Tipo de publicación: Sin árbitro

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    Spectral lines insensitive to instrumental polarization
    Not Available
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    Spectral Metallicity in M33
    Not Available
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    Spectral microvariability in Quasars
    Optical microvariability (OM, small amplitude variations in time scales from minutes to hours) in radio-quiet quasars (RQQ) may be as frequent as in radio-loud...
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    Spectral Modeling of the 3-μm Region of Cliff-Type Trans-Neptunian Objects
    Trans-Neptunian Objects (TNOs) harbor some of the most pristine materials in the Solar System. JWST observations of TNOs from Cycle 1's campaign of "Discovering...
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    Spectral Parameters Following Gaffey Method Of Near-earth Asteroids And Main Belt Objects
    We have computed the Band Area Ratio (BAR) and Band I Center parameters, following the method by Cloutis et al. (1986) and Gaffey et al. (1993) for all the...
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    Spectral properties from XMM-Newton observation of Chandra Deep Field South sources
    We present results of the X-ray spectral analysis of the ˜370 ksec deep survey obtained with XMM-Newton on the Chandra Deep Field South (CDFS). Using sample of...
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    Spectral properties of 2020 AV2, the first known asteroid orbiting inside Venus orbit
    Recent numerical simulations (Greenstreet et al. 2012, Granvik et al. 2018) predicted the existence of a population of small bodies that is orbiting entirely...
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    Spectral properties of black holes
    Not Available
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    Spectral properties of near-Earth asteroids on cometary orbits
    We studied the spectral distributions of near-Earth asteroids on cometary orbits (NEACOs) in order to identify potential dormant or extinct comets among these...