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(fù)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(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 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| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-6 15:55
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
云浮市| 闽清县| 城市| 齐河县| 资阳市| 武安市| 民和| 莫力| 武汉市| 云霄县| 抚远县| 板桥市| 忻城县| 金寨县| 丰城市| 三都| 云和县| 广西| 柘荣县| 甘德县| 高州市| 左云县| 鄂伦春自治旗| 泰和县| 都匀市| 都昌县| 会东县| 高淳县| 揭阳市| 兴安盟| 安远县| 蒲江县| 兴城市| 广德县| 濮阳县| 屏东市| 汪清县| 建始县| 荣成市| 息烽县| 彰化县|