from clustering in COBE/DIRBE maps |
| Limits on the cosmic infrared background from clustering in COBE/DIRBE maps |
| Measuring cosmological bulk flows via the kinematic Sunyaev-Zeldovich effect in the upcoming cosmic microwave background maps |
| Measuring Cosmological Bulk Flows via the Kinematic Sunyaev-Zeldovich Effect in the Upcoming Cosmic Microwave Background Maps |
| Measuring Bulk Flows with the Kinematic Sunyaev-Zeldovich Effect in CMB Maps |
| Microwave backgropund anisotropies, large-scale structure and cosmological parameters |
| Microwave background anisotropy in low-$\Omega_0$ inflationary models and the scale of homogeneity in the Universe |
| Microwave background anisotropies implied by large-scale galaxy correlations - The minimum of C(0) and cosmological parameters |
| Microwave background anisotropy in low-Ù0 inflationary models and the scale of homogeneity in the Universe |
| Microwave background anisotropies, large scale structure and cosmological parameters |
| Modified Cold-Dark-Matter models in light of 53W091 an old galaxy at high z |
| Modified Cold-Dark Matter Models in Light of 53W091, an Old Galaxy at High Z |