Tipo de publicación: Con árbitro

  • Publicación
    V404 CYG/GS 2023+338: Monitoring in the Optical with Robotic Telescopes of the MASTER Global Network during the 2015 Superburst
    2070 unique, homogeneous photometric and polarization observations of the microquasar in a binary system with a black hole V404 Cyg/GS2023+338 obtained in 2015...
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    V533 Herculis: the second SW Sex old nova displaying emission-line flaring
    We present high-time-resolution spectroscopy of the non-eclipsing old nova V533 Herculis (N Her 1963). It is the second nova remnant affected by the `SW Sex...
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    V795 Her: an SW Sex star in the period gap?
    We present optical photometry and spectroscopy of the nova-like variable V795 Her. The emission lines exhibit an extremely complex structure consisting of...
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    VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35
    We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterize galaxy populations up to z =...
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    Validating full-spectrum fitting with a synthetic integral-field spectroscopic observation of the Milky Way
    Ongoing deep integral-field spectroscopy (IFS) observations of disc galaxies provide opportunities for comparison with the Milky Way (MW) to understand galaxy...
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    Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf
    Context. The NASA space telescope TESS is currently in the extended mission of its all-sky search for new transiting planets. Of the thousands of candidates...
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    Validation of 13 Hot and Potentially Terrestrial TESS Planets
    The James Webb Space Telescope will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify...
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    Validation of a Third Planet in the LHS 1678 System
    The nearby LHS 1678 (TOI-696) system contains two confirmed planets and a wide-orbit, likely brown-dwarf companion, which orbit an M2 dwarf with a unique...
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    Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument
    The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg 2 over 5 yr to constrain the cosmic expansion history...