Tipo de publicación: Con árbitro

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    Manufacturing of 3D-metallic electromagnetic metamaterials for feedhorns usedin radioastronomy and satellite communications
    The electromagnetic metamaterials at microwaves frequencies are well established in industrial applications nowadays. Recent research has shown that a specific...
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    Mapping atomic and diffuse interstellar band absorption across the Magellanic Clouds and the Milky Way
    Diffuse interstellar bands (DIBs) trace warm neutral and weakly ionized diffuse interstellar medium (ISM). Here we present a dedicated, high signal-to-noise...
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    Mapping diffuse interstellar bands in the local ISM on small scales via MUSE 3D spectroscopy. A pilot study based on globular cluster NGC 6397
    Context. We map the interstellar medium (ISM) including the diffuse interstellar bands (DIBs) in absorption toward the globular cluster NGC 6397 using VLT/MUSE...
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    Mapping dusty galaxy growth at z > 5 with FRESCO: detection of Hα in submm galaxy HDF850.1 and the surrounding overdense structures
    We report the detection of a 13 $\sigma$ H $\alpha$ emission line from HDF850.1 at $z=5.188\pm 0.001$ using the FRESCO (First Reionization Era Spectroscopically...
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    Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck
    We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the...
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    Mapping luminous blue compact galaxies with VIRUS-P. Morphology, line ratios, and kinematics
    Context. Blue compact galaxies (BCG) are narrow emission-line systems that undergo a violent burst of star formation. They are compact, low-luminosity galaxies...
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    Mapping non-axisymmetric velocity fields of external galaxies
    Disc galaxies are typically in a stable configuration where matter moves in almost closed circular orbits. However, non-circular motions caused by distortions...
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    Mapping solar magnetic fields from the photosphere to the base of the corona
    Routine ultraviolet imaging of the Sun's upper atmosphere shows the spectacular manifestation of solar activity; yet we remain blind to its main driver, the...
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    Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136
    We introduce VLT-MUSE observations of the central 2'× 2' (30 × 30 pc) of the Tarantula Nebula in the Large Magellanic Cloud. The observations provide an...