Showing 2000 · astro-phShow all

102 papers · 2 filters

astro-ph2000★ 34 cited

3EG J2016+3657: Confirming an EGRET Blazar Behind the Galactic Plane

J. P. Halpern, M. Eracleous, R. Mukherjee +1

We recently identified the blazar-like radio source G74.87+1.22 (B2013+370) as the counterpart of the high-energy gamma-ray source 3EG J2016+3657 in the Galactic plane. However, si…

astro-ph2000★ 38 cited

Long-term Optical Variability of Radio-Selected Quasars from the FIRST Survey

David J. Helfand, Remington P. S. Stone, Beth Willman +5

We have obtained single-epoch optical photometry for 201 quasars, taken from the FIRST Bright Quasar Survey, which span a wide range in radio loudness. Comparison with the magnitud…

astro-ph2000★ 7 cited

Preliminary Results from the 1999 Balloon Flight of the Liquid Xenon Gamma-Ray Imaging Telescope (LXeGRIT)

E. Aprile, U. G. Oberlack, A. Curioni +8

LXeGRIT is a balloon-borne Compton telescope employing a large volume liquid xenon time projection chamber (LXeTPC) as the central gamma-ray detector. It is designed to image gamma…

astro-ph2000★ 4 cited

Performance of the Light Trigger System in the Liquid Xenon Gamma-Ray Telescope LXeGRIT

U. Oberlack, E. Aprile, A. Curioni +1

LXeGRIT is a balloon-borne Compton telescope for MeV gamma-ray astrophysics, based on a liquid xenon time projection chamber with charge and light readout. The energy and direction…

astro-ph2000★ 44 cited

The COMPTEL instrumental line background

G. Weidenspointner, M. Varendorff, U. Oberlack +8

The instrumental line background of the Compton telescope COMPTEL onboard the Compton Gamma-Ray Observatory is due to the activation and/or decay of many isotopes. The major compon…

astro-ph2000★ 6 cited

An Upgraded Data Acquisition System for the Balloon-Borne Liquid Xenon Gamma-Ray Telescope LXeGRIT

E. Aprile, A. Curioni, K. Giboni +2

LXeGRIT is a balloon-borne Compton telescope for MeV gamma-ray astrophysics, based on a liquid xenon time projection chamber (LXe-TPC) with charge and light readout. The first ball…

astro-ph2000★ 14 cited

Spectroscopy and Imaging Performance of the Liquid Xenon Gamma-Ray Imaging Telescope (LXeGRIT)

E. Aprile, A. Curioni, V. Egorov +8

LXeGRIT is a balloon-borne Compton telescope based on a liquid xenon time projection chamber (LXeTPC) for imaging cosmic \g-rays in the energy band of 0.2-20 MeV. The detector, wit…

astro-ph2000★ 26 cited

Compton scattering sequence reconstruction algorithm for the liquid xenon gamma-ray imaging telescope (LXeGRIT)

U. G. Oberlack, E. Aprile, A. Curioni +2

The Liquid Xenon Gamma-Ray Imaging Telescope (LXeGRIT) is a balloon born experiment sensitive to \g -rays in the energy band of 0.2-20 MeV. The main detector is a time projection c…

astro-ph2000★ 67 cited

A radio supernova remnant associated with the young pulsar J1119-6127

Fronefield Crawford, B. M. Gaensler, V. M. Kaspi +4

We report on Australia Telescope Compact Array observations in the direction of the young high magnetic-field pulsar J1119-6127. In the resulting images we identify a non-thermal r…

astro-ph2000★ 4 cited

DarkSUSY - A numerical package for dark matter calculations in the MSSM

Paolo Gondolo, Joakim Edsjo, Lars Bergstrom +2

The question of the nature of the dark matter in the Universe remains one of the most outstanding unsolved problems in basic science. One of the best motivated particle physics can…

astro-ph2000

The black hole mass vs bulge mass relationship in spiral galaxies

A. Marconi, D. Axon, J. Atkinson +15

We describe an on-going HST program aimed at determining the relationship between the nuclear black hole mass and bulge mass in spiral galaxies. We have selected a volume limited s…

astro-ph2000★ 84 cited

Discovery of Five Binary Radio Pulsars

F. Camilo, A. G. Lyne, R. N. Manchester +8

We report on five binary pulsars discovered in the Parkes multibeam Galactic plane survey. All of the pulsars are old, with characteristic ages 1-11 Gyr, and have relatively small…

