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Titlebook: High-Redshift Galaxies; Light from the Early Immo Appenzeller Book 20091st edition Springer-Verlag Berlin Heidelberg 2009 Cosmology.Dark En

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書(shū)目名稱(chēng)High-Redshift Galaxies
副標(biāo)題Light from the Early
編輯Immo Appenzeller
視頻videohttp://file.papertrans.cn/427/426717/426717.mp4
概述Very timely book on very active research field with relevance to Cosmology and Fundamental Physics.Provides a comprehensive account of the scientific results on high-redshift galaxies accumulated duri
叢書(shū)名稱(chēng)Astronomy and Astrophysics Library
圖書(shū)封面Titlebook: High-Redshift Galaxies; Light from the Early Immo Appenzeller Book 20091st edition Springer-Verlag Berlin Heidelberg 2009 Cosmology.Dark En
描述The high-redshift galaxies became a distinct research ?eld during the ?nal decade of the20thcentury. AtthattimetheLyman-breaktechniquemadeitpossibletoidentify signi?cant samples of such objects, and the new generation of 8 to 10-m telescopes resulted in ?rst good spectroscopic data. Today the high-redshift galaxies have developed into one of the important topics of astrophysics, accounting for about 5–10% of the publications in the major scienti?c journals devoted to astronomy. Because high-redshift galaxies is a rapidly developing ?eld and since new results are published constantly, writing a book on this topic is challenging. On the other hand, in view of the large amount of individual results now in the literature, and in view of the still growing interest in this topic, it appears worthwhile to summarize and evaluate the available data and to provide an introduction for those who wish to enter this ?eld, or who, for various reasons, might be interested in its results. The end of the ?rst decade of the 21st century appears to be a good point in time to attempt such a summary. The current generation of ground-based 8 to 10-m - optical telescopes, the Hubble Space Telescope, and t
出版日期Book 20091st edition
關(guān)鍵詞Cosmology; Dark Energy; Dark Matter; Early Universe; Galaxy Formation; High-Redshift Galaxies; IGM; Interga
版次1
doihttps://doi.org/10.1007/978-3-540-75824-2
isbn_softcover978-3-662-51810-6
isbn_ebook978-3-540-75824-2Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 2009
The information of publication is updating

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The Nearby Universeght fluxes, and a low surface brightness. Therefore, when observing such objects, one normally has to make do with low spatial and spectral resolutions, and (due to photon noise) with low signal-to-noise ratios. As a result, the direct information content of such data is always rather limited. In or
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