output
19922026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2002 · astro-phShow all

28 papers · 2 filters

astro-ph2002★ 33 cited

Observations of giant outbursts from Cygnus X-1

S. Golenetskii, R. Aptekar, D. Frederiks +5

We present interplanetary network localization, spectral, and time history information for 7 episodes of exceptionally intense gamma-ray emission from Cygnus X-1. The outbursts occ…

astro-ph2002★ 57 cited

Multiple Methods for Estimating the Bispectrum of the Cosmic Microwave Background with Application to the MAXIMA Data

M. G. Santos, A. Heavens, A. Balbi +11

We describe different methods for estimating the bispectrum of Cosmic Microwave Background data. In particular we construct a minimum variance estimator for the flat-sky limit and…

astro-ph2002★ 85 cited

XMM-Newton observations of PSR B1823-13: An asymmetric synchrotron nebula around a Vela-like pulsar

Bryan Gaensler, Norbert Schulz, Vicky Kaspi +2

We present a deep observation with the X-ray Multi-Mirror Mission of PSR B1823-13, a young pulsar with similar properties to the Vela pulsar. We detect two components to the X-ray…

astro-ph2002★ 554 cited

High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies

J. R. Peterson, S. M. Kahn, F. B. S. Paerels +5

We present high resolution X-ray spectra of 14 putative cooling-flow clusters of galaxies obtained with the Reflection Grating Spectrometer on XMM-Newton. The clusters in the sampl…

astro-ph2002★ 2 cited

Hidden Subluminous sd/wd among the FAUST UV sources toward OPHIUCHUS

Liliana Formiggini

A UV image in the direction of Ophiuchus, obtained with the FAUST instrument is analysed. Suitable candidates as unrecognized subluminous stars are selected comparing the observed…

astro-ph2002★ 90 cited

Confirmation of Two Cyclotron Lines in Vela X-1

I. Kreykenbohm, W. Coburn, J. Wilms +4

We present pulse phase-resolved X-ray spectra of the high mass X-ray binary Vela X-1 using the Rossi X-ray Timing Explorer. We observed Vela X-1 in 1998 and 2000 with a total obser…

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★ 55 cited

Orbital and Super-Orbital Periods of 1E 1740.7-2942 and GRS 1758-258

D. M. Smith, W. A. Heindl, J. H. Swank

Five years of Rossi X-ray Timing Explorer (RXTE) observations of the Galactic black-hole candidates 1E 1740.7-2942 and GRS 1758-258 show a periodic modulation with amplitude 3-4% i…

astro-ph2002★ 10 cited

Chandra High Resolution Camera Imaging of GRS 1758-258

W. A. Heindl, D. M. Smith

We observed the "micro-quasar" GRS 1758-258 four times with Chandra. Two HRC-I observations were made in 2000 September-October spanning an intermediate-to-hard spectral transition…

astro-ph2002★ 90 cited

Discovery of GRB 020405 and its Late Red Bump

P. A. Price, S. R. Kulkarni, E. Berger +41

We present the discovery of GRB 020405 made with the Inter-Planetary Network (IPN). With a duration of 60 s, the burst appears to be a typical long duration event. We observed the…

astro-ph2002★ 99 cited

The Faint Optical Afterglow and Host Galaxy of GRB 020124: Implications for the Nature of Dark Gamma-Ray Bursts

E. Berger, S. R. Kulkarni, J. S. Bloom +24

We present ground-based optical observations of GRB 020124 starting 1.6 hours after the burst, as well as subsequent Very Large Array (VLA) and Hubble Space Telescope (HST) observa…

astro-ph2002★ 358 cited

Magnetic Fields of Accreting X-Ray Pulsars with the Rossi X-Ray Timing Explorer

W. Coburn, W. A. Heindl, R. E. Rothschild +5

Using a consistent set of models, we parameterized the X-ray spectra of all accreting pulsars in the Rossi X-ray Timing Explorer database which exhibit Cyclotron Resonance Scatteri…

