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Chapter 9 Low-Dispersion Flux Extraction (SWET ) Spectral data are extracted from the two-dimensional (2-D) low-dispersion resampled images (SI) using a signal weighted extraction technique (SWET ). This technique provid

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ts_update_2_14_140715.indd

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Estimating interstellar extinction toward to elliptical galaxies and star clusters (# 2188) Eduardo B. de Amôres1,2,3 and Jacques R. D. Lépine3 1Universitat de Barcelona – Spain

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Mem. S.A.It. Erratum 2 c SAIt 2006 Memorie

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Effects of granulation on Cu I resonance lines in metal-poor stars P. Bonifacio1,2,3, E. Caffau2, H.-G. Ludwig1,2 1

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INES NOISE MODEL N. Schartel1 , P. Rodr´ıguez-Pascual1,2 ESA IUE Observatory, Apartado 50727, 28080 Madrid, Spain Affiliated with the Astrophysics Division, Space Science Department ESTEC, the Netherlands 2

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FACTS KThe Benefits of Socioeconomically and Racially Integrated Schools and Classrooms FEBRUARY 10, 2016

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Chapter 3 Data Quality Flag Description For the creation of the IUE Final Archive, data quality (ν) flags are provided on a pixel-bypixel basis for the two-dimensional (2-D) photometrically corrected (LI) and geometrica

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3 2. General spacecraft description. The IUE spacecraft is shown in mission orbit configuration and in an exploded view in figures 2-1 and 2-2 respectively.

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