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/

  • The Polarimetric and Helioseismic Imager on Solar Orbiter
    Aims: This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between
    Solanki, S. K. et al.

    Advertised on:

    10
    2020
    Citations
    177
  • The irregular limb of Manoetius South Pole and Improved Orbital Solution (extended analysis)
    In 2033, after a 12-year trip across the Solar System, NASA's Lucy mission will arrive at the Patroclus─Menoetius binary system, in Jupiter's L5 cloud. On its way, Lucy will visit one asteroid and seven Jupiter Trojans, all of them primitive asteroids. Lucy's foreseen discoveries about the surface geology, color, and composition of these Trojans
    Pinilla-Alonso, N. et al.

    Advertised on:

    10
    2020
    Citations
    0
  • The impact of dust attenuation laws on the stellar mass of galaxies ─ based on 170 million galaxies from HELP survey
    The Herschel Extragalactic Legacy Project (HELP) focused on the data from ESA's Herschel} mission, which covered around 1300~$\rm deg^2$ on the sky. HELP systematically combines data from 23 of the premier extragalactic survey fields. It compiles all the ancillary data that are available across the HELP fields into a catalogue with consistent
    Małek, Katarzyna et al.

    Advertised on:

    10
    2020
    Citations
    0
  • The GALAH Survey: non-LTE departure coefficients for large spectroscopic surveys
    Massive sets of stellar spectroscopic observations are rapidly becoming available and these can be used to determine the chemical composition and evolution of the Galaxy with unprecedented precision. One of the major challenges in this endeavour involves constructing realistic models of stellar spectra with which to reliably determine stellar
    Amarsi, A. M. et al.

    Advertised on:

    10
    2020
    Citations
    92
  • The Gaia-ESO Survey: A new diagnostic for accretion and outflow activity in the young cluster NGC 2264
    Context. NGC 2264 is a young cluster whose accretion properties can be investigated in detail by taking advantage of the FLAMES data in the context of the Gaia-ESO Survey. In fact, the analysis of the Hα emission line profile can provide us with information about the accretion and ejection activity of young stars. However, a strong nebular emission
    Bonito, R. et al.

    Advertised on:

    10
    2020
    Citations
    14
  • The chemical evolution of the dwarf spheroidal galaxy Sextans
    We present our analysis of the FLAMES dataset targeting the central 25' region of the Sextans dwarf spheroidal galaxy (dSph). This dataset is the third major part of the high-resolution spectroscopic section of the ESO large program 171.B-0588(A) obtained by the Dwarf galaxy Abundances and Radial-velocities Team. Our sample is composed of red giant
    Theler, R. et al.

    Advertised on:

    10
    2020
    Citations
    30