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Titlebook: An Introduction to Observational Astrophysics; Mark Gallaway Textbook 2020Latest edition Springer Nature Switzerland AG 2020 Astrometry In

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发表于 2025-3-21 18:02:23 | 显示全部楼层 |阅读模式
期刊全称An Introduction to Observational Astrophysics
影响因子2023Mark Gallaway
视频video
发行地址Covers all aspects of observational astrophysics for undergraduate students.Contains tested practicals to help students hone their skills.Includes expanded sections that cover the latest research and
学科分类Undergraduate Lecture Notes in Physics
图书封面Titlebook: An Introduction to Observational Astrophysics;  Mark Gallaway Textbook 2020Latest edition Springer Nature Switzerland AG 2020 Astrometry In
影响因子The observational component of astronomy is an exciting and vital part of any astrophysics degree. With the advent of low-cost astronomical cameras and remote and robotic operation, more students than ever have the opportunity to observe and perform observatory research. .This updated and fully corrected textbook provides a comprehensive overview of practical observing techniques for undergraduate astrophysics courses. The chapters introduce students to the basics of the field before delving into telescope types, the nature and operation of the astronomical camera, imaging techniques and reduction, photometry and spectrography, and solar and radio observations..The second edition covers the latest research on calibrating the telescope-camera-observatory system. It contains revised information on all available astronomy equipment, including filters, webcams, sensors, and telescope designs. Also included is an entirely new chapter on exoplanet transit measurements. The textbook’s practical approach will guide readers from basic first-year techniques to those required for a final-year project..
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The Telescope,ope is mounted, its limitations, and the accessories available to the astronomer. Furthermore, since on occasion, telescopes suffer from optical problems, we show how to identify such problems and to resolve them if possible.
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Spheres and Coordinates,torial coordinate systems to point telescopes and identify objects. The non-Euclidean nature of our observations means that we have to use spherical geometry when measuring the position of objects in the sky.
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