两类长γ暴的傅里叶功率谱

分析了Balastegui等（2001）应用神经网络划分出的两类长γ暴的平均傅里叶功率谱（PDS），两类暴的平均PDS都具有明显的幂律谱结构，对两类暴分别按亮度和能谱硬度分组，计算各组的平均功率谱，两类暴都具有平均功率谱随亮度和能谱硬度的增加而变平的趋势。     

A Restriction on the Duration and Peak Energy of Gamma-Ray Bursts

Two dimensional distributions of T90 versus Epeak(or Ebreak)for three bright GRB samples have been investigated.The result shows that although both T90 and Epeak(or Ebreak) each span over a wide range,they are restricted to the region log(T90)≤－log(Epeak) 5.24.This cannot be explained by the current fireball model.It may represent a constraint on the fireball model.     

Spectral Properties of Anomalous X-ray Pulsars

We examine the spectra of the persistent emission from anomalous X-ray pulsars (AXPs) and their variati on with the spin-down rate Ω. Based onan accretion-powered model, the influences of both the magnetic field and the mass accretion rate on the spectral properties of AXPs are addressed. We then investigate the relation between the spectral property of AXPs and mass accretion rate M. The result shows that there exists a linear correlation between the photon index and the mass accretion rate: the spectral hardness increases with increasing M. A possible emission mechanism for the explanation of the spectral properties of AXPs is also discussed.     

Learning Vector Quantization for Classifying Astronomical Objects

The sizes of astronomical surveys in different wavebands are increasing rapidly. Therefore, automatic classification of objects is becoming ever more important. We explore the performance of learning vector quantization (LVQ) in classifying multi-wavelength data. Our analysis concentrates on separating active sources from non-active ones. Different classes of X-ray emitters populate distinct regions of a multidimensional parameter space. In order to explore the distribution of various objects in a multidimensional parameter space, we positionally cross-correlate the data of quasars, BL Lacs, active galaxies, stars and normal galaxies in the optical, X-ray and infrared bands. We then apply LVQ to classify them with the obtained data. Our results show that LVQ is an effective method for separating AGNs from stars and normal galaxies with multi-wavelength data.     

成像硬X射线望远镜在美国和欧洲的发展

硬X射线能带（20KeV-1MeV)是我们了解天体物理中高能辐射过程的一个好窗口。成像硬X射线望远镜可以提供更好的分辨率和灵敏度来研究硬X射线天体物理学。本文介绍了成像硬X射线望远镜在美国和欧洲的发展，这包括：1）EXITE2，由美国哈佛－史密松林天体物理中心设计和运行的一个光电开关成像硬X射线望远镜；2）EXIST，一个成像硬X射线全天巡天望远镜，将于2010年由ULDB（EXIST－LINE）或国际空间站（EXIST－ISS）承载；3）HERO，由NASA／MSFC建造的一个新的硬X射线光学仪器。     

月球伽玛射线谱仪的研制及其性能

介绍将用于中国第一颗月球探测卫星主载荷之一的伽玛射线谱仪的结构设计, Monte Carlo模拟结果和原理样机性能测试结果等．该探测器采用CsI(T1)晶体作为闪烁体和反符合技术抑制本底,可探测的射线能量范围为0．3-9．0 MeV,仪器能量分辨率是9．0％(662 keV)．