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Titlebook: Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow; 3-28 August 1998 F. Casoli,J. Lequeux,F

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發(fā)表于 2025-3-21 17:48:05 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow
期刊簡稱3-28 August 1998
影響因子2023F. Casoli,J. Lequeux,F. David
視頻videohttp://file.papertrans.cn/164/163613/163613.mp4
發(fā)行地址Infrared Astronomy is a very active field and affects large parts of astronomical and cosmological research..This unique collection of high-quality lectures should attract a wide audience..Includes su
學(xué)科分類Les Houches - Ecole d‘Ete de Physique Theorique
圖書封面Titlebook: Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow; 3-28 August 1998 F. Casoli,J. Lequeux,F
影響因子This book brings together the lectures given at the Les Houches summer school "Infrared space astronomy, today and tomorrow". It gives a wide overview of infrared astronomy, a wavelength domain crucial for studies of the solar system, stars at the beginning and end of their lives, interstellar matter and galaxies at all distances. Recent developments in observational techniques have been tremendous. The first contributions give an introduction to the basic physical processes and methods of detection and data processing. They are followed by a series of lectures dealing with the wide variety of astronomical objects that can be seen in the infrared.
Pindex Conference proceedings 2000
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Some Quantitative Aspects of Galactic and Extragalactic Infrared Astronomy,Two types of infrared astrophysical problems have been intensively studied in recent years. The first is an investigation of primary coolants. The second is the nature of the diffuse extragalactic infrared background radiation.
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https://doi.org/10.1007/3-540-45573-6Cosmology; Dark Matter; Data Analysis; Galactic Structure; Infrared Astronomy; Stellar Structure; astronom
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Fluorescence methods in polymer science,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.
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發(fā)表于 2025-3-23 06:12:47 | 只看該作者
Michio Kurata,Walter H. Stockmayermmunity, covered the wavelength range from 2.5 – 240 μm at a wide variety of spectral and spatial resolutions and was operational between November 1995 and April 1998. The ISO data archive opened to the community in December 1998, at URL “www.iso.vilspa.esa.es”. The paper summarises the design and i
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