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911.
将基于多重信号分类的MUSIC谱估计算法引入BL Lac天体光变周期分析中.给出了MUSIC算法的基本原理,利用模拟信号检测了算法的频谱分辨率.从大量文献中收集了BL Lac天体S5 0716+714光学V、R、I 3个波段从1994年到2008年的有效观测数据,用MUSIC算法和平均周期图算法分别计算了它们的光变周期,发现存在两个主要光变周期:一个是(3.33±0.08)yr的周期,另一个是(1.24±0.01)yr的周期.对这两种算法的周期估计性能进行了比较,结果表明,MUSIC谱估计算法对样本长度要求较低,具有良好的分辨特性和抗噪声能力,能提高在样本长度较短情况下光变周期分析的准确性. 相似文献
912.
A diverse range of crustal xenoliths is hosted in young alkalibasalt lavas and scoria deposits (erupted 35 ka) at thesummit of Huallai. Leucocratic xenoliths, including monzodiorites,diorites and syenogabbros, are distinctive among Hawaiian plutonicrocks in having alkali feldspar, apatite, zircon and biotite,and evolved mineral compositions (e.g. albitic feldspar, clinopyroxeneMg-number 6778). Fine-grained diorites and monzodioritesare plutonic equivalents of mugearite lavas, which are unknownat Huallai. These xenoliths appear to represent melt compositionsfalling along a liquid line of descent leading to trachyteamagma type which erupted from Huallai as a prodigious lava flowand scoria cone at 114 ka. Inferred fractionating assemblages,MELTS modeling, pyroxene geobarometry and whole-rock norms allpoint to formation of the parent rocks of the leucocratic xenolithsat 37 kbar pressure. This depth constraint on xenolithformation, coupled with a demonstrated affinity to hypersthene-normativebasalt and petrologic links between the xenoliths and the trachyte,suggests that the shift from shield to post-shield magmatismat Huallai was accompanied by significant deepening of the activemagma reservoir and a gradual transition from tholeiitic toalkalic magmas. Subsequent differentiation of transitional basaltsby fractional crystallization was apparently both extremeculminatingin >5·5 km3 of trachyteand rapid, at 2·75x 106 m3 magma crystallized/year. KEY WORDS: geothermobarometry; magma chamber; xenolith; cumulate; intensive parameters 相似文献
913.
为适应施工期短的严/高寒地区和近海铁路桥梁工程发展,提高铁路桥梁工程的施工效率和工程质量.文中提出了一种用于铁路桥梁工程中的模块化预制拼装实心桥墩,该桥墩不仅可以纵向节段连接,还可以通过多个可互连的模块水平连接.基于ABAQUS程序,开展了铁路桥梁模块化预制拼装桥墩在单调、往复荷载作用下力学性能数值分析,对该桥墩的承载... 相似文献
914.
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916.
介绍了GPS现代化实施后调制在L2C码和L5码上的导航电文CNAV中地球定向参数EOP、卫星导航定位系统之间的时间差参数GGTO、微分改正参数DC和卫星星历参数等新增的参数,以及这些参数相应的算法。 相似文献
917.
Nicolas Taburet Nabila Aghanim Marian Douspis Mathieu Langer 《Monthly notices of the Royal Astronomical Society》2009,392(3):1153-1158
We examine the biases induced on cosmological parameters when the presence of secondary anisotropies is not taken into account in cosmic microwave background analyses. We first develop an exact analytical expression for computing the biases on parameters when any additive signal is neglected in the analysis. We then apply it in the context of the forthcoming Planck experiment. For illustration, we investigate the effect of the sole residual thermal Sunyaev–Zel'dovich signal that remains after cluster extraction. We find, in particular, that analyses neglecting the presence of this contribution introduce on the cosmological parameters n s and τ biases, at least ∼6.5 and 2.9 times their 1σ confidence intervals. The Ωb parameter is also biased to a lesser extent. 相似文献
918.
A. Nigoche-Netro A. Ruelas-Mayorga A. Franco-Balderas 《Monthly notices of the Royal Astronomical Society》2009,392(3):1060-1069
Studying three samples of early-type galaxies, which include approximately 8800 galaxies and cover a relatively ample magnitude range (〈Δ M 〉∼ 5.5 mag) , we find that the coefficients as well as the intrinsic dispersion of the Fundamental Plane depend on the width and brightness of the magnitude range within which the galaxies are distributed. We analyse this dependence, and the results show that it is due to the fact that the distribution of galaxies in the space defined by the variables depends on the luminosity. 相似文献
919.
Surhud More † Frank C. van den Bosch Marcello Cacciato H. J. Mo Xiaohu Yang Ran Li 《Monthly notices of the Royal Astronomical Society》2009,392(2):801-816
The kinematics of satellite galaxies reflect the masses of the extended dark matter haloes in which they orbit, and thus shed light on the mass–luminosity relation (MLR) of their corresponding central galaxies. In this paper, we select a large sample of centrals and satellites from the Sloan Digital Sky Survey and measure the kinematics (velocity dispersions) of the satellite galaxies as a function of the r -band luminosity of the central galaxies. Using the analytical framework presented in More, van den Bosch & Cacciato, we use these data to infer both the mean and the scatter of the MLR of central galaxies, carefully taking account of selection effects and biases introduced by the stacking procedure. As expected, brighter centrals on average reside in more massive haloes. In addition, we find that the scatter in halo masses for centrals of a given luminosity, σlog M , also increases with increasing luminosity. As we demonstrate, this is consistent with σlog L , which reflects the scatter in the conditional probability function P ( L c | M ) , being independent of halo mass. Our analysis of the satellite kinematics yields σlog L = 0.16 ± 0.04 , in excellent agreement with constraints from clustering and group catalogues, and with predictions from a semi-analytical model of galaxy formation. We thus conclude that the amount of stochasticity in galaxy formation, which is characterized by σlog L , is well constrained, independent of halo mass and in a good agreement with current models of galaxy formation. 相似文献
920.