decipher
发表于 2025-3-26 23:34:09
978-981-99-4411-8The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
制度
发表于 2025-3-27 03:12:18
High-Resolution X-ray Spectroscopy978-981-99-4409-5Series ISSN 2731-734X Series E-ISSN 2731-7358
半导体
发表于 2025-3-27 09:06:03
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
才能
发表于 2025-3-27 10:20:41
http://reply.papertrans.cn/43/4268/426739/426739_34.png
凝结剂
发表于 2025-3-27 16:27:41
http://reply.papertrans.cn/43/4268/426739/426739_35.png
POLYP
发表于 2025-3-27 18:06:23
http://reply.papertrans.cn/43/4268/426739/426739_36.png
Morphine
发表于 2025-3-28 01:41:27
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.
影响带来
发表于 2025-3-28 02:43:22
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 ..
heterodox
发表于 2025-3-28 10:00:11
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.
corpuscle
发表于 2025-3-28 12:47:42
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.