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Documents CHALLENGES OF RELATIVISTIC ASTROPHYSICS Reuven Opher (Univ. of Sao Paulo/Cornell. Univ.)

Slide 1 CHALLENGES OF RELATIVISTIC ASTROPHYSICS Reuven Opher (Univ. of Sao Paulo/Cornell. Univ.) Slide 2 WHAT ARE THE BIGGEST PROBLEMS THAT NEED TO BE SOLVED IN RELATIVISTIC…

Documents Photometric Redshifts in Astro-Wise PhotRedCatalog Astro-Wise Workshop Leiden 2008 Jan Snigula, MPE.

Slide 1Photometric Redshifts in Astro-Wise PhotRedCatalog Astro-Wise Workshop Leiden 2008 Jan Snigula, MPE Slide 2 Introduction Photometric redshifts deducing redshifts from…

Documents Cosmological Constraints from the maxBCG Cluster Sample

Cosmological Constraints from the maxBCG Cluster Sample Eduardo Rozo October 12, 2006 In collaboration with: Risa Wechsler, Benjamin Koester, Timothy McKay, August Evrard,…

Documents The formation of galactic disks An overview of Mo Mao & White 1998 MNRAS 295 319.

The formation of galactic disks An overview of Mo Mao & White 1998 MNRAS 295 319 Introduction Disk formation in hierarchical cosmogonies Two component theory: dark matter…

Documents What can we learn from the luminosity function and color studies? THE SDSS GALAXIES AT REDSHIFT 0.1.

The sdss galaxies at redshift 0.1 What can we learn from the luminosity function and color studies? The sdss galaxies at redshift 0.1 1 OUTline Scientific Questions SDSS…

Documents Ay 123 Lecture 11 - Supernovae & Neutron Stars

Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster.. Structure of Massive Star at End of HS Burning Delayed Explosions Neutrino…

Documents The Fate of the Universe. The cosmological principle The simplest universes is: Homogenous – the.....

The Fate of the Universe The cosmological principle The simplest universes is: Homogenous â the same everywhere you go Isotropic â the same in all directions Discussion…

Documents Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster..

Ay 123 Lecture 11 - Supernovae & Neutron Stars Timescales for HS Burning faster and faster.. Structure of Massive Star at End of HS Burning Neutrinos Arrive from SN1987A…

Documents Impact of Early Dark Energy on non-linear structure formation

Impact of Early Dark Energy on non-linear structure formation Margherita Grossi MPA, Garching Advisor : Volker Springel 3rd Biennial Leopoldina Conference on Dark Energy…

Documents The sdss galaxies at redshift 0.1

The sdss galaxies at redshift 0.1 What can we learn from the luminosity function and color studies? The sdss galaxies at redshift 0.1 1 OUTline Scientific Questions SDSS…