astro-ph2002★ 30 cited

GRB 010921: Strong Limits on an Underlying Supernova from HST

P. A. Price, S. R. Kulkarni, B. P. Schmidt +24

GRB 010921 was the first HETE-2 GRB to be localized via its afterglow emission. The low-redshift of the host galaxy, z=0.451, prompted us to undertake intensive multi-color observa…

astro-ph2002★ 65 cited

The Pulsar Wind Nebula in G11.2-0.3

Mallory S. E. Roberts, Cindy R. Tam, Victoria M. Kaspi +5

We present an X-ray and radio study of the wind nebula surrounding the central pulsar PSR J1811-1925 in the supernova remnant G11.2-0.3. Using high resolution data obtained with th…

astro-ph2002★ 59 cited

Imaging the disk around the luminous young star LkHalpha 101 with infrared interferometry

P. G. Tuthill, J. D. Monnier, W. C. Danchi +2

The Herbig Ae/Be star LkHalpha 101 has been imaged at high angular resolution at a number of wavelengths in the near-infrared (from 1 to 3 microns) using the Keck 1 Telescope, and…

astro-ph2002★ 137 cited

Spectral analysis of 35 GRBs/XRFs observed with HETE-2/FREGATE

C. Barraud, J-F. Olive, J. P. Lestrade +27

We present a spectral analysis of 35 GRBs detected with the HETE-2 gamma-ray detectors (the FREGATE instrument) in the energy range 7-400 keV. The GRB sample analyzed is made of GR…

astro-ph2002★ 114 cited

The distant Type Ia supernova rate

R. Pain, S. Fabbro, M. Sullivan +26

We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample, which su…

astro-ph2002★ 15 cited

An EUV Study of the Intermediate Polar EX Hydrae

Kunegunda E. Belle, Steve B. Howell, Martin Sirk +1

On 2000 May 5, we began a large multi-wavelength campaign to study the intermediate polar, EX Hydrae. The simultaneous observations from six satellites and four telescopes were cen…

astro-ph2002★ 77 cited

New Tests of Magnetospheric Accretion in T Tauri Stars

Christopher M. Johns-Krull, April D. Gafford

We examine 3 analytic theories of magnetospheric accretion onto classical T Tauri stars under the assumption that the magnetic field strength does not vary appreciably from star to…

astro-ph2002★ 9 cited

Measuring the Boundary Layer and Inner Accretion Disk Temperatures for WX Ceti During Superoutburst

S. B. Howell, R. Fried, P. Szkody +2

We obtained EUV photometry, optical spectroscopy, and multi-color optical photometry for WX Cet during its 1998 November superoutburst. WX Cet is only the second short-period, low…

astro-ph2002

Subluminous Stars among the FAUST UV sources toward OPHIUCHUS

L. Formiggini, N. Brosch, E. Almoznino +2

We present results of an analysis of a UV image in the direction of Ophiuchus, obtained with the FAUST instrument. The image contains 228 UV sources. Most of these were identified…

astro-ph2002★ 105 cited

GRB 011121: A Massive Star Progenitor

P. A. Price, E. Berger, D. E. Reichart +29

Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z=0.36. More importantly, the multi-color excess in the afterglow detected in the Hubble Space Telescope (…

astro-ph2002★ 182 cited

Detection of a supernova signature associated with GRB 011121

J. S. Bloom, S. R. Kulkarni, P. A. Price +20

Using observations from an extensive monitoring campaign with the Hubble Space Telescope we present the detection of an intermediate-time flux excess which is redder in color relat…

astro-ph2002★ 21 cited

Evidence for a Fast Decline in the Progenitor Population of Gamma Ray Bursts and the Nature of their Origin

B. E. Stern, J-L. Atteia, K. Hurley

We show that the source population of long gamma-ray bursts (GRBs) has declined by at least a factor of 12 (at the 90% confidence level) since the early stages of the Universe ($z…