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Multi-Wavelength Astronomy
Radio Astronomy
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  • Multi-Wavelength Astronomy
    • Preamble
    • Introduction
    • History of Multiwavelength Astronomy
    • Why Multi-Wavelength Astronomy?
    • Radiative Processes
    • Radio Astronomy
    • Optical Astronomy
    • X-ray Detectors
    • $\gamma $-ray Telescopes and Introduction to Multiwavelength Blazar Observations
    • Multiwavelength Observing Campaigns of Blazars and Other AGN
Introduction
The Radio-Window in the Electromagnetic Spectrum, The Radio vs. the Optical Sky, The Birth of Radio Astronomy
Single-Dish Radio Telescopes
Overview, Parabolic Reflectors, Theory of Radio Antennas
21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I
Background, Measuring Galactic Structure and Dynamics, Demo: The Bamberg Small Radio Telescope
The biggest dishes
Arecibo, FAST
Radio Interferometry
The Two-Element Interferometer, Effects of Finite Bandwidth, Effects of Finite Source Size, The $u,v$-plane, Aperture Synthesis, Obtaining Images, Calibration of Interferometer Data, VLBI, Summary of Interferometer Theory, Demo: Virtual Radio Interferometer, Hybrid Imaging, The Quest for Angular Resolution
Applications of Radio Interferometry -- Example: Radio-Loud AGN
Radio Loud AGN -- Context, VLA Images of Radio Galaxies, Classification of Radio-Loud AGN, Flat-Spectrum Radio Sources: Blazars, Radio Spectra, Multifrequency VLBI Observations, Apparent Superluminal Motion, Relativistic Boosting, Jet One-Sidedness, Kinematics of Relativistic Jets
Future Projects of Radioastronomy
LOFAR, SKA
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Introduction: The Radio-Window in the Electromagnetic SpectrumIntroduction: The Radio-Window in the Electromagnetic SpectrumIntroduction: The Radio-Window in the Electromagnetic SpectrumIntroduction: The Radio-Window in the Electromagnetic Spectrum
Introduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical Sky
Introduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical SkyIntroduction: The Radio vs. the Optical Sky
Introduction: The Radio vs. the Optical SkyIntroduction: The Birth of Radio AstronomySingle-Dish Radio Telescopes: OverviewSingle-Dish Radio Telescopes: Parabolic Reflectors
Single-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic Reflectors
Single-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic Reflectors
Single-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Parabolic ReflectorsSingle-Dish Radio Telescopes: Theory of Radio AntennasSingle-Dish Radio Telescopes: Theory of Radio Antennas
Single-Dish Radio Telescopes: Theory of Radio AntennasSingle-Dish Radio Telescopes: Theory of Radio AntennasSingle-Dish Radio Telescopes: Theory of Radio AntennasSingle-Dish Radio Telescopes: Theory of Radio Antennas
Single-Dish Radio Telescopes: Theory of Radio Antennas21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Background21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Background21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Background
21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Measuring Galactic Structure and Dynamics21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Measuring Galactic Structure and Dynamics21\tmspace +\thinmuskip {.1667em}cm Line Observations of Galactic H\tmspace +\thinmuskip {.1667em}I: Demo: The Bamberg Small Radio TelescopeThe biggest dishes: Arecibo
The biggest dishes: AreciboThe biggest dishes: AreciboThe biggest dishes: AreciboThe biggest dishes: Arecibo
The biggest dishes: AreciboThe biggest dishes: AreciboThe biggest dishes: AreciboThe biggest dishes: Arecibo
The biggest dishes: FASTRadio Interferometry: The Two-Element InterferometerRadio Interferometry: The Two-Element InterferometerRadio Interferometry: The Two-Element Interferometer
Radio Interferometry: The Two-Element InterferometerRadio Interferometry: The Two-Element InterferometerRadio Interferometry: Effects of Finite BandwidthRadio Interferometry: Effects of Finite Bandwidth