astro-ph2000

The Nuclei of Nearby Radio-Loud Ellipticals

G. A. Verdoes Kleijn, P. T. de Zeeuw, S. A. Baum +5

We have observed a complete sample of 21 nearby (D < 70h^{-1} Mpc) Fanaroff & Riley Type I galaxies with HST/WFPC2 and detected dust disks and lanes in 19 of them. The radio jets a…

astro-ph2000★ 54 cited

PSR J1740-3052 - a pulsar with a massive companion

I. H. Stairs, R. N. Manchester, A. G. Lyne +14

We report on the discovery of a binary pulsar, PSR J1740-3052, during the Parkes multibeam survey. Timing observations of the 570-ms pulsar at Jodrell Bank and Parkes show that it…

astro-ph2000★ 3 cited

The Brown Dwarf Mass Function from Pixel Microlensing

E. A. Baltz, J. Silk

We argue that gravitational microlensing is a feasible technique for measuring the mass function of brown dwarf stars in distant galaxies. Microlensing surveys of the bulge of M31,…

astro-ph2000

Stellar Coronae with \textit{XMM-Newton} RGS. II. X-ray Variability

M. Audard, M. Guedel, A. J. den Boggende +16

First results from high-resolution coronal spectroscopy of flares with the Reflection Grating Spectrometers on board the \textit{XMM-Newton} satellite are reviewed. Rotational modu…

astro-ph2000

Stellar Coronae with \textit{XMM-Newton} RGS. I. Coronal Structure

M. Guedel, M. Audard, A. J. den Boggende +16

First results from high-resolution coronal spectroscopy with the {\it XMM-Newton} Reflection Grating Spectrometers (RGS) are reviewed. Five stellar systems (HR 1099, Capella, Procy…

astro-ph2000★ 152 cited

Constraints from the Lyman alpha forest power spectrum

Matias Zaldarriaga, Lam Hui, Max Tegmark

We use published measurements of the transmission power spectrum of the Lyman alpha forest to constrain several parameters that describe cosmology and thermal properties of the int…

astro-ph2000★ 11 cited

Detection of X-ray line emission from the shell of SNR B0540-69.3 with XMM-Newton RGS

K. J. van der Heyden, F. Paerels, J. Cottam +2

We present X-ray observations of PSR 0540-69.3 with the XMM-Newton observatory. The spectra obtained with the Reflection Grating Spectrometer reveal, for the first time, emission f…

astro-ph2000★ 9 cited

A Giant Bipolar Shell around the WO star in the Galaxy IC 1613: Structure and Kinematics

V. L. Afanasiev, T. A. Lozinskaya, A. V. Moiseev +1

Observations of the nebula associated with the WO star in the galaxy IC 1613 are presented. The observations were carried out with a scanning Interferometer Fabry-Perot in H_alpha…

astro-ph2000★ 42 cited

The Metallicity of 0.5<z<1 Field Galaxies

C. M. Carollo, S. J. Lilly

We have measured the emission line ratios in a sample of 34 CFRS star-forming galaxies with redshifts between 0.5 < z < 1.0, and computed their metallicities by means of the empiri…

astro-ph2000★ 58 cited

Radio Pulsars in the Magellanic Clouds

F. Crawford, V. M. Kaspi, R. N. Manchester +3

We report the results of a survey of the Small Magellanic Cloud (SMC) for radio pulsars conducted with the 20-cm multibeam receiver of the Parkes 64-meter telescope. This survey ta…

astro-ph2000★ 250 cited

Observation of X-ray lines from a Gamma-Ray Burst (GRB991216): Evidence of Moving Ejecta from the Progenitor

L. Piro, G. Garmire, M. Garcia +18

We report on the discovery of two emission features observed in the X-ray spectrum of the afterglow of the gamma-ray burst (GRB) of 16 Dec. 1999 by the Chandra X-Ray Observatory. T…

astro-ph2000★ 65 cited

High-resolution X-ray spectroscopy and imaging of supernova remnant N132D

Ehud Behar, Andrew P. Rasmussen, R. Gareth Griffiths +4

The observation of the supernova remnant N132D by the scientific instruments on board the XMM-Newton satellite is presented. The X-rays from N132D are dispersed into a detailed lin…