Publicación
Spectral Energy Distributions of Single Stellar Populations in the Infrared range
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PublicaciónSpectral evidence for jets from Accreting Millisecond X-ray PulsarsTransient radio emission from X-ray binaries is associated with synchrotron emission from collimated jets that escape the system, and accreting millisecond X...
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PublicaciónSpectral Indices in the NIR for Studying Stellar PopulationsSo far, detailed stellar population studies, based on the absorption line strengths have been concentrated mainly in the optical spectral range. In this work...
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PublicaciónSpectral library of age-benchmark low-mass stars and brown dwarfsIn recent years, some extremely red brown dwarfs have been discovered. They were believed to have a low surface gravity, but many of their spectral...
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PublicaciónSpectral Line Selection for HMIWe present information on two spectral lines, Fe I 6173 Å and Ni I 6768 Å, that were candidates for use in the Helioseismic and Magnetic Imager (HMI) instrument...
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PublicaciónSpectral lines insensitive to instrumental polarizationNot Available
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PublicaciónSpectral Metallicity in M33Not Available
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PublicaciónSpectral microvariability in QuasarsOptical 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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PublicaciónSpectral Modeling of the 3-μm Region of Cliff-Type Trans-Neptunian ObjectsTrans-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...