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
    The JEM-EUSO instrument
    In this paper we describe the main characteristics of the JEM-EUSO instrument. The Extreme Universe Space Observatory on the Japanese Experiment Module (JEM-EUSO) of the International Space Station (ISS) will observe Ultra High-Energy Cosmic Rays (UHECR) from space. It will detect UV-light of Extensive Air Showers (EAS) produced by UHECRs
    Adams, J. H. et al.

    Advertised on:

    11
    2015
    Bibcode
    2015ExA....40...19A
    Citations
    43
  • Refereed
    The JEM-EUSO mission: An introduction
    The Extreme Universe Space Observatory on board the Japanese Experiment Module of the International Space Station, JEM-EUSO, is being designed to search from space ultra-high energy cosmic rays. These are charged particles with energies from a few 1019 eV to beyond 1020 eV, at the very end of the known cosmic ray energy spectrum. JEM-EUSO will also
    Adams, J. H. et al.

    Advertised on:

    11
    2015
    Bibcode
    2015ExA....40....3A
    Citations
    35
  • Refereed
    The JEM-EUSO observation in cloudy conditions
    The JEM-EUSO (Extreme Universe Space Observatory on-board the Japanese Experiment Module) mission will conduct extensive air shower (EAS) observations on the International Space Station (ISS). Following the ISS orbit, JEM-EUSO will experience continuous changes in the atmospheric conditions, including cloud presence. The influence of clouds on
    Adams, J. H. et al.

    Advertised on:

    11
    2015
    Bibcode
    2015ExA....40..135A
    Citations
    9
  • Refereed
    The K2-ESPRINT Project V: A Short-period Giant Planet Orbiting a Subgiant Star*
    We report on the discovery and characterization of the transiting planet K2-39b (EPIC 206247743b). With an orbital period of 4.6 days, it is the shortest-period planet orbiting a subgiant star known to date. Such planets are rare, with only a handful of known cases. The reason for this is poorly understood but may reflect differences in planet
    Van Eylen, V. et al.

    Advertised on:

    11
    2016
    Bibcode
    2016AJ....152..143V
    Citations
    45
  • Refereed
    The kinematic behaviour of optical recombination lines and collisionally excited lines in Galactic planetary nebulae*†
    The kinematics of the plasma in 14 planetary nebulae (PNe) is analysed by measuring the expansion velocities (Vexp) of different ions as derived from their collisionally excited lines (CELs) and optical recombination lines (ORLs). Vexp is analysed as a function of the ionization potential of ions, which at a first approximation represents the
    García-Rojas, J. et al.

    Advertised on:

    11
    2017
    Bibcode
    2017MNRAS.472.1182P
    Citations
    15
  • Non-refereed
    The kinematics and morphology of NGC 520: One, two, or three galaxies
    The peculiar galaxy NGC 520 (Arp 157) is often interpreted as an interacting pair of galaxies. The identification of the two bulges and overall morphology of the two galaxies has long been a puzzle which the authors attempt to solve here. New longslit optical spectroscopy and near-infrared images of NGC 520 are presented. These data suggest that
    Stanford, S. A. et al.

    Advertised on:

    11
    1990
    Bibcode
    1990NASCP3098..347S
    Citations
    1