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),
Metal distribution in sloshing galaxy clusters: the case of A496
Stellar population results from NFPS: Age and Metallicity along the Red Sequence
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.
X-RAY GROUPS WITH CHANDRA AND XMM: MASS, ENTROPY AND AGN HEATING
OU & APO
