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    Chapter and Conference Paper

    ESPRESSO: A High Resolution Spectrograph for the Combined Coudé Focus of the VLT

    In the frame of the call for proposal for the E-ELT instrumentation studies, the CODEX team carried out the feasibility study for a spectrograph for extremely stable Doppler measurements. The CODEX project and...

    Luca Pasquini, A. Manescau, G. Avila, B. Delabre in Science with the VLT in the ELT Era (2009)

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    Chapter and Conference Paper

    From ESPRESSO to CODEX

    CODEX and ESPRESSO are concepts for ultra-stable, high-resolution spectrographs at the E-ELT and VLT, respectively. Both instruments are well motivated by distinct sets of science drivers. However, ESPRESSO wi...

    J. Liske, L. Pasquini, P. Bonifacio, F. Bouchy in Science with the VLT in the ELT Era (2009)

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    Chapter and Conference Paper

    Transiting Planets: Follow the FLAMES...

    The identification of transiting planets candidates and their a posteriori confirmation and characterization by means of spectroscopic follow-up is allowing us to study the internal physics of these planets. H...

    C. Melo, N. C. Santos, F. Pont, M. Mayor, S. Udry in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    Codex

    Many talks in this conference have shown the power of high resolution spectroscopy, coupled to high precision. A new spectrograph, fed by an Extremely Large Telescope, will have such a huge collecting power th...

    Luca Pasquini, G. Avila, B. Délabre, H. Dekker in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    Planet Detection Around M Dwarfs: New Constraints on Planet Formation Models

    The dependence of planetary statistics on the physical conditions during the initial stages of the system (i.e. in the proto-planetary disk) represent an essential constraint on planetary formation mechanisms....

    T. Forveille, X. Bonfils, X. Delfosse in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    Pushing Down the Limits of the Radial Velocity Technique

    We present results from the first three years of operations of the HARPS spectrograph installed on the ESO-3.6m telescope at La Silla Observatory, Chile. This instrument, primarily built to detect extrasolar p...

    C. Lovis, M. Mayor, F. Pepe, D. Queloz, S. Udry in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    High-resolution Spectroscopy of Faint Stars with Transiting Planets

    We present a series of studies based on high-resolution UVES/VLT spectroscopy of several faint stars for which a transit by a giant planet has been detected. The spectra were used to derive accurate stellar pa...

    N. C. Santos, C. Melo, F. Pont, T. Guillot in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    The HARPS Project

    To pursue a competitive programme in the domain of extra-solar planet search, ESO proposed to build HARPS (High-Accuracy Radial-velocity Planetary Search), a new high-resolution spectrograph to be installed on...

    F. Pepe, M. Mayor, W. Benz, J.-L. Bertaux in From Extrasolar Planets to Cosmology: The … (2000)

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    Chapter and Conference Paper

    Extrasolar Planets in the Southern Hemisphere: The CORALIE Survey

    We are conducting a large survey to detect extrasolar planets by high precision Doppler spectroscopy using the new swiss Euler telescope and the spetrograph CORALIE. The sample includes 1600 nearby G and K sta...

    D. Queloz, M. Mayor, D. Naef, N. Santos in From Extrasolar Planets to Cosmology: The … (2000)

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    Chapter and Conference Paper

    The CORALIE Planet-Search Sample

    This short contribution presents a description of the CORALIE sample selection of more than 1600 dwarf stars for the planet-search programme on the 1.2-m Euler Swiss telescope at La Silla. The instrumentation,...

    S. Udry, M. Mayor, D. Queloz, D. Naef in From Extrasolar Planets to Cosmology: The … (2000)

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    Chapter

    The New Planetary Systems

    A summary on recent results about planet detections are presented. Some results about brown-dwarfs are also discussed in the context of the maximum mass for a giant planet and the realm of planetary formation ...

    D. Queloz in Planets Outside the Solar System: Theory and Observations (1999)

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    Chapter

    Indirect Searches: Doppler Spectroscopy and Pulsar Timing

    The search for planetary systems by monitoring the motion of stellar objects along the line-of-sight is, up to now, the most efficient and successful way to detect planets. For millisec-pulsars, the measuremen...

    D. Queloz in Planets Outside the Solar System: Theory and Observations (1999)

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    Chapter and Conference Paper

    Epicurus was Right: Other Worlds Exist!

    The discovery of the first planet orbiting a solar type star acted on all groups working in that field as a tremendeous stimulation. Nine months after the discovery of 51 Peg B, five planetary companions have ...

    M. Mayor, D. Queloz in Infrared Space Interferometry: Astrophysic… (1997)