Líneas de instrumentación: Instrumentación infrarroja

Instrumentación infrarroja

La instrumentación para detectar y analizar la luz en el rango infrarrojo del espectro es uno de los campos de conocimiento del Área de Instrumentación. El diseño y construcción de cámaras y espectrógrafos infrarrojos requiere de tecnologías del alto vacío y criogenia, que abarcan las especialidades de la ingeniería mecánica, óptica y electrónica, principalmente. La integración y funcionamiento de mecanismos y dispositivos en criogenia es especialmente compleja y exige unos conocimientos y equipamiento altamente especializados. El Área de Instrumentación tiene una larga historia de participación internacional en este tipo de instrumentación.

  • Publicación
    The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516
    Dwarf barred galaxies are the perfect candidates for hosting slowly rotating bars. They are common in dense environments and have a relatively shallow potential...
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    The effect of environment on star forming galaxies at redshift 1 First insight from PACS (Corrigendum)
    Not Available
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    The effect of environment on star forming galaxies at redshift. I. First insight from PACS
    We use deep 70, 100 and 160 μm observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS...
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    The effects of spatial resolution on integral field spectrograph surveys at different redshifts - The CALIFA perspective
    Context. Over the past decade, 3D optical spectroscopy has become the preferred tool for understanding the properties of galaxies and is now increasingly used...
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    The Emission and Distribution of Dust of the Torus of NGC 1068
    We present observations of NGC 1068 covering the 19.7–53.0 μm wavelength range using FORCAST and HAWC+ on board SOFIA. Using these observations, high-angular...
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    The ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) . I. Project description, survey sample, and quality assessment
    The carriers of the diffuse interstellar bands (DIBs) are largely unidentified molecules ubiquitously present in the interstellar medium (ISM). After decades of...
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    The evolution of the dust temperatures of galaxies in the SFR-M∗ plane up to z s 2
    We study the evolution of the dust temperature of galaxies in the SFR- M∗ plane up to z ~ 2 using far-infrared and submillimetre observations from the Herschel...
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    The Filling Factor-Radius Relation for 58 H II Regions across the Disk of NGC 6946
    Using the OSIRIS tunable narrowband imager on the 10.4 m GTC (La Palma), we have mapped the SAB(rs)cd galaxy NGC 6946 over a ~7.3 × 7.5 arcmin2 field in the...
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    The first super-Earth detection from the high cadence and high radial velocity precision Dharma Planet Survey
    The Dharma Planet Survey (DPS) aims to monitor about 150 nearby very bright FGKM dwarfs (within 50 pc) during 2016-2020 for low-mass planet detection and...