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/

  • Refereed
    SOPHIE velocimetry of Kepler transit candidates. XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet
    In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the Kepler space telescope and then validated thanks to a radial velocity follow-up with the SOPHIE spectrograph. It orbits its host star with a period of 86.647661 d ± 3 s and a high eccentricity of 0.772 ± 0.045
    Santerne, A. et al.

    Advertised on:

    11
    2014
    Bibcode
    2014A&A...571A..37S
    Citations
    68
  • Refereed
    Single-walled Carbon Nanohorn: Electronic Absorption Spectra in Neutral and Oxodized State
    The electronic absorption spectrum of single-walled carbon nanohorn (SWCNH) shows a relatively broad absorption peak at 256-259 nm when suspended in tetradecane and in decalin. The electronic absorption spectrum is also characterized by a series of small bands recalling the spectra of C-60 and C-70 fullerenes. Surprisingly, SWCNH shows a minimal
    Iglesias-Groth, S. et al.

    Advertised on:

    11
    2014
  • Refereed
    Sailing under the Magellanic Clouds: a DECam view of the Carina dwarf
    We present deep optical photometry from the DECam imager on the 4 m Blanco telescope of over 12 deg2 around the Carina dwarf spheroidal, with complete coverage out to 1 deg and partial coverage extending out to 2.6 deg. Using a Poisson-based matched-filter analysis to identify stars from each of the three main stellar populations, old, intermediate
    McMonigal, B. et al.

    Advertised on:

    11
    2014
    Bibcode
    2014MNRAS.444.3139M
    Citations
    39
  • Refereed
    Precision Measurement of the (e++e-) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
    We present a measurement of the cosmic ray (e++e-) flux in the range 0.5 GeV to 1 TeV based on the analysis of 10.6 million (e++e-) events collected by AMS. The statistics and the resolution of AMS provide a precision measurement of the flux. The flux is smooth and reveals new and distinct information. Above 30.2 GeV, the flux can be described by a
    Aguilar, M. et al.

    Advertised on:

    11
    2014
    Bibcode
    2014PhRvL.113v1102A
    Citations
    269
  • Refereed
    Planck 2013 results. XXXI. Consistency of the Planck data
    The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the comparison of the 70 GHz (amplifier) and 100 GHz (bolometer) channels. Based on different instrument technologies, with feeds located differently in the focal plane, analysed
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Bibcode
    2014A&A...571A..31P
    Citations
    73
  • Refereed
    Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
    We present new measurements of cosmic infrared background (CIB) anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross-frequency power spectrum is measured from 143 to 3000 GHz, and the auto-bispectrum from 217 to 545 GHz. The total areas used to compute the CIB power spectrum and bispectrum are about 2240 and 4400
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Bibcode
    2014A&A...571A..30P
    Citations
    271