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Titolo:
Fundamental photon noise limit to radial velocity measurements
Autore:
Bouchy, F; Pepe, F; Queloz, D;
Indirizzi:
Observ Geneva, CH-1290 Sauverny, Switzerland Observ Geneva Sauverny Switzerland CH-1290 CH-1290 Sauverny, Switzerland
Titolo Testata:
ASTRONOMY & ASTROPHYSICS
fascicolo: 2, volume: 374, anno: 2001,
pagine: 733 - 739
SICI:
1432-0746(200108)374:2<733:FPNLTR>2.0.ZU;2-Q
Fonte:
ISI
Lingua:
ENG
Soggetto:
EXTRA-SOLAR PLANETS; COOL STARS; SPECTROGRAPH; ACCELEROMETRY; PRECISION; SPECTRA; SEARCH;
Keywords:
techniques : radial velocities; instrumentation : spectrographs; stars : oscillations; stars : planetary systems;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
25
Recensione:
Indirizzi per estratti:
Indirizzo: Bouchy, F Observ Geneva, 51 Ch Maillettes, CH-1290 Sauverny, Switzerland Observ Geneva 51 Ch Maillettes Sauverny Switzerland CH-1290 and
Citazione:
F. Bouchy et al., "Fundamental photon noise limit to radial velocity measurements", ASTRON ASTR, 374(2), 2001, pp. 733-739

Abstract

In the past 5 years, improvements in radial velocity measurements have ledto discovery of extra-solar planets and progress in asteroseismology programs. Doppler measurements with high precision is close to the limit given by photon noise. In this paper the methodology to compute the fundamental limit of radial velocity measurement given by photon noise is presented and illustrated with a representative sample of synthetic solar-type stellar spectra. Stellar rotational broadening, instrumental spectral range as well asspectral resolution influences are also considered. This study is applied to two dedicated spectrographs in order to help the optimization of radial velocity programs. Current methods of Doppler calculation are discussed andcompared.

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Documento generato il 24/05/13 alle ore 08:52:06