Tipo de publicación: Con árbitro

  • Publicación
    Filtering out near-surface uncertainties from helioseismic inversions
    The differences between observed solar p-mode frequencies and the frequencies of a reference model can be inverted to infer the structure of the Sun using a...
  • Publicación
    Final analysis of ELAIS 15-μm observations: method, reduction and catalogue
    We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-μm observations, carried out with the ISO Camera...
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    Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey
    The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is a dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of...
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    Finding galaxy clusters using Voronoi tessellations
    We present an objective and automated procedure for detecting clusters of galaxies in imaging galaxy surveys. Our Voronoi Galaxy Cluster Finder (VGCF) uses...
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    Finding Our Place in the Cosmos: The Role of Astronomy In Ancient Cultures
    Mircea Eliade (1992) argued that a single view of the starry celestial vault would be sufficient to awake a religious experience. This idea is as true today as...
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    Finding the hidden Milky Way.
    The Astrophysics Institute of the Canaries (IAC) studies the Galaxy's hidden centre from the Teide Observatory, Tenerife.
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    Fine structure and dynamics in a light bridge inside a solar pore
    A photometric analysis of the sub-structure of a granular light bridge in a large solar pore is performed. The data consist of a 66 min time series of white...
  • Publicación
    Fine structure in the Sigma Orionis cluster revealed by Gaia DR3
    Context. Sigma Orionis is an open cluster in the nearest giant star formation site - Orion. Its youth (3−5 Myr), low reddening, and relative vicinity make it an...
  • Publicación
    Fine structure of wave motions in the solar photosphere: Observations and theory
    Spectral observations of the 639.361-nm FeI line at the center of the quiet solar disk with high spatial (0.4″) and temporal (10 s) resolution are used to...