output
19942026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2005 · astro-phShow all

18 papers · 2 filters

astro-ph2005★ 9 cited

ROSAT observations of the soft X-ray background and of the cluster soft excess emission in the Hercules supercluster

Max Bonamente, Richard Lieu, Jelle Kaastra

Recent observations with the XMM-Newton satellite confirmed the existence of the soft excess phenomenon in galaxy clusters, earlier discovered in several EUVE, ROSAT and BeppoSAX o…

astro-ph2005★ 30 cited

GRB 050911: a black hole - neutron star merger or a naked GRB

K. L. Page, A. R. King, A. J. Levan +16

GRB 050911, discovered by the Swift Burst Alert Telescope, was not seen 4.6 hr later by the Swift X-ray Telescope, making it one of the very few X-ray non-detections of a Gamma-Ray…

astro-ph2005★ 355 cited

Determination of the Cosmic Distance Scale from Sunyaev-Zel'dovich Effect and Chandra X-ray Measurements of High Redshift Galaxy Clusters

M. Bonamente, M. Joy, S. La Roque +3

We determine the distance to 38 clusters of galaxies in the redshift range 0.14 < z < 0.89 using X-ray data from Chandra and Sunyaev-Zeldovich Effect data from the Owens Valley Rad…

astro-ph2005★ 9 cited

Cross-Correlation analysis of WMAP and EGRET in Wavelet Space

Xin Liu, Shuang Nan Zhang

We cross correlate the Wilkinson Microwave Anisotropy Probe (WMAP) first year data and the diffuse gamma-ray intensity maps from the Energetic Gamma Ray Experiment Telescope (EGRET…

astro-ph2005

Magnetic topologies and two-class coronal mass ejections: a numerical magnetohydrodynamic study

W. Liu, X. P. Zhao, S. T. Wu +1

White-light observations of the solar corona show that there are two characteristic types of Coronal Mass Ejections (CMEs) in terms of speed-height profiles: so-called fast CMEs th…

astro-ph2005★ 33 cited

Forming supermassive black holes by accreting dark and baryon matter

Jian Hu, Yue Shen, Yu-Qing Lou +1

Given a large-scale mixture of self-interacting dark matter (SIDM) particles and baryon matter distributed in the early Universe, we advance here a two-phase accretion scenario for…

astro-ph2005★ 56 cited

The Sunyaev-Zel'dovich effect in a sample of 31 clusters - a comparison between the X-ray predicted and WMAP observed CMB temperature decrement

Richard Lieu, Jonathan P. D. Mittaz, Shuang-Nan Zhang

The WMAP Q, V, and W band radial profiles of temperature deviation of the cosmic microwave background (CMB) were constructed for a sample of 31 randomly selected nearby clusters of…

astro-ph2005★ 6 cited

CASTER - a concept for a Black Hole Finder Probe based on the use of new scintillator technologies

Mark L. McConnell, Peter F. Bloser, Gary Case +13

The primary scientific mission of the Black Hole Finder Probe (BHFP), part of the NASA Beyond Einstein program, is to survey the local Universe for black holes over a wide range of…

astro-ph2005★ 22 cited

Black hole X-ray binaries LMC X-1 and X-3: observations confront spectral models

Yangsen Yao, Q. Daniel Wang, Shuang Nan Zhang

We present a comprehensive spectral analysis of black hole X-ray binaries, LMC X-1 and LMC X-3, based on BeppoSAX observations. We test both the multi-color disk plus power law (MC…

astro-ph2005★ 19 cited

Critical Examinations of QSO Redshift Periodicities and Associations with Galaxies in Sloan Digital Sky Survey Data

Su Min Tang, Shuang Nan Zhang

We have used the publicly available data from the Sloan Digital Sky Survey and 2dF QSO Redshift Survey to test the hypothesis that QSOs are ejected from active galaxies with period…

astro-ph2005★ 35 cited

The temperature structure in the core of Sersic 159-03

J. de Plaa, J. S. Kaastra, M. Mendez +6

We present results from a new 120 ks XMM-Newton observation of the cluster of galaxies Sersic 159-03. In this paper we focus on the high-resolution X-ray spectra obtained with the…

astro-ph2005★ 20 cited

Thermal and non-thermal nature of the soft excess emission from Sersic 159-03 observed with XMM-Newton

M. Bonamente, R. Lieu, J. P. D. Mittaz +2

Several nearby clusters exhibit an excess of soft X-ray radiation which cannot be attributed to the hot virialized intra-cluster medium. There is no consensus to date on the origin…

astro-ph2005★ 33 cited

Probing the Spatial Distribution of the Interstellar Dust Medium by High Angular Resolution X-ray Halos of Point Sources

Jingen Xiang, Shuang Nan Zhang, Yangsen Yao

We studied the X-ray dust scattering halos around 17 bright X-ray point sources using {\it Chandra} data. We use an iterative method to resolve the halos at small scattering angles…

astro-ph2005★ 20 cited

Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches

Xin Liu, Shuang Nan Zhang

We perform multi-scale non-Gaussianity detection and localization to the Wilkinson Microwave Anisotropy Probe (WMAP) first-year data in both wavelet and real spaces. Such an analys…

astro-ph2005★ 74 cited

Submillimetre photometry of X-ray absorbed QSOs: their formation and evolutionary status

J. A. Stevens, M. J. Page, R. J. Ivison +4

We present an analysis of the submillimetre/X-ray properties of 19 X-ray absorbed, Compton-thin quasi-stellar objects (QSOs) selected to have luminosities and redshifts which repre…

astro-ph2005★ 36 cited

The transient hard X-ray tail of GX 17+2: new BeppoSAX results

R. Farinelli, F. Frontera, A. A. Zdziarski +5

We report on results of two BeppoSAX observations of the Z source GX 17+2. In both cases the source is in the horizontal branch of the colour-intensity diagram. The persistent cont…

astro-ph2005★ 4 cited

The Cluster Soft Excess: new faces of an old enigma

Richard Lieu, Jonathan Mittaz

Until the advent of XMM-Newton, the cluster soft excess (CSE) was the subject of some controversy due to both data analysis issues and uncertainties with the soft excess emission m…

astro-ph2005★ 153 cited

Testing the Gamma-Ray Burst Energy Relationships

David L. Band, Robert D. Preece

Building on Nakar & Piran's analysis of the Amati relation relating gamma-ray burst peak energies E_p and isotropic energies E_iso, we test the consistency of a large sample of BAT…