1.The Co-Evolution of Black Holes & Bulges:A Local Perspective2. COLLABORATORS G. Kauffmann – MPA (Garching) P. Best – ROE (Edinburgh) J. Brinchmann – CAUP (Portugal)…

Slide 1 Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen Slide 2 Background Galaxies are full of stars, and sometimes gas and dust too. Beyond just images…

Slide 1Data-Intensive Statistical Challenges in Astrophysics Alex Szalay The Johns Hopkins University Collaborators: T. Budavari, C-W Yip (JHU), M. Mahoney (Stanford), I.…

Slide 1Ching-Wa Yip Johns Hopkins University Slide 2  Alex Szalay (JHU)  Rosemary Wyse (JHU)  László Dobos (ELTE)  Tamás Budavári (JHU)  Istvan Csabai…

Slide 1 Andrew Humphrey INAOE Submitted to MNRAS Letters with M. Villar-Martín, S.F. Sánchez, A. Martínez-Sansigre, R. González Delgado, E. Pérez, C. Tadhunter, M.-A.…

The nuclear activity of late-type galaxies in the Virgo Cluster Roberto Decarli Università degli Studi di Milano – Bicocca Dipartimento di Fisica Santiago, September,…

Detection of the 2175Å Dust Extinction Feature at high z Junfeng Wang (Penn State/UFL) Collaborators: Jian Ge (U. of Florida), Pat Hall (Princeton U./York U.), Jason Prochaska…

Detection of the 2175Å Dust Extinction Feature at high z Junfeng Wang (Penn State/UFL) Collaborators: Jian Ge (U. of Florida), Pat Hall (Princeton U./York U.), Jason Prochaska…

High-redshift QSOs and Galaxies in the GOODS Pierluigi Monaco & Stefano Cristiani DAUT - University of Trieste INAF-Trieste Observatory S.Cristiani THE GOODS TEAM D.M.Alexander,…

The Kilo-Degree Survey Konrad Kuijken Leiden Observatory Survey parameters Area covered Median redshift Image quality Wavelength coverage area zmed U  K…