The CoRoT ground-based asteroseismological programme

Bibcode
2012AN....333.1061R
DOI
10.1002/asna.201211794
the CoRoT SWG Ground-based Observations Working Group; Uytterhoeven, K.; Amado, P. J.; Aerts, C.; Mathias, P.; Poretti, E.; Rainer, M.
Referencia bibliográfica

Astronomische Nachrichten, Vol.333, Issue 10, p.1061

Fecha de publicación:
12
2012
Número de autores
7
Número de autores del IAC
1
Número de citas
4
Número de citas referidas
1
Descripción
A large ground-based spectroscopic and photometric programme has accompanied the asteroseismological photometric observations of the satellite CoRoT since its launch. These simultaneously complementary observations allow to better characterize the targets, identify the modes and recover many other interesting physical information. In this paper, the spectroscopic ground-based programme is described, particularly with regards of the HARPS data, and some scientific cases are presented. The CoRoT space mission has been developed and is operated by the French space agency CNES, with participation of ESA (RSSD and Science Programme), Austria, Belgium. Brazil, Germany and Spain.
Tipo
Con árbitro
Instrumentación

Te puede interesar

  • Con árbitro
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Fecha de publicación:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Número de citas
    0
  • Con árbitro
    Counting stars from the integrated spectra of galaxies
    Over the last few decades, evolutionary population synthesis models have powered an unmatched leap forward in our understanding of galaxies. From dating the age of the first galaxies in the Universe to providing detailed measurements of the chemical composition of nearby galaxies, the success of this approach built upon simple stellar population
    Martín-Navarro, I. et al.

    Fecha de publicación:

    11
    2024
    Bibcode
    2024A&A...691L..10M
    Número de citas
    0
  • Con árbitro
    Model-based identification of solar coronal mass ejections using deep neural networks
    Coronal mass ejections (CMEs) are a major driver of space weather and thus can have important negative technological and social impacts. To assess their geoeffectiveness once they are ejected, it is crucial their prompt identification in coronagraph images. In the last decade, deep neural networks (DNN) have experienced enormous improvements in
    Iglesias, F. A. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024BAAA...65...17I
    Número de citas
    0