Astrofísicas: Cartografiados

  • Publicación
    Deep Ks -near-infrared Surface Photometry of 80 Dwarf Irregular Galaxies in the Local Volume
    We present deep near-infrared (Ks ) images and surface photometry for 80 dwarf irregular galaxies (dIs) within ~5 Mpc of the Milky Way. The galaxy images were...
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    Deep learning and numerical simulations to infer the evolution of MaNGA galaxies
    As surveys grow, the challenge is how to explore and interpret the increasing quantity of data. Integral field spectroscopic (IFS) galaxy surveys are a good...
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    Deep Optical and Near Infrared Observations in ELAIS Areas
    We present deep optical and near infrared imaging over half square degree of sky in the centres of the ELAIS regions N1 and N2 and coincident with deep XMM...
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    DENIS Catalogue toward Magellanic Clouds (DCMC) (Cioni+ 2000)
    This is the first version of a complete near-IR point source catalogue towards the Magellanic Clouds extracted from the data obtained with the DEep Near...
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    DES Y3 cosmic shear down to small scales: Constraints on cosmology and baryons
    We present the first analysis of cosmic shear measured in DES Y3 that employs the entire range of angular scales in the data. To achieve this, we built upon...
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    Detection and analysis of a new INTEGRAL hard X-ray transient, IGR J17285-2922
    We present the transient nature of INTEGRAL source IGR J17285 2922, identified from a single period of activity during an IBIS/ISGRI Galactic Centre Deep...
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    Detection of spectral variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
    Anomalous Microwave Emission (AME) is a significant component of Galactic diffuse emission in the frequency range 10- $60\, \mathrm{GHz}$ and a new window into...
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    Determining the fraction of reddened quasars in COSMOS with multiple selection techniques from X-ray to radio wavelengths
    The sub-population of quasars reddened by intrinsic or intervening clouds of dust are known to be underrepresented in optical quasar surveys. By defining a...
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    Differences between the Pallas collisional family and similarly sized B-type asteroids
    Context. B-type asteroids constitute a peculiar spectral class within the C-complex. Previous work has pointed out the difference between the visible geometric...