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/

  • Physical properties of simulated galaxy populations at z = 2 - I. Effect of metal-line cooling and feedback from star formation and AGN
    We use hydrodynamical simulations from the OverWhelmingly Large Simulations (OWLS) project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on metal-line cooling and feedback from star formation and active galactic nuclei (AGN). We find that if the sub-grid feedback from star formation is implemented
    Haas, Marcel R. et al.

    Advertised on:

    11
    2013
    Citations
    72
  • Physical properties of simulated galaxy populations at z = 2 - II. Effects of cosmology, reionization and ISM physics
    We use hydrodynamical simulations from the OverWhelmingly Large Simulations project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on the assumed star formation law, the equation of state imposed on the unresolved interstellar medium, the stellar initial mass function, the reionization history and the
    Haas, Marcel R. et al.

    Advertised on:

    11
    2013
    Citations
    33
  • Physical properties of the extreme Centaur and super-comet candidate 2013 AZ60
    We present estimates of the basic physical properties including size and albedo of the extreme Centaur 2013 AZ60. These properties have been derived from optical and thermal infrared measurements. Our optical measurements revealed a probable full period of ≈9.4 h with a shallow amplitude of 4.5%. By combining optical brightness information and
    Pál, A. et al.

    Advertised on:

    11
    2015
    Citations
    11
  • PKS 1814-637: a powerful radio-loud AGN in a disk galaxy
    We present a detailed study of PKS 1814-637, a rare case of powerful radio source (P5 GHz = 4.1 × 1025 W Hz-1) hosted by a disk galaxy. Optical images have been used to model the host galaxy morphology confirming it to be dominated by a strong (and warped) disk component that is observed close to edge-on to the line of sight. This is the first
    Morganti, R. et al.

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    11
    2011
    Citations
    59
  • Planck 2013 results. I. Overview of products and scientific results
    The European Space Agency’s Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    1000
  • Planck 2013 results. II. Low Frequency Instrument data processing
    We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. In particular, we discuss the various steps involved in reducing the data, from telemetry packets through to the production of
    Planck Collaboration et al.

    Advertised on:

    11
    2014
    Citations
    78