Slide 1 Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly  = ionizing…

The Luminosity-Metallicity and Mass-Metallicity Relations of 0.4 Collaboration with Francois Hammer, Hector Flores, Francois Assemat at Paris-Meudon Observatory; David Elbaz,…

School/Workshop on parallel computing in astrophysics: 19-23 April, 2010, Santiago, Chile Closing remarks Data: large databases -> mining large sets of raw data ->…

1 [pre-print; final version forthcoming in Utilitas, no. 3, 2010] Being and Betterness Jens Johansson Stockholm University Abstract. In this paper I discuss the question…

High Redshift Radio Galaxies: The most massive galaxies up to z>5? Carlos De Breuck (ESO) [email protected] How massive are High-z Radio Galaxies (HzRGs)? Does their AGN…

Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly a = ionizing photons (dust…

Slide 1 [email protected], slide 1 German Aerospace CenterMicrowaves and Radar Institute Methodology for obtaining physical parameters from fully polarimetric coherent…

DATA WAREHOUSING AND DATA MINING S. Sudarshan Krithi Ramamritham IIT Bombay [email protected] [email protected] www.jntuworld.com www.jntuworld.com www.jwjobs.net…

pitch

DATA WAREHOUSING AND DATA MINING S. Sudarshan Krithi Ramamritham IIT Bombay [email protected] [email protected] www.jntuworld.com www.jntuworld.com www.jwjobs.net…