Soft X-Ray Spectra of AGN Discovered Via Their Hard X-Ray

机译：通过硬X射线发现aGN的软X射线光谱

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The subject of this study were Active Galactic Nuclei (AGN) with the ROSAT position sensitive proportional counter (PSPC). AGN's were first discovered via their hard (1-10 keV) X-ray emission. We selected objects identified by the scanning modulation collimator (MC), from the NRL Large Area Sky Survey catalog, at galactic latitudes greater than 20 degrees, and galactic hydrogen column density less than 3 x 10(exp 20). We have received data from observations of nine of these objects. We will report on their soft X-ray spectral shape, and on confirmation of the HEAO-1 identifications. We are especially motivated to test the hypothesis of Schwartz and Tucker that the AGN energy spectra do not have exact power laws, but exhibit constant flattening with energy. We describe a novel adaptation of the PROS software to allow us to perform fits to a Log-Gaussian spectral shape.

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作者
Schwartz, Daniel;
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年度 1998
页码 1-1
总页数 1
原文格式 PDF
正文语种 eng
中图分类工业技术;
关键词
ACTIVE GALACTIC NUCLEI; X RAY SPECTRA; X RAY ASTRONOMY; X RAY SOURCES; HEAO 1; PROPORTIONAL COUNTERS; ROSAT MISSION;

机译：活跃的GaLaCTIC NUCLEI; X射线光谱; X射线天文学; X射线源;嘿1;比例计数器;罗莎特使命;

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1. THE COSMIC MeV GAMMA-RAY BACKGROUND AND HARD X-RAY SPECTRA OF ACTIVE GALACTIC NUCLEI: IMPLICATIONS FOR THE ORIGIN OF HOT AGN CORONAE [J] . Yoshiyuki Inoue, Tomonori Totani, Yoshihiro Ueda The Astrophysical journal . 2008,第1pa2期

机译：活性银河系核的宇宙MeV伽玛射线背景和X射线硬光谱：对热银冠冕起源的启示
2. THE COSMIC MeV GAMMA-RAY BACKGROUND AND HARD X-RAY SPECTRA OF ACTIVE GALACTIC NUCLEI: IMPLICATIONS FOR THE ORIGIN OF HOT AGN CORONAE [J] . Yoshiyuki Inoue, Tomonori Totani, Yoshihiro Ueda The Astrophysical journal . 2008,第1pa2期

机译：活性银河核的宇宙MeV伽玛射线背景和X射线硬光谱：对热银冠冕起源的启示
3. A hard X-ray view of the soft excess in AGN [J] . Rozenn Boissay, Claudio Ricci, Stéphane Paltani Astronomy and astrophysics . 2016,第21期

机译：AGN中软过量的硬X射线视图
4. Reddening and the Similarity of Shapes of the Infra-Red to X-Ray Spectral Energy Distribution of AGNs: Implications for AGN Surveys and AGN Physics [C] . Gaskell C.M., Goosmann R.W., Antonucci R.J., Conference on AGN physics with the Sloan Digital Sky Survey . 2004

机译：红外线与X射线谱能量分布的红外线和X射线光谱能量分布的变红和相似性：AGN调查和AGN物理的影响
5. A Spectral Study of the Soft X-Ray Background with the X-Ray Quantum Calorimeter [D] . Wulf, Dallas W. 2018

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6. Room temperature redox reaction by oxide ion migration at carbon/Gd-doped CeO2 heterointerface probed by an in situ hard x-ray photoemission and soft x-ray absorption spectroscopies [O] . Takashi Tsuchiya, Shogo Miyoshi, Yoshiyuki Yamashita, 2013

机译：室温氧化还原反应通过原位硬X射线光发射和软X射线吸收光谱探测碳/ carbon掺杂CeO2异质界面上的氧化物离子迁移
7. X-ray spectral variability in PG 1535+547: the changing-look of a “soft X-ray weak ” AGN [O] . L. Ballo, M. Giustini, N. Schartel, 2008

机译：PG 1535 + 547中的X射线光谱变异性：“软X射线弱” AGN的外观变化

Soft X-Ray Spectra of AGN Discovered Via Their Hard X-Ray

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