找回密碼
 To register

QQ登錄

只需一步,快速開(kāi)始

掃一掃,訪問(wèn)微社區(qū)

打印 上一主題 下一主題

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

[復(fù)制鏈接]
查看: 15885|回復(fù): 51
樓主
發(fā)表于 2025-3-21 17:32:35 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
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

書(shū)目名稱(chēng)High-Redshift Galaxies影響因子(影響力)




書(shū)目名稱(chēng)High-Redshift Galaxies影響因子(影響力)學(xué)科排名




書(shū)目名稱(chēng)High-Redshift Galaxies網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱(chēng)High-Redshift Galaxies網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱(chēng)High-Redshift Galaxies被引頻次




書(shū)目名稱(chēng)High-Redshift Galaxies被引頻次學(xué)科排名




書(shū)目名稱(chēng)High-Redshift Galaxies年度引用




書(shū)目名稱(chēng)High-Redshift Galaxies年度引用學(xué)科排名




書(shū)目名稱(chēng)High-Redshift Galaxies讀者反饋




書(shū)目名稱(chēng)High-Redshift Galaxies讀者反饋學(xué)科排名




單選投票, 共有 1 人參與投票
 

0票 0.00%

Perfect with Aesthetics

 

1票 100.00%

Better Implies Difficulty

 

0票 0.00%

Good and Satisfactory

 

0票 0.00%

Adverse Performance

 

0票 0.00%

Disdainful Garbage

您所在的用戶(hù)組沒(méi)有投票權(quán)限
沙發(fā)
發(fā)表于 2025-3-21 22:09:46 | 只看該作者
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
板凳
發(fā)表于 2025-3-22 01:54:13 | 只看該作者
地板
發(fā)表于 2025-3-22 05:02:22 | 只看該作者
5#
發(fā)表于 2025-3-22 12:44:12 | 只看該作者
6#
發(fā)表于 2025-3-22 14:31:47 | 只看該作者
7#
發(fā)表于 2025-3-22 20:25:42 | 只看該作者
8#
發(fā)表于 2025-3-22 23:22:32 | 只看該作者
9#
發(fā)表于 2025-3-23 03:32:21 | 只看該作者
10#
發(fā)表于 2025-3-23 07:03:41 | 只看該作者
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛(ài)論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-5 02:39
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
永清县| 奉节县| 上饶市| 错那县| 田林县| 鸡西市| 洪洞县| 吐鲁番市| 隆昌县| 页游| 洞头县| 营山县| 思茅市| 延长县| 宜春市| 仁化县| 永修县| 万荣县| 陆川县| 普兰店市| 克拉玛依市| 和平区| 塔河县| 巫溪县| 汉沽区| 满洲里市| 丰镇市| 兴山县| 长汀县| 云霄县| 潢川县| 义乌市| 明星| 益阳市| 石门县| 任丘市| 泸定县| 乌拉特中旗| 伊宁县| 大丰市| 册亨县|