Radio Interferometry: Effects of Finite Source SizeRadio Interferometry: Effects of Finite Source SizeRadio Interferometry: Effects of Finite Source SizeRadio Interferometry: Effects of Finite Source Size
Radio Interferometry: The $u,v$-planeRadio Interferometry: The $u,v$-planeRadio Interferometry: Aperture SynthesisRadio Interferometry: Aperture Synthesis
Radio Interferometry: Aperture SynthesisRadio Interferometry: Aperture SynthesisRadio Interferometry: Aperture SynthesisRadio Interferometry: Aperture Synthesis
Radio Interferometry: Aperture SynthesisRadio Interferometry: Aperture SynthesisRadio Interferometry: Obtaining ImagesRadio Interferometry: Obtaining Images
Radio Interferometry: Obtaining ImagesRadio Interferometry: Obtaining ImagesRadio Interferometry: Obtaining ImagesRadio Interferometry: Obtaining Images
Radio Interferometry: Calibration of Interferometer DataRadio Interferometry: VLBIRadio Interferometry: VLBIRadio Interferometry: VLBI
Radio Interferometry: VLBIRadio Interferometry: VLBIRadio Interferometry: VLBIRadio Interferometry: VLBI
Radio Interferometry: VLBIRadio Interferometry: Summary of Interferometer TheoryRadio Interferometry: Demo: Virtual Radio InterferometerRadio Interferometry: Demo: Virtual Radio Interferometer
Radio Interferometry: Hybrid ImagingRadio Interferometry: Hybrid ImagingRadio Interferometry: Hybrid ImagingRadio Interferometry: Hybrid Imaging
Radio Interferometry: Hybrid ImagingRadio Interferometry: The Quest for Angular ResolutionRadio Interferometry: The Quest for Angular ResolutionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Radio Loud AGN -- Context
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Radio Loud AGN -- ContextApplications of Radio Interferometry -- Example: Radio-Loud AGN: VLA Images of Radio GalaxiesApplications of Radio Interferometry -- Example: Radio-Loud AGN: VLA Images of Radio GalaxiesApplications of Radio Interferometry -- Example: Radio-Loud AGN: VLA Images of Radio Galaxies
Applications of Radio Interferometry -- Example: Radio-Loud AGN: VLA Images of Radio GalaxiesApplications of Radio Interferometry -- Example: Radio-Loud AGN: Classification of Radio-Loud AGNApplications of Radio Interferometry -- Example: Radio-Loud AGN: Classification of Radio-Loud AGNApplications of Radio Interferometry -- Example: Radio-Loud AGN: Classification of Radio-Loud AGN
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Classification of Radio-Loud AGNApplications of Radio Interferometry -- Example: Radio-Loud AGN: Classification of Radio-Loud AGNApplications of Radio Interferometry -- Example: Radio-Loud AGN: Flat-Spectrum Radio Sources: BlazarsApplications of Radio Interferometry -- Example: Radio-Loud AGN: Radio Spectra
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Radio SpectraApplications of Radio Interferometry -- Example: Radio-Loud AGN: Multifrequency VLBI ObservationsApplications of Radio Interferometry -- Example: Radio-Loud AGN: Multifrequency VLBI ObservationsApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal Motion
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal Motion
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal Motion
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Apparent Superluminal MotionApplications of Radio Interferometry -- Example: Radio-Loud AGN: Relativistic BoostingApplications of Radio Interferometry -- Example: Radio-Loud AGN: Relativistic BoostingApplications of Radio Interferometry -- Example: Radio-Loud AGN: Relativistic Boosting
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Jet One-SidednessApplications of Radio Interferometry -- Example: Radio-Loud AGN: Jet One-SidednessApplications of Radio Interferometry -- Example: Radio-Loud AGN: Kinematics of Relativistic JetsApplications of Radio Interferometry -- Example: Radio-Loud AGN: Kinematics of Relativistic Jets
Applications of Radio Interferometry -- Example: Radio-Loud AGN: Kinematics of Relativistic JetsFuture Projects of Radioastronomy: LOFARFuture Projects of Radioastronomy: SKAFuture Projects of Radioastronomy: SKA
Future Projects of Radioastronomy: SKAFuture Projects of Radioastronomy: SKA 
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Jörn Wilms / joern.wilms@sternwarte.uni-erlangen.de