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Astroseismic data analysis: Foundatin and Techniques

By: Basu, Sarbani.
Contributor(s): Chaplin, William J.
Material type: materialTypeLabelBookSeries: Prinston Series in Modern observational astronomy. Publisher: New Jersey Princeton Press 2017Description: xii,337p. HB 10x7.ISBN: 9780691162928.Subject(s): Astrophysics | Astronomy | Cosmology | Research and MethodologyDDC classification: 522.8 Summary: Studies of stars and stellar populations, and the discovery and characterization of exoplanets, are being revolutionized by new satellite and telescope observations of unprecedented quality and scope. Some of the most significant advances have been in the field of asteroseismology, the study of stars by observation of their oscillations. Asteroseismic Data Analysis gives a comprehensive technical introduction to this discipline. This book not only helps students and researchers learn about asteroseismology; it also serves as an essential instruction manual for those entering the field. The book presents readers with the foundational techniques used in the analysis and interpretation of asteroseismic data on cool stars that show solar-like oscillations. The techniques have been refined, and in some cases developed, to analyze asteroseismic data collected by the NASA Kepler mission. Topics range from the analysis of time-series observations to extract seismic data for stars to the use of those data to determine global and internal properties of the stars. Reading lists and problem sets are provided, and data necessary for the problem sets are available online. The first book to describe in detail the different techniques used to analyze the data on stellar oscillations, Asteroseismic Data Analysis offers an invaluable window into the hearts of stars. Introduces the asteroseismic study of stars and the theory of stellar oscillations Describes the analysis of observational (time-domain) data Examines how seismic parameters are extracted from observations Explores how stellar properties are determined from seismic data Looks at the “inverse problem,” where frequencies are used to infer internal structures of stars
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Item type Current location Collection Call number Status Date due Barcode Item holds
Book Book Astronomy Book 522.8 Bas/Cha (Browse shelf) Checked out to Anwesh Mazumdar (17) 02/01/2020 25122
Book Book Astronomy 522.8 Bas/Cha (Browse shelf) Checked out to Pritesh Ranadive (141) 18/05/2019 24790
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Studies of stars and stellar populations, and the discovery and characterization of exoplanets, are being revolutionized by new satellite and telescope observations of unprecedented quality and scope. Some of the most significant advances have been in the field of asteroseismology, the study of stars by observation of their oscillations. Asteroseismic Data Analysis gives a comprehensive technical introduction to this discipline. This book not only helps students and researchers learn about asteroseismology; it also serves as an essential instruction manual for those entering the field.

The book presents readers with the foundational techniques used in the analysis and interpretation of asteroseismic data on cool stars that show solar-like oscillations. The techniques have been refined, and in some cases developed, to analyze asteroseismic data collected by the NASA Kepler mission. Topics range from the analysis of time-series observations to extract seismic data for stars to the use of those data to determine global and internal properties of the stars. Reading lists and problem sets are provided, and data necessary for the problem sets are available online.

The first book to describe in detail the different techniques used to analyze the data on stellar oscillations, Asteroseismic Data Analysis offers an invaluable window into the hearts of stars.

Introduces the asteroseismic study of stars and the theory of stellar oscillations
Describes the analysis of observational (time-domain) data
Examines how seismic parameters are extracted from observations
Explores how stellar properties are determined from seismic data
Looks at the “inverse problem,” where frequencies are used to infer internal structures of stars

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