Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • 3D non-LTE corrections for the 6Li/7Li isotopic ratio in solar-type stars
    Doppler shifts induced by convective motions in stellar atmospheres affect the shape of spectral absorption lines and create slightly asymmetric line profiles. It is important to take this effect into account in modeling the subtle depression created by the 6Li isotope which lies on the red wing of the Li I 670.8 nm resonance doublet line, since
    Harutyunyan, G. et al.

    Fecha de publicación:

    2017
    Número de citas
    0
  • WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
    We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric light curves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 d, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805
    Hay, K. L. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    26
  • UV-extended E-MILES stellar population models: young components in massive early-type galaxies
    We present UV-extended E-MILES stellar population synthesis models covering the spectral range λλ 1680-50 000 Å at moderately high resolution. We employ the NGSL space-based stellar library to compute spectra of single-age, single-metallicity stellar populations in the wavelength range from 1680 to 3540 Å. These models represent a significant
    Vazdekis, A. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    390
  • Transmission spectroscopy of the inflated exoplanet WASP-52b, and evidence for a bright region on the stellar surface
    We have measured the transmission spectrum of the extremely inflated hot Jupiter WASP-52b using simultaneous photometric observations in Sloan Digital Sky Survey u', g' and a filter centred on the sodium doublet (Na I) with the ULTRACAM instrument mounted on the 4.2-m William Herschel Telescope. We find that Rayleigh scattering is not the dominant
    Kirk, J. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    51
  • Transit timing variation and transmission spectroscopy analyses of the hot Neptune GJ3470b
    GJ3470b is a hot Neptune exoplanet orbiting an M dwarf and the first sub-Jovian planet to exhibit Rayleigh scattering. We present transit timing variation (TTV) and transmission spectroscopy analyses of multiwavelength optical photometry from 2.4-m and 0.5-m telescopes at the Thai National Observatory, and the 0.6-m PROMPT-8 telescope in Chile. Our
    Awiphan, S. et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    36
  • The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters
    We present a direct measurement of the mean halo occupation distribution (HOD) of galaxies taken from the eleventh data release (DR11) of the Sloan Digital Sky Survey-III Baryon Oscillation Spectroscopic Survey (BOSS). The HOD of BOSS low-redshift (LOWZ: 0.2 z 0.4) and Constant-Mass (CMASS: 0.43 z 0.7) galaxies is inferred via their association
    White, Martin et al.

    Fecha de publicación:

    12
    2016
    Número de citas
    7