Object Classification Using Infrared Photometry Techniques

This exam investigates the methodologies of infrared photometry for the classification of astronomical objects. It emphasizes the principles of light measurement and their application in distinguishing various celestial phenomena.

Infrared photometry is essential for categorizing astronomical objects based on their brightness, temperature, and distance. It supports a variety of applications, including the classification of stellar types, the assessment of exoplanet characteristics, and the analysis of active galactic nuclei.

During this exam, students will be evaluated on their ability to verbally articulate photometric techniques and their implications in object classification. They will demonstrate their understanding of how light measurements inform our knowledge of celestial bodies.

Candidates should review key methodologies, including photometric systems and reduction techniques, to effectively discuss the classification of objects based on their infrared emissions.