位置：成果数据库 > 期刊 > 期刊详情页
A WENO Algorithm for the Radiative Transfer and Ionized Sphere at Reionization
  • ISSN号：1384-1076
  • 期刊名称：New Astronomy
  • 时间：0
  • 页码：1-12
  • 语言：英文
  • 相关项目：宇宙恒星形成和星暴-活动星系核关联
作者： Shu, Chiwang|Fang, Lizhi|Qiu, Jingmei|Feng, Longlong|
同期刊论文项目
宇宙恒星形成和星暴-活动星系核关联
期刊论文 65 会议论文 2
同项目期刊论文
Photometry of the Cataclysmic Variables V1159 Ori and BZ UMa
Circumnuclear Star Forming Activity in NGC 3982
Fermi observations of GRB 090510: a short hard gamma-ray burst with an additional, hard power-law co
赛弗特星系恒星速度弥散度的测量
Diffuse high energy neutrinos and cosmic rays from hyperflares of soft-gamma repeaters
Klein-Nishina effects on the high-energy afterglow emission of gamma-ray bursts
IRAS F13308+5946: A Possible Transition Phase from Type I Ultraluminous Infrared Galaxy to Optical Q
Fermi detection of delayed GeV emission from the short GRB 081024B
Swift and Fermi observations of the early afterglow of the short gamma-ray burst GRB 090510
Measurements of the Stellar Velocity Dispersions of Seyfert Galaxies
Log-Poisson non-Gaussianity of Lyα transmitted flux fluctuations at high redshift
Magnetic energy injection in GRB 080913
Late-time detections of the X-ray afterglow of GRB 060729 with Chandra – the latest detections of an
The afterglow and host galaxy of GRB 090205: evidence for a Ly-alpha emitter at z=4.65
A comprehensive analysis of Fermi gamma-ray burst data. I. spectral components and their possible ph
Low-ionization galaxies and evolution in a pilot survey up to z = 1
A redshift distortio free correlation function at third order in the nonlinear regime
The quasar SDSS J142507.32+323137.4 : dual AGNs?
Surface Photometry and Radial Color Gradients of Nearby Luminous Early-type Galaxies in SDSS Stripe
Multi-Phase Dusty Gas in the Center of NGC 427
Galaxy Evolution in a Pilot Survey up to z=1 and CDM Halos
The Stellar Population and Star Formation Properties of Blue Compact Dwarf Galaxies
Broadband observations of the naked-eye gamma-ray burst GRB 080319B
Lyα leaks and reionization
A note on black hole masses estimated by the second moment in narrow-line Seyfert 1 Galaxies
An Ideal Mass Assignment Scheme for Measuring the Power Spectrum with Fast Fourier Transforms
Stellar and dust properties of local elliptical galaxies: clues to the onset of nuclear activity
DWT Power Spectrum of the Two-Degree Field Galaxy Redshift Survey
Chandra and XMM-Newton view of the warm absorbing gas in Mrk290
On the fairness of the main galaxy sample of SDSS
Early afterglows from radially structured outflows and the application to X-ray shallow decays
An optimal method for the power spectrum measurement
Discerning the physical origins of cosmological gamma-ray bursts based on multiple observational cri
Clustering of K-band selected local galaxies
Recent star-forming activity in local elliptical galaxies
Stellar ages and metallicities of nearby elliptical galaxies
A limit on the variation of the speed of light arising from quantum gravity effects
GRB 080913 at redshift 6.7
Scaling relation between Sunyaev Zel’dovich effect and X-ray luminosity and scale-free evolution of
Spectral Properties from Lyα to Hα for an Essentially Complete Sample of Quasars. I. Data
Fermi observations of high-energy gamma-ray emission from GRB 080916C
21 cm Signals from Early Ionizing Sources
The Eddington Ratios in Seyfert 2 Galaxies with and without Hidden Broad-Line Regions
Fractional Brownian motion and the halo mass function
The dependence of quasar variability on black hole mass
Note on Redshift Distortion in Fourier Space
Scale transformations, tree-level perturbation theory and the cosmological matter bispectrum
X-ray flares from late internal and late external shocks
A Study of the Star-forming Dwarf Galaxy NGC 855 with Spitzer
Active Galactic Nuclei with Double-Peaked Balmer Lines. I. Black Hole Masses and Eddington Ratios
Direct Evidence from Spitzer for a low-luminosity AGN at the center of the Elliptical Galaxy NGC 315
CDFS天区中暗蓝星系的测光红移研究
Serendipitous discovery of warm absorbers in the Seyfert 2 galaxy IRAS 18325-5926
Low-ionization galaxies and evolution in a pilot survey up to z=1