R. Chris Smith, C. Aguilera, K. Krisciunas, N. B. Suntzeff (NOAO/CTIO), A. Becker, R. Covarrubias, A. Miceli, G. Miknaitis, A. Rest, C. Stubbs (U. Washington),
Radio and X-ray Properties of Magellanic Cloud - Chandra X-Ray ...
Yashar Akrami Modern Cosmology: Early Universe, CMB and LSS/ Benasque/ August 17, 2012 Postdoctoral Fellow Institute of Theoretical Astrophysics University.
SuperNova Acceleration Probe Research and Development Efforts Chris Bebek UC Berkeley Lawrence Berkeley National Laboratory.
Highlights of Cosmology Physics 114 Spring 2004 – S. Manly References and photo sources: Ned Wright wright/cosmolog.htmwright/cosmolog.htm.
NYSS-AAPT meeting SUNY - Brockport October 1, 2005 [email protected] manly/ Much ado about nothing: the 30 minute.
Cosmology with Galaxy Clusters Princeton University Zoltán Haiman Dark Energy Workshop, Chicago, 14 December 2001 Collaborators: Joe Mohr (Illinois) Gil.
University of Rochester July 28, 2005 [email protected] manly/main/manlyhome.htm Much ado about nothing: the.
the theoretical understanding of Type Ia Supernovae
NASA Update to the AAAC, Part 1: JDEM Concept Studies NRC’s Beyond Einstein Study SMD Science Plan Update Astronomy and Astrophysics Advisory Committee.
The measurement of q 0 If objects are observed at large distances of known brightness (standard candles), we can measure the amount of deceleration since.
