Be captivated by the exotic objects that populate the Radio Sky and gain a solid understanding of their physics and the fundamental techniques we use to observe them. The serendipitous and unexpected discovery of radio emission from celestial objects opened up the possibility of studying a new and exciting view of the universe beyond the visible spectrum. Astronomers have been studying the cosmos in visible light since ancient Greece, but it is only in comparatively modern times that the universe beyond the visible spectrum has become accessible to us. In this course you will learn about the most important objects that emit in the radio regime, both within and beyond our own galaxy.
Class Deals by MOOC List - Click here and see EdX's Active Discounts, Deals, and Promo Codes.
Covering topics from the birth and death of stars to the detection of Gravitational waves you will learn how radio observations contribute to a richer understanding of the universe we inhabit. This course also introduces the basics of radio detectors and the technologies we use to observe at radio wavelengths.
What you'll learn
- Gain an overview of Radio Astronomy and its context
- Understand the different detector technologies used at different wavelengths
- Learn the features of the main emission mechanisms which cause radio emission
- Characterise the different types of celestial radio emitters
- Use radio emission to diagnose key physical and scientific insights into the nature of the object being observed.
Syllabus
Week 1: An historical perspective of radio astronomy, followed by the description of the main objects in the universe that can be observed at radio wavelength.
Week 2: The basics of photon properties and propagation. Black-body emission and radiation transport.
Week 3: Description of the photon spectrum: continuum production and line physics.
Week 4: Basics of detection of photons. Detectors across the electromagnetic spectrum.
Week 5: The main objects that can be detected in the Universe at radio wavelength - first part.
Week 6: The main objects that can be detected in the Universe at radio wavelength - second part.
