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/

  • 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.

    Advertised on:

    12
    2016
    Citations
    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.

    Advertised on:

    12
    2016
    Citations
    38
  • 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.

    Advertised on:

    12
    2016
    Citations
    7
  • The rotation-metallicity relation for the Galactic disk as measured in the Gaia DR1 TGAS and APOGEE data
    Aims: Previous studies have found that the Galactic rotation velocity-metallicity (V-[Fe/H]) relations for the thin and thick disk populations show negative and positive slopes, respectively. The first Gaia data release includes the Tycho-Gaia Astrometric Solution (TGAS) information, which we use to analyze the V-[Fe/H] relation for a strictly
    Cropper, Mark et al.

    Advertised on:

    12
    2016
    Citations
    30
  • The rotation-metallicity relation for the Galactic disk as measured in the Gaia DR1 TGAS and APOGEE data
    Aims: Previous studies have found that the Galactic rotation velocity-metallicity (V-[Fe/H]) relations for the thin and thick disk populations show negative and positive slopes, respectively. The first Gaia data release includes the Tycho-Gaia Astrometric Solution (TGAS) information, which we use to analyze the V-[Fe/H] relation for a strictly
    Allende Prieto, C. et al.

    Advertised on:

    12
    2016
    Citations
    0
  • The role of partial ionization in solar chromospheric heating
    The most energetic part of the Sun, its interior, due to its plasma parameters is hidden below the solar surface and invisible to the observer. Nevertheless, the solar interior generates the energy and provokes atmospheric magnetic activity. Despite great progress in both observational and simulational methods, the mechanism of energy transport
    Shelyag, S. et al.

    Advertised on:

    12
    2016
    Citations
    0