Exoplanet Detection Methods offers a comprehensive exploration of techniques used to discover and study planets outside our solar system. The book emphasizes optical and spectroscopic methods, revealing how these tools bridge theoretical astrophysics with practical applications. Two pivotal methods discussed are transit photometry, which measures the dimming of a star's light as a planet passes in front of it, and radial velocity measurements, detecting the subtle wobble of a star caused by a planet's gravity. These methods are crucial, as combining them reveals a more complete picture of an exoplanet's characteristics.

The book progresses methodically, beginning with fundamental principles like stellar properties and planetary formation, then delving into specific detection techniques. It covers transit photometry, highlighting missions like Kepler and TESS, radial velocity measurements and direct imaging, including spectroscopic analysis of exoplanet atmospheres. A unique aspect of the book is its integration of theory with practical data analysis, making it valuable for students and researchers alike.

The book emphasizes that a complete understanding of exoplanet detection methods is essential to advance the study of planetary formation, habitability, and the possibility of life beyond Earth.