'Spectral classification' diaporamas de présentation

Stellar Spectral classification The First Step in Quantitative Spectral Analysis PART I AND II

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Image Classification and Others

Image Classification and Others. Ruiliang Pu Ecosystem Science Division Department of ESPM University of California, Berkeley, USA March 02, 2004. Outline. What is image classification? General classification procedures General classifiers Accuracy assessment

1.09k views • 62 slides

Spectral Classification: The First Step in Quantitative Spectral Analysis

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Line Spectra

Line Spectra. From the Study of Spectral Lines We can Know. Composition (which lines occur). H lines. CaII lines. CaI line. Fe I lines. Composition. From the Study of Spectral Lines We can Know. Composition (which lines occur) Temperature (relative strength of lines).

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Origin and Early Evolution of Brown Dwarfs

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Chair : M. Deleuil

Exoplanets Complementary Observations Working Group. Chair : M. Deleuil. Goal:. organise and coordinate observational efforts for programs using the exoplanet channel. prepare the targets selection + mask allocation. prepare the scientific analysis.

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Snow cover mapping using multi-temporal Meteosat-8 data Martijn de Ruyter de Wildt

280 views • 16 slides

VIMOS@VLT observations of Dolidze 25

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SED Machine A Transient Classifier

SED Machine A Transient Classifier. Electromagnetic counterparts to physics experiments. Palomar Transient Factory. Spectral Classification. Follow up. WHT 4.2 m. Lick 3 m. Discovery. Keck. Gemini. Mayall 4 m. P48. HST. + four band imaging. P60. Gemini. P60. P200. P200.

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EXODAT : a Data Base for the CoRoT/ Exoplanet channel

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Bruce Gendre Osservatorio di Roma / ASI Science Data Center

Recent activities from the TAROT/Zadko network. Bruce Gendre Osservatorio di Roma / ASI Science Data Center. The TAROT/Zadko Network. Set of 3 robotic telescopes France (20 cm diameter) Chile (20 cm diameter) Australia (1m diameter) Aims GRB studies Space debris monitoring

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