Astrofísicas: Instrumentación

  • Publicación
    Statistics and analysis of high-altitude wind above the Canary Islands observatories
    High-altitude wind has been recently proposed as an important parameter to be taken into account for astronomical site selection. We present here comprehensive...
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    Status and scientific performance of Elmer, a multi-purpose instrument for the GTC
    ELMER is an instrument for the GTC designed to observe between 365 and 1000 nm. The observing modes for the instrument at Day One shall be: Imaging, Long Slit...
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    Stellar and ionized gas kinematics of the interacting Seyfert 1.9 galaxy NGC 2992
    Integral field spectroscopy in the central 16''x 12'' (2.4 kpc x 1.8 kpc, if H0 = 75 km s-1 Mpc-1) of the Seyfert 1.9 galaxy NGC 2992 has been obtained using...
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    Stellar Observations Network Group: The prototype is nearly ready
    The prototype telescope and instruments for the Stellar Observations Network Group (SONG) are nearing completion at the Observatorio del Teide on Tenerife. In...
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    Strategy for the Inversion of Hinode Spectropolarimetric Measurements in the Quiet Sun
    In this paper we propose an inversion strategy for the analysis of spectropolarimetric measurements taken by Hinode in the quiet Sun. The Spectro-Polarimeter of...
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    Submillimeter Polarization Spectrum in the Vela C Molecular Cloud
    Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500 μm during the 2012 flight of the balloon-borne telescope BLASTPol. These...
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    Submillimeter Polarization Spectrum of the Carina Nebula
    Linear polarization maps of the Carina Nebula were obtained at 250, 350, and 500 μm during the 2012 flight of the Balloon-borne Large Aperture Submillimeter...
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    SUNRISE Impressions from a successful science flight
    SUNRISE is a balloon-borne telescope with an aperture of one meter. It is equipped with a filter imager for the UV wavelength range between 214 nm and 400 nm...
  • Publicación
    SYMPA, a dedicated instrument for Jovian seismology. I. Principle and performance
    Aims:The detection and measurement of acoustic modes on the giant planets of the solar system is of great interest for the study of the internal structure and...