AstroWISE LC workshop 2008 VESUVIO/ beyond AstroWISE OmegaCEN NOVA – Kapteyn Institute – University Groningen 3 April 2008 VVvve VESUVIO/ beyond AstroWISE.
Stellar population results from NFPS: Age and Metallicity along the Red Sequence Russell Smith (Waterloo), Jenica Nelan (Dartmouth), Mike Hudson (Waterloo),
Lecture 21 Cosmological Models ASTR 340 Fall 2006 Dennis Papadopoulos.
Metal distribution in sloshing galaxy clusters: the case of A496
Stellar population results from NFPS: Age and Metallicity along the Red Sequence
COSMIC GAMMA-RAY BURSTS The Current Status
3C120 R. Craig Walker National Radio Astronomy Observatory Socorro, NM Collaborators: J.M. Benson, S.C. Unwin, M.B. Lystrup, T.R.Hunter, G. Pilbratt, P.E.
XMM-Newton observation of the distant (z 0.4) galaxy clusters: RX J2359.5-3211, RX J0858.7-1902 and RX J2202.7-1902 Sergey Anokhin, [email protected],
Making the most of the ISW effect Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto.
XMM-Newton observation of the distant ( z 0.4 ) galaxy clusters:
COSMIC GAMMA-RAY BURSTS The Current Status Kevin Hurley UC Berkeley Space Sciences Laboratory.
