Precision Spectroscopy in Astrophysics: Proceedings of the ESO/Lisbon/Aveiro Conference held in Aveiro, Portugal, 11 - 15 September 2006
High-accuracy Doppler shift measurements and high-precision spectroscopy are primary techniques in the search for exo-planets. Further extremely interesting applications include the analysis of QSO absorption lines to determine the variability of physical constants and the analysis of the isotopic r...
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| Format: | Conference Paper |
| Language: | English |
| Published: |
Berlin, Heidelberg
Springer-Verlag Berlin Heidelberg
2008
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| Series: | ESO Astrophysics Symposia, European Southern Observatory
SpringerLink Bücher |
| Volumes / Articles: | Show Volumes / Articles. |
| DOI: | 10.1007/978-3-540-75485-5 |
| Subjects: | |
| Online Access: | Verlag, Volltext: https://doi.org/10.1007/978-3-540-75485-5 Resolving-System, lizenzpflichtig, Volltext: http://dx.doi.org/10.1007/978-3-540-75485-5 Cover: https://swbplus.bsz-bw.de/bsz278314163cov.jpg Einführung/Vorwort: https://swbplus.bsz-bw.de/bsz278314163vor.htm Inhaltsverzeichnis: https://swbplus.bsz-bw.de/bsz278314163inh.htm 
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| Author Notes: | ed. by Nuno C. Santos, Luca Pasquini, Alexandre C. M. Correia, Martino Romaniello |
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| 245 | 0 | 0 | |a Precision Spectroscopy in Astrophysics |b Proceedings of the ESO/Lisbon/Aveiro Conference held in Aveiro, Portugal, 11 - 15 September 2006 |c ed. by Nuno C. Santos, Luca Pasquini, Alexandre C. M. Correia, Martino Romaniello |
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| 505 | 8 | |a Front Matter; Lithium Isotopic Abundances in Stars; Lithium Isotopic Abundances in Old Stars; Accurate Quantitative Spectroscopy of OB Stars: the H, He and C Spectrum; High Resolution Spectroscopy of HgMn stars: A Time of Surprises; High-resolution Spectroscopy of Faint Stars with Transiting Planets; First Resolved Narrow Line Profiles in Ultracool Dwarfs; Physical Parameters of Evolved Stars in Clusters and in the Field from Line-depth Ratios; UVES and CRIRES Spectroscopy of AGB Stars: Technetium and the Third Dredge-up; Characterisation of the Ursa Major Group | |
| 505 | 8 | |a [C/O] Observations in Low-[Fe/H] Halo StarsOxygen Abundances in Metal-poor Stars, from [OI], OI and IR OH Lines; Sulphur Abundances in Metal-poor Stars; Isotopic Abundances of Eu, Ba, and Sm in Metal-Poor Stars; Gas-phase Deuterium Abundances, Near and Far; Comprehensive Abundance Measurements in Damped Lya, Systems; Molecular Hydrogen at High Redshift and the Variation with Time of the Electron-to-proton Mass Ratio, µ = me/mP; Spectroscopy of QSO Pairs; Small-scale Structure of High-redshift OVI Absorption Systems; Hot Halos around High-Redshift Galaxies | |
| 505 | 8 | |a Astrophysical Probes of Fundamental PhysicsRevisiting VLT/UVES Constraints on a Varying Fine-structure Constant; On the Variation of the Fine-structure Constant, and Precision Spectroscopy; High-Precision Measurements of .aa, from QSO Absorption Spectra; Probing Fundamental Constant Evolution with Redshifted OH Lines; A Molecular Probe of Dark Energy; Establishing Wavelength Standards in the near Infra-red: Th-Ar; Atomic Data for Astrophysics - Parameters, Precision, Priorities; Optimal Extraction of Echelle Spectra; Hydrodynamical Model Atmospheres and 3D Spectral Synthesis | |
| 505 | 8 | |a Intrinsic Lineshifts in Astronomical SpectraStudy of Line Bisectors and its Relation with Precise Radial Velocities in the Search for Extrasolar Planets; A Pan-Spectral Method of Abundance Determination; Spectroscopic Binary Mass Determination Using Relativity; Asteroseismology Across the HR Diagram; High-Precision Spectroscopy of Pulsating Stars; Mapping Atmospheric Motions in Classical and Type II Cepheids; Iron Abundances of Southern Double-mode Cepheids from High-resolution Echelle Spectroscopy; Radial Velocity Planet Detection using a Gas Absorption Cell | |
| 505 | 8 | |a Pushing Down the Limits of the Radial Velocity TechniqueTransiting Planets: Follow the FLAMES...; Planet Detection Around M Dwarfs: New Constraints on Planet Formation Models; Planets Around Giant Stars; Planets Around Active Stars; A Catalogue of Nearby Exoplanets; Determination of the Orbital Parameters of a System with N +1 Bodies using a Simple Fourier Analysis of the Data; Extrasolar Comets; Measuring Winds in Titan's Atmosphere with High-precision Doppler Velocimetry; The European Large Telescope and its Spectroscopic Instrumentation | |
| 505 | 8 | |a CRIRES: A High Resolution Infrared Spectrograph for ESO's VLT | |
| 520 | |a High-accuracy Doppler shift measurements and high-precision spectroscopy are primary techniques in the search for exo-planets. Further extremely interesting applications include the analysis of QSO absorption lines to determine the variability of physical constants and the analysis of the isotopic ratios of absorption lines both in stars and in QSOs, and the determination of stellar oscillations through radial velocity measurements. Since the use of high-precision/resolution spectroscopy is closely connected to the ability to collect a large number of photons, the scientific domains using this | ||
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