output
19932026
most citedDiscovery of a Cool Planet of 5.5 Earth Masses Through Gravitational Microlensing

596 citations

Showing 2002 · astro-phShow all

7 papers · 2 filters

astro-ph2002★ 253 cited

A New Look at the Large-Scale HI Structure of the LMC

L. Staveley-Smith, S. Kim, M. R. Calabretta +2

We present a Parkes multibeam \HI survey of the Large Magellanic Cloud (LMC). This survey, which is sensitive to spatial structure in the range 200 pc to 10 kpc, complements the Au…

astro-ph2002★ 49 cited

A sample of southern Compact Steep Spectrum radio sources: The VLBI observations

A. Tzioumis, E. King, R. Morganti +19

A small sample of 7 southern Compact Steep Spectrum (CSS) radio sources has been selected as part of the study of a larger flux-limited complete sample of radio sources. High resol…

astro-ph2002★ 62 cited

Magnetic fields in barred galaxies I. The atlas

R. Beck, V. Shoutenkov, M. Ehle +5

The total and polarized radio continuum emission of 20 barred galaxies was observed with the Very Large Array (VLA) at 3, 6, 18 and 22 cm and with the Australia Telescope Compact A…

astro-ph2002★ 66 cited

The Multi-Component Nature of the Vela Pulsar Nonthermal X-ray Spectrum

Alice K. Harding, Mark S. Strickman, Carl Gwinn +2

We report on our analysis of a 274 ks observation of the Vela pulsar with the Rossi X-Ray Timing Explorer (RXTE). The double-peaked, pulsed emission at 2 - 30 keV, which we had pre…

astro-ph2002★ 32 cited

A Short, Non-Planetary, Microlensing Anomaly: Observations and Lightcurve Analysis of MACHO 99-BLG-47

M. D. Albrow, J. An, J. -P. Beaulieu +17

We analyze PLANET and MACHO observations of MACHO 99-BLG-47, the first nearly-normal microlensing event for which high signal-to-noise-ratio data reveal a well-covered, short-durat…

astro-ph2002★ 161 cited

High time resolution observations of the January 2000 glitch in the Vela pulsar

R. G. Dodson, P. M. McCulloch, D. R. Lewis

Pulsars are rotating neutron stars, sweeping the emission regions from the magnetic poles across our line of sight. Isolated neutron stars lose angular momentum through dipole radi…