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Instrumentation for the detection and characterization of exoplanets

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arxiv 1409.5266 v1 pith:K5WCWG57 submitted 2014-09-18 astro-ph.EP astro-ph.IM

classification astro-ph.EPastro-ph.IM
keywords exoplanetsbeencharacterizationdetectioninstrumentationtheoreticalwillastrophysics
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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 about exoplanets was mainly based on philosophical and theoretical considerations. The following years have been marked, instead, by surprising discoveries made possible by high-precision instruments. More recently the availability of new techniques moved the focus from 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.

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Cited by 1 Pith paper

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  1. NuAncestor: an artificial satellite-borne star for accurate frequency calibration of ground-based EPRV spectrographs

    astro-ph.IM 2025-07 unverdicted novelty 6.0 of 10

    A concept for a satellite-borne optical frequency comb that would provide a universal absolute calibration source for precision radial-velocity spectrographs worldwide.

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