. "Other Physics Kas"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Extragalactic physics"@en . . "6" . "Specific Competition\nCE1 - Understand the basic conceptual schemes of Astrophysics\nCE5 - Understand the models of the origin and evolution of the Universe\nGeneral Competencies\nCG1 - Know the advanced mathematical and numerical techniques that allow the application of Physics and Astrophysics to the solution of complex problems using simple models\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\nCB8 - That students are able to integrate knowledge and face the complexity of formulating judgments based on information that, being incomplete or limited, includes reflections on the social and ethical responsibilities linked to the application of their knowledge and judgments\nCB10 - That students possess the learning skills that allow them to continue studying in a way that will be largely self-directed or autonomous\n6. Subject contents\nTheoretical and practical contents of the subject\nProfessor: Jairo Méndez Abreu\nTopics:\n\n1. Introduction to galaxy observations\n - Introduction to the concept of galaxy \n - Physical units and basic equations\n - Basic principles of photometry and relationship between apparent and intrinsic quantities\n - Redshift, Hubble's law and distance measurements\n2 Photometric and morphological properties of galaxies\n - Hubble diagram (properties)\n - Modern classifications of galaxies\n - Galactic structures and formation of bulges, bars and disks\n - Photometric decompositions\n - Luminosity functions of galaxies.\n3. Kinematic and dynamical properties of galaxies\n - Determination of the kinematics of gas and stars
\n - Rotation curves and velocity dispersion in galaxies\n - Angular momentum of galaxies along the Hubble sequence\n4. Properties of the stellar populations of galaxies\n - History of star formation and populations simple stars\n - Synthesis of stellar populations\n 5. Observational characteristics of galaxies\n 5.1 Properties of spiral galaxies\n - Basic photometric and structural properties \n - Content in atomic, molecular and dust gas \n - Stellar populations \n - Scaling relationships \n 5.2. Properties of early type galaxies\n - Basic photometric and structural properties\n - Kinematic and dynamical properties\n - Stellar populations\n - Gas and dust\n - Scaling relationships\n6. Galaxy clusters \n - Main properties of galaxy clusters\n - Scaling relationships in galaxy clusters \n - Environment dependence on properties of galaxies \n - Evolution of galaxies in clusters\n - Pre-processing Professor: Arianna Di Cintio Topics: 7. Formation of structures and galaxies in the Universe - Large-scale structure - Formation of dark matter halos - Press-Schechter formalism\n \n\n\n\n\n \n\n\n - Properties of dark matter haloes\n - Hierarchical structure and internal structure of dark matter haloes (density profiles)\n - Baryon physics: gas cooling, star formation and feedback processes\n - Internal structure of galaxies and haloes in the presence of baryons (adiabatic contraction and expansion)\n8. Introduction to models of galaxy formation and large-scale structure \n - Theoretical models of galaxy formation \n - N-body simulations\n - Semi-analytical models -\n Hydrodynamic simulations\n - Galaxies in the Local Universe: Local Group Simulations\n - Problems of the standard cosmological model at the scale of Local Groups (\" missing satellite problem \", number and radial distribution of satellites, satellite density profiles, \" cusp-core \" problem)\n9. Active galactic nuclei (AGN)\n - Classification of types of AGN\n - Unified model and its improvements\n10. The Universe at high redshift\n - Galaxies at high redshift: morphology, kinematics, Lyman-break galaxies, Lyman-alpha emitters, ULIRG\n - Evolution of galactic properties with redshift \n - Evolution diagram Hubble\n - Evolution \"M-size relation\"\n - Evolution of the main sequence" . . "Presential"@en . "FALSE" . . "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 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .