Tipo de publicación: Sin árbitro

  • Publicación
    The Sloan Digital Sky Survey as an Archetypal Mid-Scale Program
    We describe the Sloan Digital Sky Survey (SDSS) as an archetypal mid-scale program, including the technical, scientific, and organizational aspects underpinning...
  • Publicación
    The Sloan Digital Sky Survey extended point spread functions, a summary
    A robust and extended characterization of the point spread function (PSF) is crucial to extract the photometric information produced by deep imaging surveys...
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    The Sloan Digital Sky Survey Quasar Catalog Sixteenth Data Release
    Starting with its earliest Data Releases, the Sloan Digital Sky Survey (SDSS) has a long history of producing visually inspected quasar catalogs. Here, we...
  • Publicación
    The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
    The Sloan Digital Sky Survey (SDSS) has a rich history of releasing value-added catalogs for objects of interest to researchers, especially quasars. In that...
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    The small scale angular anisotropy at 145 GHz as seen by the Atacama Cosmology Telescope
    Not Available
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    The small-ELF project: toward an ultra-large coronagraphic optical receiver
    The small ExoLife Finder (sELF) telescope is a 3.4m diameter fixed pupil tracking Fizeau interferometer. Its design relies on several new technologies the ELF...
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    The Solar Acoustic Spectrum as Seen by GOLF. I. The Difficult Case: Modes With n<10
    Below 1.3 mHz the solar background level increases as well as the energy of the solar acoustic modes decreases. This situation yields the detection of low...
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    The Solar Acoustic Spectrum as Seen by GOLF. II. Noise Statistics Background and Methods of Analysis
    Data acquired by GOLF experiment onboard SOHO during ~20 months has been analysed. GOLF is a disk-integrated sunlight experiment therefore biased to observe...
  • Publicación
    The Solar Acoustic Spectrum as Seen by GOLF. III. Asymmetries, Resonant Frequencies and Splittings
    The definition of the model to fit to the observed spectra depends on the physics we are assuming is present in the phenomena we are observing. Here we present...