Instrumentation for the detection and characterization of exoplanets

被引：73

作者：

Pepe, Francesco ^{[1
]}

Ehrenreich, David ^{[1
]}

Meyer, Michael R. ^{[2
]}

机构：

[1] Univ Geneva, Astron Observ, CH-1290 Versoix, Switzerland

[2] Swiss Fed Inst Technol, Inst Astron, CH-8093 Zurich, Switzerland

来源：

NATURE | 2014年 / 513卷 / 7518期

基金：

瑞士国家科学基金会;

关键词：

INFRARED TRANSMISSION SPECTROSCOPY; TELESCOPE IMAGING SPECTROGRAPH; RADIAL-VELOCITY CONFIRMATION; TIME-SERIES PHOTOMETRY; LASER FREQUENCY COMB; EXTRA-SOLAR PLANETS; FIELD CAMERA 3; HIGH-RESOLUTION; HD; 189733B; ORBITAL MOTION;

D O I：

10.1038/nature13784

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

In no other field of astrophysics has the impact of new instrumentation been as substantial as in the domain of exoplanets. Before 1995 our knowledge of exoplanets was mainly based on philosophical and theoretical considerations. The years that followed have been marked, instead, by surprising discoveries made possible by high-precision instruments. Over the past decade, the availability of new techniques has moved the focus of research from the detection to the characterization of exoplanets. Next-generation facilities will produce even more complementary data that will lead to a comprehensive view of exoplanet characteristics and, by comparison with theoretical models, to a better understanding of planet formation.

引用

页码：358 / 366

页数：9

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