Líneas de instrumentación: Instrumentación microondas

Instrumentación microondas

Desde los años 80 el Área de Instrumentación viene desarrollando instrumentación y experimentos en el rango de las microondas con el objetivo principal de caracterizar la radiación del Fondo Cósmico de Microondas (FCM) y otros procesos de emisión galáctica y extra-galáctica.

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    The effect of environment on star forming galaxies at redshift 1 First insight from PACS (Corrigendum)
    Not Available
  • Publicación
    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 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 Herschel PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4
    We exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the Herschel Guaranteed Time Observation (GTO) PACS Evolutionary Probe (PEP) Survey...
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    The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
    By making use of Herschel PACS Evolutionary Probe observations of the COSMOS and Extended Groth Strip fields, we have estimated the dependence of the clustering...
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    The impact from survey depth and resolution on the morphological classification of galaxies
    We consistently analyse for the first time the impact of survey depth and spatial resolution on the most used morphological parameters for classifying galaxies...
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    The Impact of Evolving Infrared Spectral Energy Distributions of Galaxies on Star Formation Rate Estimates
    We combine Herschel-Photodetector Array Camera and Spectrometer (PACS) data from the PACS Evolutionary Probe (PEP) program with Spitzer 24 μm and 16 μm...
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    The Lockman-SpReSO project. Description, target selection, observations, and catalogue preparation
    Context. Extragalactic surveys are a key tool for better understanding the evolution of galaxies. Both deep and wide-field surveys serve to provide a clearer...