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

14.2k citations

Showing 2002 · astro-phShow all

21 papers · 2 filters

astro-ph2002★ 54 cited

Chandra Observations of the Anomalous X-ray Pulsar 4U 0142+61

Sandeep K. Patel, Chryssa Kouveliotou, Peter M. Woods +7

We present X-ray imaging, timing, and phase resolved spectroscopy of the anomalous X-ray pulsar 4U 0142+61 using the Chandra X-ray Observatory. The spectrum is well described by a…

astro-ph2002★ 2 cited

Distance Determination of Variable Galactic Sources

J. Hu, S. N. Zhang, T. P. Li

We have developed a timing analysis method to determine the distances of variable galactic X-ray sources based on the method advanced by Trümper and Schönfelder in 1973. The light-…

astro-ph2002

Relativistic Effects on the Appearance of a Clothed Black Hole

Xiaoling Zhang, S. Nan Zhang, Yuxin Feng +1

For an accretion disk around a black hole, the strong relativistic effects affect every aspect of the radiation from the disk, including its spectrum, light-curve, and image. This…

astro-ph2002★ 45 cited

A massive warm baryonic halo in the Coma cluster

M. Bonamente, M. K. Joy, R. Lieu

Several deep PSPC observations of the Coma cluster reveal a very large-scale halo of soft X-ray emission, substantially in excess of the well known radiation from the hot intra-clu…

astro-ph2002★ 5 cited

An accretion model for the growth of the central black hole associated with ionization instability in quasars

Y. Lu, K. S. Cheng, S. N. Zhang

A possible accretion model associated with the ionization instability of quasar disks is proposed to address the growth of the central black hole harbored in the host galaxy.The ma…

astro-ph2002★ 80 cited

The Properties of Microjansky Radio Sources in the HDF-N, SSA13, and SSA22 Fields

S. C. Chapman, A. J. Barger, L. L. Cowie +9

(abridged) We present multiwavelength observations for a large sample of microjansky radio sources detected in ultradeep 1.4GHz maps centered on the Hubble Deep Field-North (HDF-N)…

astro-ph2002★ 109 cited

XMM-Newton confirmation of Soft X-ray excess emission in clusters of galaxies - the discovery of O VII emission from an extended warm baryonic component

J. S. Kaastra, R. Lieu, T. Tamura +2

We investigate a sample of 14 clusters of galaxies observed with XMM-Newton in a search for soft X-ray excess emission. In five of these clusters a significant soft excess is evide…

astro-ph2002★ 29 cited

The Faint Sky Variability Survey I: Goals and data reduction process

Paul J. Groot, Paul M. Vreeswijk, Mark E. Huber

The Faint Sky Variability Survey is aimed at finding photometric and/or astrometric variable objects in the brightness range between 16<V<24 on timescales between tens of minutes a…

astro-ph2002★ 56 cited

Soft X-ray excess emission in clusters of galaxies observed with XMM-Newton

J. Nevalainen, R. Lieu, M. Bonamente +1

We present results on the spectroscopic analysis of XMM-Newton EPIC data of the central 0.5/h_50 Mpc regions of the clusters of galaxies Coma, A1795 and A3112. The temperature of t…

astro-ph2002★ 54 cited

RHESSI as a Hard X-Ray Polarimeter

M. L. McConnell, J. M. Ryan, D. M. Smith +2

Polarization measurements of hard X-rays from solar flares can provide a direct handle on the extent to which the accelerated electrons are beamed, which, in turn, has important im…

astro-ph2002★ 79 cited

How Sample Completeness Affects Gamma-Ray Burst Classification

Jon Hakkila, Timothy W. Giblin, Richard J. Roiger +3

Unsupervised pattern recognition algorithms support the existence of three gamma-ray burst classes; Class I (long, large fluence bursts of intermediate spectral hardness), Class II…

astro-ph2002★ 25 cited

A Chandra Spectroscopic Survey of Persistent Black Hole Candidates

W. Cui, Y. X. Feng, S. N. Zhang +3

We present results from observations of persistent black hole candidates with the High Energy Transmission Gratings aboard the Chandra X-ray Observatory. The sources include LMC X-…

astro-ph2002★ 10 cited

Low-energy X-ray emission from the Abell 2199 cluster of galaxies

Jelle S. Kaastra, Richard Lieu, Johan A. M. Bleeker +2

In a recent Letter, Berghoefer & Bowyer rediscussed the analysis of BeppoSAX LECS data of the cluster of galaxies Abell 2199 as presented by Kaastra et al., in particular the detec…

astro-ph2002★ 27 cited

A Comprehensive Study of Pulse Profile Evolution in SGR 1806-20 & SGR 1900+14 with the RXTE PCA

Ersin Gogus, Chryssa Kouveliotou, Peter M. Woods +2

Soft Gamma Repeaters undergo pulse profile changes in connection with their burst activity. Here we present a comprehensive pulse profile history of SGR 1806-20 and SGR 1900+14 in…

astro-ph2002★ 57 cited

The soft X-ray emission in a large sample of galaxy clusters with ROSAT PSPC

M. Bonamente, R. Lieu, M. K. Joy +1

The study of soft X-ray emission of 38 X-ray selected galaxy clusters observed by ROSAT PSPC indicates that the soft excess phenomenon may be a common occurrence in galaxy clusters…

astro-ph2002★ 29 cited

The extreme ultraviolet excess emission in five clusters of galaxies revisited

Florence Durret, Eric Slezak, Richard Lieu +2

Evidence for excess extreme ultraviolet (EUV) emission over a tail of X-ray gas bremsstrahlung emission has been building up recently, but in some cases remains controversial, most…

astro-ph2002★ 107 cited

XMM-Newton observation of the distant (z=0.6) galaxy cluster RX J1120.1+4318

M. Arnaud, S. Majerowicz, D. Lumb +12

We report on a 20 ksec XMM observation of the distant cluster RXJ1120.1+4318, discovered at z=0.6 in the SHARC survey. The cluster has a regular spherical morphology, suggesting it…

astro-ph2002★ 194 cited

Understanding the long-term spectral variability of Cygnus X-1 with BATSE and ASM observations

Andrzej A. Zdziarski, Juri Poutanen, William S. Paciesas +1

We present an analysis of all observations of Cygnus X-1 by the BATSE (20-300 keV) and by ASM (1.5-12 keV) until 2002 June, including 1200 days of simultaneous data. We find a numb…

astro-ph2002★ 11 cited

The effect of Planck scale space time fluctuations on Lorentz invariance at extreme speeds

Richard Lieu

The starting point of this work is the axiomatic existence of a smallest measurable interval, viz. the Planck time , set by quantum fluctuations in the vacuum metric tensor. B…

astro-ph2002

Extended Power-Law Decays in BATSE Gamma-Ray Bursts: Signatures of External Shocks?

T. W. Giblin, V. Connaughton, J. van Paradijs +5

The connection between Gamma-Ray Bursts (GRBs) and their afterglows is currently not well understood. Afterglow models of synchrotron emission generated by external shocks in the G…

astro-ph2002★ 74 cited

The Micro-Jansky Sky at 8.4 GHz

E. B. Fomalont, K. I. Kellermann, R. B. Partridge +2

We present the results from two radio integrations at 8.4 GHz using the VLA. One of the fields, at 13h,+43d (SA13 field), has an rms noise level of 1.49 microJy and is the deepest…