Publicación
An Attempt to Estimate the Intensity Background Spectra
Not Available
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PublicaciónAn Attempt to Observe Stellar Convection via Power SpectrumIt is known that the convective motions at solar photosphere level are visible in the frequency domain through the so called ""solar noise"". Time-resolved...
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PublicaciónAn Automatic Approach for Selecting New HA Emission-Line GalaxiesNot Available
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PublicaciónAn Automatic Pipeline for Very High-Energy Gamma-Ray Data Analysis: Application to ASTRI SimulationsWith the evolution of very high-energy (VHE) gamma-ray astronomy, new tools for data analysis are being developed. One of these new tools is Gammapy, a python...
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PublicaciónAn automatically controlled SCIDAR instrument for Roque de los Muchachos ObservatorySCIDAR has proved to be the most efficient technique to obtain the optical vertical structure of the atmospheric turbulence measured from ground level. However...
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PublicaciónAn efficient evolution algorithm for population synthesis of AGB starsWe have developed an efficient and accurate set of mostly analytic formulae, that describe the evolution of stars in a wide range of mass and metallicity from...
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PublicaciónAn Efficient Low-Resolution NIR Classification Scheme for M, L, and T dwarfs and Its Application to Young BDsWe present the preliminary results of a programme aimed at defining a low-resolution near-infrared spectral classification scheme for faint M, L, and T-dwarfs...
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PublicaciónAn ellipsoidal modulation in X-ray Nova VELA 1993Observations of the soft X-ray transient Nova Vela 1993 are presented. These are the first observations, taken during quiescence in 1995 and 1996. An orbital...
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PublicaciónAn emerging hybrid technology toward ultra-light and self-correcting, "live" mirrorsThe constantly increasing needs for astronomical imaging of ever fainter objects as well as for imaging the Earth from space require much higher angular...