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: High-Resolution X-ray Spectroscopy; Instrumentation, Dat Cosimo Bambi,Jiachen Jiang Book 2023 The Editor(s) (if applicable) and The Author(

[復(fù)制鏈接]
樓主: Amalgam
31#
發(fā)表于 2025-3-26 23:34:09 | 只看該作者
978-981-99-4411-8The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
32#
發(fā)表于 2025-3-27 03:12:18 | 只看該作者
High-Resolution X-ray Spectroscopy978-981-99-4409-5Series ISSN 2731-734X Series E-ISSN 2731-7358
33#
發(fā)表于 2025-3-27 09:06:03 | 只看該作者
Book 2023rnerstone of X-ray spectroscopy since their launches more than 20 years ago. The onboard gratings provide us a unique opportunity to distinguish individual spectral lines from different atoms thanks to their high energy resolutions. Enormous discoveries have been achieved by these two missions when
34#
發(fā)表于 2025-3-27 10:20:41 | 只看該作者
35#
發(fā)表于 2025-3-27 16:27:41 | 只看該作者
36#
發(fā)表于 2025-3-27 18:06:23 | 只看該作者
37#
發(fā)表于 2025-3-28 01:41:27 | 只看該作者
XMM-Newton Reflection Grating Spectrometereter aboard XMM-Newton, which provides high-quality high-resolution spectra in the soft X-ray band. Its performance and excellent calibration quality have allowed breakthrough advancements in a wide range of astrophysical topics. For the benefit of new learners, we illustrate how to reduce RGS imaging, timing, and spectral data.
38#
發(fā)表于 2025-3-28 02:43:22 | 只看該作者
High-Resolution Spectral Analysisinds of astrophysical environments. This chapter will provide some basic commands and threads to fit high-resolution X-ray spectra of a nearby Seyfert 1 galaxy under the photoionisation equilibrium with ..
39#
發(fā)表于 2025-3-28 10:00:11 | 只看該作者
Hitomi/XRISM Micro-Calorimeteresolution of .5 eV in orbit, but it was lost after only a month of operation due to the loss of spacecraft attitude control. For the recovery mission, XRISM will be equipped with the . spectrometer which has mostly the same design as SXS and is expected to have the same in-flight performance.
40#
發(fā)表于 2025-3-28 12:47:42 | 只看該作者
Active Galactic Nuclei with High-Resolution X-Ray Spectroscopy on: (i) the relatively slow moving ionised winds known as warm absorbers and obscurers; (ii) the iron emitting from different regions of the inner and outer disc, broad line region, and torus; and (iii) the ultrafast outflows that may be the key to understanding AGN feedback.
 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 期刊點評 投稿經(jīng)驗總結(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, 2025-10-12 13:50
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
万安县| 商水县| 秦安县| 商都县| 喀喇沁旗| 栾城县| 南充市| 巴中市| 丰顺县| 廉江市| 定襄县| 涿鹿县| 连山| 霸州市| 隆昌县| 社旗县| 鹿邑县| 和硕县| 来凤县| 湘潭市| 罗平县| 黄石市| 集贤县| 张家口市| 南召县| 钦州市| 鄂伦春自治旗| 鄱阳县| 瑞丽市| 肥西县| 甘孜县| 太保市| 龙口市| 石嘴山市| 永州市| 晋宁县| 旌德县| 楚雄市| 宁武县| 浏阳市| 广州市|