找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: ;

[復制鏈接]
樓主: estradiol
11#
發(fā)表于 2025-3-23 12:11:46 | 只看該作者
12#
發(fā)表于 2025-3-23 17:30:13 | 只看該作者
The Spatial Clustering of X-ray Selected AGN in the Chandra Msec Fields,andra Deep Field South (CDFS). The AGN clustering amplitude, measured for sources with median luminosity .~ 10. erg?s. and at a median redshift of ~ 0.9, is found to be a factor of ~ 2 higher in the CDFS than in the CDFN, revealing large cosmic variance in these 0.1 deg. fields. The extra correlatio
13#
發(fā)表于 2025-3-23 18:39:43 | 只看該作者
What Powers High-Redshift SCUBA Galaxies?,e 2?Ms . Deep Field-North) and deep optical spectroscopic data. Even though a large fraction of high-redshift SCUBA galaxies host AGN activity (upward of 38%), we argue that in almost all cases the AGNs are not bolometrically important (i.e., contribute <20% of the energetics). Thus, most high-redsh
14#
發(fā)表于 2025-3-24 01:25:17 | 只看該作者
Early Spitzer Detections of Extreme X-ray/Optical Sources (EXOs),ray sources are completely undetected in our deep optical GOODS HST/ACS imaging, to limits that place them at the extreme end of the .x/. parameter space, with values about 100 to 1000 times higher than generally found for Active Galactic Nuclei (AGN). We use their Spitzer detections to investigate
15#
發(fā)表于 2025-3-24 02:55:26 | 只看該作者
Why Are Only High-Redshift Obscured AGN Bright Submillimeter Sources?,]. We have used sensitive submillimetre (submm) observations?[8,9,12] (using SCUBA at the JCMT) to show that the submm luminosities of unabsorbed and absorbed broad line QSO in those intervals are radically different (>3.): only 1 out of 20 unabsorbed QSO has been detected, while 8 out of 19 absorbe
16#
發(fā)表于 2025-3-24 06:56:38 | 只看該作者
17#
發(fā)表于 2025-3-24 13:20:46 | 只看該作者
XMM-Newton Observations of Four High-z Quasars, most luminous and distant sources of electromagnetic radiation known. The X-ray emission gives insight into the accretion mechanisms onto super-massive black holes. Current questions are whether quasars exhibit spectral evolution or not and whether absorption in excess of the galactic . is a genera
18#
發(fā)表于 2025-3-24 14:49:28 | 只看該作者
19#
發(fā)表于 2025-3-24 19:26:20 | 只看該作者
https://doi.org/10.1007/978-94-011-5129-0inciple of ., by which supermassive black holes grow until they release sufficient energy to unbind the gas that feeds them from their host galaxy. This principle explains several observed facts, including the correlation between the mass of a central black hole and the depth of the gravitational po
20#
發(fā)表于 2025-3-24 23:24:32 | 只看該作者
 關于派博傳思  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 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結 SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-5 21:30
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
务川| 梓潼县| 巴中市| 隆安县| 长丰县| 望谟县| 宝山区| 莎车县| 茌平县| 龙陵县| 吉安县| 安宁市| 饶阳县| 吴旗县| 黄山市| 文登市| 聂拉木县| 阳高县| 迁安市| 通榆县| 阿尔山市| 蓬莱市| 荆门市| 贵港市| 宜宾县| 五指山市| 安塞县| 柳江县| 阿鲁科尔沁旗| 保德县| 忻州市| 和田县| 灵宝市| 新安县| 密云县| 上蔡县| 和顺县| 昌平区| 巴东县| 襄汾县| 买车|