Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Complemetary Observations for the CoRoT Exoplanet Program
    We review the needs of the CoRoT /exoplanet program in terms of complementary observations. Such observations are indeed an essential element of the science of the CoRoT mission at different levels: prior to the launch for a characterization and a careful selection of the target stars in the exoplanet fields and during or after the CoRoT flight
    Deleuil, M. et al.

    Advertised on:

    11
    2006
    Citations
    23
  • Close Galaxy Counts as a Probe of Hierarchical Structure Formation
    The standard ΛCDM model predicts that the major merger rate of galaxy-size dark matter halos rises rapidly with redshift. The average number of close companions per galaxy, Nc, is often used to infer the galaxy merger rate; however, recent observational studies suggest that Nc evolves very little with redshift. Here we use a ``hybrid'' N-body
    Berrier, Joel C. et al.

    Advertised on:

    11
    2006
    Citations
    99
  • Chemical abundances for the transiting planet host stars OGLE-TR-10, 56, 111, 113, 132, and TrES-1. Abundances in different galactic populations
    Aims.We used the UVES spectrograph (VLT-UT2 telescope) to obtain high-resolution spectra of 6 stars hosting transiting planets, namely for OGLE-TR-10, 56, 111, 113, 132, and TrES-1. These spectra are now used to derive and discuss the chemical abundances for C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Cu, and Zn. Methods: .Abundances
    Santos, N. C. et al.

    Advertised on:

    11
    2006
    Citations
    27
  • Characteristics and performance of the GAW experiment for a large field of view Cerenkov γ rays telescope
    The GAW project aims to test the feasibility of a new generation of Imaging Atmospheric Cherenkov Telescopes that join high flux sensitivity with Large Field of View capability. It consists of an array of 3 imaging Cherenkov telescopes each equipped with a Fresnel refractive lens of about 3.6 m2 geometrical area and an array of multi-anode
    Delgado, C.

    Advertised on:

    11
    2006
    Citations
    0
  • CAMPOS MAGNÉTICOS EN EL SOL EN CALMA
    En esta tesis doctoral se realiza un estudio de las propiedades magnéticas del Sol en calma, aquellas regiones en el Sol donde el magnetismo pasa casi desapercibido. Se llega a la conclusión que los campos magnéticos son débiles, de unas pocas centenas de Gauss, llenando una porción pequeña del elemento de resolución. Además las estructuras
    Mª JESUS MARTÍNEZ GONZALEZ

    Advertised on:

    11
    2006
  • ANISOTROPIAS PRIMARIAS Y SECUNDARIAS DEL FONDO COSMICO DE MICROONDAS: PARAMETROS COSMOLOGICOS Y LA DISTRIBUCION DE BARIONES
    En esta tesis se presentó un estudio de las anisotropías primarias y secundarias del Fondo Cósmico de Microondas (FCM) en escalas angulares intermedias (entre 2º y 11 minutos de arco), utilizando principalmente observaciones del interferómetro Very Small Array (VSA). Este instrumento se encuentra situado en el Observatorio del Teide y opera a una
    RICARDO T. GENOVA SANTOS

    Advertised on:

    11
    2006