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/

  • Planck 2013 results. XI. All-sky model of thermal dust emission
    This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857 GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky maps of the dust optical depth, temperature, and spectral index over the 353-3000 GHz range. This model is a good representation of the IRAS and Planck data at 5' between
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    677
  • Planck 2013 results. XII. Diffuse component separation
    Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds, including thermal dust and line emission from
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    287
  • Planck 2013 results. XIII. Galactic CO emission
    Rotational transition lines of CO play a major role in molecular radio astronomy as a mass tracer and in particular in the study of star formation and Galactic structure. Although a wealth of data exists for the Galactic plane and some well-known molecular clouds, there is no available high sensitivity all-sky survey of CO emission to date. Such
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    178
  • Planck 2013 results. XIV. Zodiacal emission
    The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and diffuse interplanetary dust emission (IPD) are all observed. The IPD can be separated from Galactic and other emissions because Planck views a given point on the celestial sphere multiple times, through different columns of IPD
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    94
  • Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
    Based on cosmic microwave background (CMB) maps from the 2013 Planck Mission data release, this paper presents the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials. The significance of detection ranges from 2 to 4σ, depending on which method is used. We
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    180
  • Planck 2013 results. XV. CMB power spectra and likelihood
    This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature. We use this likelihood to derive our best estimate of the CMB angular power spectrum from
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    631