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

14.2k citations

Showing 2000 · astro-phShow all

27 papers · 2 filters

astro-ph2000★ 38 cited

SW Sextantis in an excited, low state

Paul J Groot, Rene' G. M. Rutten, Jan van Paradijs

We present low-resolution spectrophotometric optical observations of the eclipsing nova-like cataclysmic variable SW Sex, the prototype of the SW Sex stars. We observed the system…

astro-ph2000

EUV and soft X-rays from clusters of galaxies - the `cluster soft-excess' phenomenon

Max Bonamente, Richard Lieu

Clusters of galaxies are strong emitters of EUV and soft X-rays substantially in excess of the contribution from the hot intra-cluster medium at X-ray temperatures. After the initi…

astro-ph2000★ 170 cited

Galaxy Cluster Gas Mass Fractions from Sunyaev-Zel'dovich Effect Measurements: Constraints on Omega_M

Laura Grego, John E. Carlstrom, Erik D. Reese +5

Using sensitive centimeter-wave receivers mounted on the Owens Valley Radio Observatory and Berkeley-Illinois-Maryland-Association millimeter arrays, we have obtained interferometr…

astro-ph2000

Mining Gamma-Ray Burst Data

Jon Hakkila, Richard J. Roiger, David J. Haglin +3

Gamma-ray bursts provide what is probably one of the messiest of all astrophysical data sets. Burst class properties are indistinct, as overlapping characteristics of individual bu…

astro-ph2000★ 41 cited

The EUV excess emission of the Virgo and A1795 clusters - re-observation with in-situ background measurements

Max Bonamente, Richard Lieu, Jonathan P. D. Mittaz

The Virgo and A1795 clusters of galaxies were re-observed by EUVE with {\it in situ} background measurements by pointing at small offsets. Earlier, a similar re-observational strat…

astro-ph2000★ 74 cited

The nature of the bright submillimeter galaxy population: a radio pre-selected sample with I>25

S. C. Chapman, E. Richards, G. Lewis +2

Deep submillimetre surveys have successfully detected distant, star-forming galaxies, enshrouded in vast quantities of dust and which emit most of their energy at far infrared wave…

astro-ph2000★ 2 cited

EUV and X-ray observations of Abell 2199: a three-phase intracluster medium with a massive warm component

Richard Lieu, Max Bonamente, Jonathan P. D. Mittaz

Various independent ways of constraining key cosmological parameters yielded a consensus range of values which indicates that at the present epoch the bulk of the universe's baryon…

astro-ph2000★ 10 cited

VLT identification of the optical afterglow of the gamma-ray burst GRB 000131 at z=4.50

M. I. Andersen, J. Hjorth, H. Pedersen +16

We report the discovery of the gamma-ray burst GRB 000131 and its optical afterglow. The optical identification was made with the VLT 84 hours after the burst following a BATSE det…

astro-ph2000★ 22 cited

Search for Millisecond Periodicities in Type I X-ray Bursts of the Rapid Burster

D. W. Fox, W. H. G. Lewin, R. E. Rutledge +8

We have searched the rising portion of type I X-ray bursts observed from the Rapid Burster with the Rossi X-ray Timing Explorer for the presence of periodicities. The 95 per cent c…

astro-ph2000★ 120 cited

VLT spectroscopy of GRB 990510 and GRB 990712; probing the faint and bright end of the GRB host galaxy population

P. M. Vreeswijk, A. Fruchter, L. Kaper +15

We present time-resolved optical spectroscopy of the afterglows of the gamma-ray bursts GRB 990510 and GRB 990712. Through the identification of several absorption lines in the fir…

astro-ph2000★ 29 cited

The multiphase nature of the intra-cluster medium of some clusters of galaxies

Max Bonamente, Richard Lieu, Jonathan P. D. Mittaz

The discovery of EUV and soft X-ray excess emission in clusters of galaxies (the cluster soft-excess phenomenon) challenged the notion of the hot ( K) gas as the onl…

astro-ph2000★ 75 cited

An Unusual Burst from Soft Gamma Repeater SGR 1900+14: Comparisons with Giant Flares and Implications for the Magnetar Model

Alaa I. Ibrahim, Tod E. Strohmayer, Peter M. Woods +6

The Soft Gamma Repeater SGR 1900+14 entered a remarkable phase of activity during the summer of 1998. This activity peaked on August 27, 1998 when a giant periodic gamma-ray flare…

astro-ph2000★ 65 cited

GRB990712: First Indication of Polarization Variability in a Gamma-ray Burst Afterglow

