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Universidad de Cantabria Departamen
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A mis padres
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explicar las altas luminosidades de
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Además, una importante fracción (
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ealizar estudios de espectroscopía
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distribución diferencial que, al e
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materia sobre el agujero negro cent
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analizadas proviene de fuentes en t
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Haciendo uso del segundo catálogo
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With magic, you can turn a frog int
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Un capítulo aparte merecen mis com
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Summary Since its discovery more th
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xxxiv
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CONTENTS 1.6.1 The K-correction . .
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CONTENTS 5.3.2 Analytical model . .
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LIST OF FIGURES 4.6 Soft 1 − P µ
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Chapter 1 Introduction In the last
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CHAPTER 1: INTRODUCTION have confir
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CHAPTER 1: INTRODUCTION by this mis
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CHAPTER 1: INTRODUCTION Figure 1.2
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CHAPTER 1: INTRODUCTION [161], [242
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CHAPTER 1: INTRODUCTION tant contri
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CHAPTER 1: INTRODUCTION to-noise ra
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CHAPTER 1: INTRODUCTION Compton up-
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CHAPTER 1: INTRODUCTION ([142]). It
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CHAPTER 1: INTRODUCTION (NLR) and i
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CHAPTER 1: INTRODUCTION optically c
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CHAPTER 1: INTRODUCTION ber of AGN
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CHAPTER 1: INTRODUCTION Figure 1.5
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CHAPTER 1: INTRODUCTION 1.7.3 The X
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CHAPTER 1: INTRODUCTION AGN are ess
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CHAPTER 1: INTRODUCTION subjects ma
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CHAPTER 2: AGN SURVEYS WITH XMM-New
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R R OQP ONM 40 Table 2.1: Continued
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Chapter 3 Source counts of the AXIS
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CHAPTER 3: SOURCE COUNTS OF THE AXI
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61 Table 3.1 Maximum likelihood fit
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CHAPTER 4: CLUSTERING OF AXIS AND X
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