'Sed fitting' diaporamas de présentation

The GRAMS Evolved Star Mass-Loss Models: CMDs, CCDs, and Stellar Population Analysis for the LMC

The GRAMS Evolved Star Mass-Loss Models: CMDs, CCDs, and Stellar Population Analysis for the LMC. Benjamin Sargent Collaborators: S. Srinivasan, M. Meixner, SAGE, and SAGE-Spec teams Mass-Loss Return from Stars to Galaxies Workshop May 20, 2010.

279 views • 15 slides

The GRAMS Evolved Star Mass-Loss Models: CMDs, CCDs, and Stellar Population Analysis for the LMC

The GRAMS Evolved Star Mass-Loss Models: CMDs, CCDs, and Stellar Population Analysis for the LMC. Benjamin Sargent Collaborators: S. Srinivasan, M. Meixner, SAGE, and SAGE-Spec teams Mass-Loss Return from Stars to Galaxies Workshop May 20, 2010.

155 views • 15 slides

EZ and GOSSIP Two new VO compliant tools for spectral analysis

EZ and GOSSIP Two new VO compliant tools for spectral analysis. Paolo Franzetti & the PANDORA Group - IASF Milano 22/3/2007. PANDORA Group. http://cosmos.iasf-milano.inaf.it/pandora. PANDORA Group. EZ. EZ: Easy-Z

154 views • 15 slides

First Unbiased Estimates of the Metallicity and Star-Formation Activity of Lyman Alpha Emitters

First Unbiased Estimates of the Metallicity and Star-Formation Activity of Lyman Alpha Emitters. Kimihiko Nakajima ( U. Tokyo ) - Co-Investigators - Masami Ouchi, Kazuhiro Shimasaku, Yoshiaki Ono (U. Tokyo) , J. Lee(Carnegie), C. Ly(STScI), D. Dale(U. Wyoming),

204 views • 13 slides

Bringing order to chaos New data-mining techniques for new surveys

232 views • 10 slides

Bringing order to chaos New data-mining techniques for new surveys

102 views • 10 slides

SED OF NORMAL GALAXIES

207 views • 1 slides