E. Rol, R. A. M. J. Wijers, P. M. Vreeswijk +9

We report the detection of significant polarization in the optical afterglow of GRB990712 on three instances 0.44, 0.70 and 1.45 days after the gamma-ray burst, with (P, theta) bei…

astro-ph2000★ 10 cited

Detailed Analysis of the Pulsations During and After Bursts from the Bursting Pulsar (GRO J1744-28)

Peter M. Woods, Chryssa Kouveliotou, Jan van Paradijs +5

The hard X-ray bursts observed during both major outbursts of the Bursting Pulsar (GRO J1744-28) show pulsations near the neutron star spin frequency with an enhanced amplitude rel…

astro-ph2000★ 52 cited

Timing Noise in SGR 1806-20

Peter M. Woods, Chryssa Kouveliotou, Mark H. Finger +9

We have phase connected a sequence of RXTE PCA observations of SGR 1806-20 covering 178 days. We find a simple secular spin-down model does not adequately fit the data. The period…

astro-ph2000★ 49 cited

Discovery of the optical counterpart and early optical observations of GRB990712

Kailash C. Sahu

We present the discovery observations of the optical counterpart of the gamma-ray burster GRB990712 taken 4.16 hours after the outburst and discuss its light curve observed in the…

astro-ph2000★ 46 cited

The Sunyaev-Zel'dovich Effect in Abell 370

Laura Grego, John E. Carlstrom, Marshall K. Joy +5

We present interferometric measurements of the Sunyaev-Zel'dovich (SZ) effect towards the galaxy cluster Abell 370. These measurements, which directly probe the pressure of the clu…

astro-ph2000★ 5 cited

Searching for periodicities in the MACHO light curve of LMC X-2

C. Alcock, R. A. Allsman, D. R. Alves +23

Using the exceptional long-term monitoring capabilities of the MACHO project, we present here the optical history of LMC X-2 for a continuous 6-yr period. These data were used to i…

astro-ph2000★ 86 cited

Three-Layered Atmospheric Structure in Accretion Disks Around Stellar-Mass Black Holes

S. N. Zhang, Wei Cui, Wan Chen +5

Modeling of the x-ray spectra of the Galactic superluminal jet sources GRS 1915+105 and GRO J1655-40 reveal a three-layered atmospheric structure in the inner region of their accre…

astro-ph2000★ 163 cited

Statistical properties of SGR 1806-20 bursts

Ersin Gogus, Peter M. Woods, Chryssa Kouveliotou +4

We present statistics of SGR 1806-20 bursts, combining 290 events detected with RXTE/PCA, 111 events detected with BATSE and 134 events detected with ICE. We find that the fluence…

astro-ph2000★ 77 cited

Simultaneous Measurements of X-Ray Luminosity and Kilohertz Quasi-Periodic Oscillations in Low-Mass X-Ray Binaries

Eric C. Ford, Michiel van der Klis, Mariano Mendez +4

We measure simultaneously the properties of the energy spectra and the frequencies of the kilohertz quasi-periodic oscillations (QPOs) in fifteen low mass X-ray binaries covering a…

astro-ph2000★ 86 cited

The power spectral properties of the Z-source GX 340+0

Peter G. Jonker, Michiel van der Klis, Rudy Wijnands +6

We present an analysis of ~390 ksec of data of the Z source GX 340+0 taken during 24 observations with the Rossi X-ray Timing Explorer satellite. We report the discovery of a new b…

astro-ph2000★ 20 cited

Spectral Evolution of the Peculiar Ic Supernova 1998bw

R. A. Stathakis, B. J. Boyle, D. H. Jones +13

SN 1998bw holds the record for the most energetic Type Ic explosion, one of the brightest radio supenovae and probably the first supernova associated with a gamma-ray burst. In thi…

astro-ph2000★ 24 cited

Irradiation of the secondary star in X-ray Nova Scorpii 1994 (=GRO J1655--40)

T. Shahbaz, P. Groot, S. N. Phillips +3

We have obtained intermediate resolution optical spectra of the black-hole candidate Nova Sco 1994 in June 1996, when the source was in an X-ray/optical active state (R~15.05). We…