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Can we use nonlinear and selfconsistent models for data analysis? We learned from Prof. Schindler about the importance of nonlinear and selfconsistent.
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ACCRETION
Modeling the UV/EUV and its relevance for PROBA2 observations
Solar Irradiance Observations with LYRA on PROBA2 I. E. Dammasch , M. Dominique, J.-F. Hochedez
Active Galactic Nuclei Itziar Aretxaga, UPenn, April 2003 Lecture 1: Taxonomy and Unification Classification of AGN AGN vs other emission line galaxies.
