. "Laboratory II: synthesis and characterization of advanced"@en . . "6" . "Specific Competition\nCE6 - Understand the structure of matter being able to solve problems related to the interaction between matter and radiation in different energy ranges\nCE7 - Know how to find solutions to specific astrophysical problems by themselves using specific bibliography with minimal supervision. Know how to function independently in a novel research project\nCE11 - Know how to use current astrophysical instrumentation (both in terrestrial and space observatories) especially that which uses the most innovative technology and know the fundamentals of the technology used\nGeneral Competencies\nCG2 - Understand the technologies associated with observation in Astrophysics and instrumentation design\nCG3 - Analyze a problem, study the possible published solutions and propose new solutions or lines of attack\nCG4 - Evaluate the orders of magnitude and develop a clear perception of physically different situations that show analogies allowing the use, to new problems, of synergies and known solutions\nBasic skills\nCB6 - Possess and understand knowledge that provides a basis or opportunity to be original in the development and/or application of ideas, often in a research context\nCB7 - That students know how to apply the knowledge acquired and their ability to solve problems in new or little-known environments within broader contexts\nCB10 - That students possess the learning skills that allow them to continue studying in a way that will be largely self-directed or autonomous\nExclusive to the Structure of Matter Specialty\nCX15 - Understand the state of degenerated systems and systems far from equilibrium\nCX18 - Apply physical and technical knowledge to extract experimental information from physical systems in laboratories.\n6. Subject contents\nTheoretical and practical contents of the subject\nTHEORETICAL CONTENTS:\n\n1.- Obtaining materials.\n- Mono and polycrystalline materials: Reaction in solid state. gel techniques.\n- Vitreous and nanostructured materials. Melt, sol-gel and solvothermal techniques. Doping with luminescent ions (rare earth).\n\n2.- Thermal stability and structural and microstructural characterization\n- Thermal Analysis. Infrared Spectroscopy. Electron Microscopy. X-ray diffraction.\n\n3.- Characterization of the properties of the materials.\n- Electrical properties: Dielectric Spectroscopy. Study of complex dielectric permittivity as a function of frequency and temperature.\n- Magnetic properties. Study of magnetic susceptibility as a function of temperature for different magnetic fields.\n- Optical properties: Photoluminescence and optical absorption. Energy transfer processes, conversion of infrared energy to UV-visible with photonic applications (telecommunications and renewable energies). Optical anisotropy.\n\nPRACTICAL CONTENTS:\n\nPractice 1: Obtaining and spectroscopic characterization of oxyfluoride nano-glass ceramics using melting techniques doped with rare earth ions for infrared to visible energy conversion applications (“up-conversion”).\n\nPractice 2: Obtaining and characterization of a sol-gel nano-glass ceramic doped with rare earth ions for applications in photon conversion processes.\n\nPractice 3: Obtaining solid state reaction and identification of phases in polycrystalline samples by X-ray diffraction (SEGAI).\n\nPractice 4: Analysis of crystalline powder diffractograms for their structural and microstructural characterization obtained in practice 3 and/or proposed by the teaching staff.\n\nPractice 5: Dielectric spectroscopy on polycrystalline samples obtained through the solid state reaction technique (practice 3).\n\nPractice 6: Characterization of thermal stability (thermal analysis), microstructure (electron microscopy) and molecular structure (infrared spectroscopy) of samples obtained in practices (1, 2 and 3). Such experiences will be carried out at SEGAI and the data will be analyzed in the subject laboratories.\n\nPractice 7: Magnetic characterization of materials (optional).\n\nPractice 8: Characterization of optical anisotropy in crystals (optional)." . . "Presential"@en . "FALSE" . . "Qualitative, Quantitative Research Skills"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Master in Astrophysics"@en . . "https://www.ull.es/en/masters/astrophysics/" . "90"^^ . "Presential"@en . "The exceptional atmospheric conditions for top-quality astronomic observation to be found in the Canary Islands, together with its geographic proximity and excellent connections with Europe, justify the presence here of the European Northern Hemisphere Observatory (ENO). This fact, along with the consequent concentration of teachers and researchers around the Canary Island Institute of Astrophysics, the ULL Department of Astrophysics and the Observatories, generates the ideal atmosphere for a Master in Astrophysics in which direct contact with leading professionals represents exceptional value added. The Master has been designed based on an ample and rigorous choice of subjects, options and itineraries that that take the form of three specialities: “Theory and Computing Speciality”, “Observation and Instrumentation Speciality” and “Material Structure”\n\nGeneral skills\nKnow the advanced mathematical and numerical techniques that allow Physics and Astrophysics to be applied to solving complex problems using simple models\nUnderstand the technologies associated with observation in Astrophysics and the design of instrumentation\nAnalyse a problem, study the possible solutions published and propose new solutions or lines of attack\nAssess orders of magnitude and develop a clear perception of physically different situations that show analogies allowing the use of synergies and known solutions for new problems\nSpecific skills\nUnderstand the basic conceptual schemes of Astrophysics\nUnderstand the structure and evolution of the stars\nUnderstand the mechanisms of nucleosynthesis\nUnderstand the structure and evolution of galaxies\nUnderstand the models of the origin and evolution of the Universe\nUnderstand the structure of matter to be able to solve problems related to the interaction between matter and radiation in different energy ranges\nKnow how to find solutions to specific astrophysical problems on your own, using specific bibliography with minimum supervision\nKnow how to work independently on new research projects\nKnow how to programme, at least in one important language for scientific calculation in Astrophysics\nUnderstand the instrumentation used to observe the universe in the different frequency ranges\nUse current scientific instrumentation (both Earth-based and Space-based) and have a command of their innovative technologies\nKnow how to use current astrophysical instrumentation (both in terrestrial and space observatories), especially the instrumentation that uses the most innovative technology and know the foundations of the technology used\nApply the knowledge acquired to undertake an original research work in Astrophysics"@en . . . "1.5"@en . "FALSE" . . . "Master"@en . "Thesis" . "Not informative" . "no data"@en . "Not informative" . "None" . "no data"@en . "no data" . "FALSE" . "Upstream"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .