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/

  • A Comparative Study of Knots of Star Formation in Interacting versus Spiral Galaxies
    Interacting galaxies are known to have higher global rates of star formation on average than normal galaxies, relative to their stellar masses. Using UV and IR photometry combined with new and published Hα images, we have compared the star formation rates (SFRs) of ∼700 star forming complexes in 46 nearby interacting galaxy pairs with those of
    Smith, B. J. et al.

    Advertised on:

    3
    2016
    Citations
    19
  • A clean sightline to quiescence: multiwavelength observations of the high Galactic latitude black hole X-ray binary Swift J1357.2-0933
    We present coordinated multiwavelength observations of the high Galactic latitude (b = +50°) black hole X-ray binary (BHXB) Swift J1357.2-0933 in quiescence. Our broad-band spectrum includes strictly simultaneous radio and X-ray observations, and near-infrared, optical, and ultraviolet data taken 1-2 d later. We detect Swift J1357.2-0933 at all
    Plotkin, R. M. et al.

    Advertised on:

    3
    2016
    Citations
    30
  • 1RXS J180408.9-342058: An ultra compact X-ray binary candidate with a transient jet
    Aims: We present a detailed near-infrared/optical/UV study of the transient low-mass X-ray binary 1RXS J180408.9-342058 performed during its 2015 outburst, which is aimed at determining the nature of its companion star. Methods: We obtained three optical spectra (R ~ 1000) at the 2.1 m San Pedro Mártir Observatory telescope (México). We performed
    Baglio, M. C. et al.

    Advertised on:

    3
    2016
    Citations
    26
  • WASP-135b: A Highly Irradiated, Inflated Hot Jupiter Orbiting a G5V Star
    We report the discovery of a new transiting planet from the WASP survey. WASP-135b is a hot Jupiter with radius 1.30 ± 0.09 R Jup, mass 1.90 ± 0.08 M Jup, and an orbital period of 1.401 days. Its host is a Sun-like star, with a G5 spectral type and a mass and radius of 0.98 ± 0.06 M ⊙ and 0.96 ± 0.05 R ⊙, respectively. The proximity of the planet
    Spake, J. J. et al.

    Advertised on:

    2
    2016
    Citations
    16
  • THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system
    We present THERMAP, a mid-infrared spectro-imager for space missions to small bodies in the inner solar system, developed in the framework of the MarcoPolo-R asteroid sample return mission. THERMAP is very well suited to characterize the surface thermal environment of a NEO and to map its surface composition. The instrument has two channels, one
    Groussin, O. et al.

    Advertised on:

    2
    2016
    Citations
    3
  • The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
    In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph at Apache Point Observatory. These observations will be conducted simultaneously with the Time Domain Spectroscopic Survey (TDSS) designed for variability studies and the
    Dawson, K. S. et al.

    Advertised on:

    2
    2016
    Citations
    790