Tipo de publicación: Con árbitro

  • Publicación
    New Galactic supernova remnants discovered with IPHAS
    As part of a systematic search programme of a 10° wide strip of the northern Galactic plane, we present preliminary evidence for the discovery of four (and...
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    New giant planet beyond the snow line for an extended MOA exoplanet microlens sample
    Characterizing a planet detected by microlensing is hard if the planetary signal is weak or the lens-source relative trajectory is far from caustics. However...
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    New groups of planetary nebulae with peculiar dust chemistry towards the Galactic bulge
    Aims: We investigate Galactic bulge planetary nebulae without emission-line central stars for which peculiar infrared spectra have been obtained with the...
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    New GTC spectroscopic data and a statistical study to better constrain the redshift of the BL Lac RGB J2243 + 203
    We present new spectroscopic data of the BL Lac RGB 2243 + 203, and its surroundings, obtained with the OSIRIS Multi Object Spectrograph (MOS) mounted in the...
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    New H-band Stellar Spectral Libraries for the SDSS-III/APOGEE Survey
    The Sloan Digital Sky Survey-III (SDSS-III) Apache Point Observatory Galactic Evolution Experiment (APOGEE) has obtained high-resolution (R ∼ 22,500), high...
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    New Hard-TeV Extreme Blazars Detected with the MAGIC Telescopes
    Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic synchrotron emission. They also feature nonthermal gamma-ray...
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    New horizons in cosmology with spectral distortions of the cosmic microwave background
    This Voyage 2050 paper highlights the unique science opportunities using spectral distortions of the cosmic microwave background (CMB). CMB spectral distortions...
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    New Hubble Space Telescope WFC3/UVIS Observations Augment the Stellar-population Complexity of ω Centauri
    We used archival multi-band Hubble Space Telescope observations obtained with the Wide Field Camera 3 in the UV-optical channel to present important new...
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    New insights into the outflows from R Aquarii
    Context. The source R Aquarii is a symbiotic binary surrounded by a large and complex nebula with a prominent curved jet. It is one of the closest known...