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/

  • Design of the J-PAS and J-PLUS filter systems
    J-PAS (Javalambre-PAU Astrophysical Survey) is a Spanish-Brazilian collaboration to conduct an innovative photometric survey of more than 8000 square degrees of northern sky using a system of 57 filters, 54 narrow-band (FWHM=13.8 nm) filters continuously populating the spectrum between 370 to 920 nm with 10.0 nm steps, plus 3 broad-band filters
    Marín-Franch, A. et al.

    Advertised on:

    9
    2012
    Citations
    31
  • Design-considerations For A Ground-based Transit Survey To Find Habitable Planets Around L And T Dwarfs
    Detection of planets in the habitable zone is one of the key drivers of the exoplanet science community. We present a detailed strategy for such detection around L and T dwarfs. We plan to implement the outcome of the analysis as a transit survey to search for planets around known L and T dwarfs. Understanding of the variability of these cool
    Tata, R. et al.

    Advertised on:

    9
    2011
    Citations
    0
  • Detailed Bayesian Analysis of the CoRoT-7 Lightcurve
    With a mass of 7.4 Earth masses and radius of 1.6 Earth radii, CoRoT-7b is among the smallest transiting planets found to date. Due to its small size, the transit signal is very shallow, which makes the estimation of the planetary parameters from the light curve challenging. We carry out a Bayesian analysis of the CoRoT-7b lightcurve using a
    Parviainen, H. et al.

    Advertised on:

    9
    2011
    Citations
    0
  • Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry
    Aims: Using the CoRoT space based photometry of the O-type binary HD 46149, stellar atmospheric effects related to rotation can be separated from pulsations, because they leave distinct signatures in the light curve. This offers the possibility of characterising and exploiting any pulsations seismologically. Methods: Combining high-quality space
    Degroote, P. et al.

    Advertised on:

    9
    2010
    Citations
    57
  • Detection of Habitable-Sized Planets: A Progress Report
    Planets forming around close binary systems should form in the binary orbital plane (varying precession periods of protoplanetary material should provide strong collisional damping; Schneider and Doyle 1995). Planets around eclipsing binaries may then be expected to have formed in the binary orbital plane and thus to be detected by their transits
    Doyle, L. R. et al.

    Advertised on:

    9
    1996
    Citations
    0
  • Detection of the old stellar component of the major Galactic bar
    We present near-infrared colour-magnitude diagrams and star counts for a number of regions along the Galactic plane. It is shown that along the l=27°, b=0° line of sight there is a feature at 5.7+/-0.7kpc with a density of stars at least a factor of 2 and probably more than a factor of 5 times that of the disc at the same position. This feature
    Hammersley, P. L. et al.

    Advertised on:

    9
    2000
    Citations
    145