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19942026
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 10.8k across the 113 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 95 cited

The Radio and X-ray Luminous Type Ibc Supernova 2003L

A. M. Soderberg, S. R. Kulkarni, E. Berger +4

We present extensive radio observations of SN 2003L, the most luminous and energetic Type Ibc radio supernova with the exception of SN 1998bw (associated with GRB 980425). Observat…

astro-ph2004★ 206 cited

The sub-energetic GRB 031203 as a cosmic analogue to GRB 980425

A. M. Soderberg, S. R. Kulkarni, E. Berger +13

Over the six years since the discovery of the gamma-ray burst GRB 980425, associated with the nearby (distance, ~40 Mpc) supernova 1998bw, astronomers have fiercely debated the nat…

astro-ph2004★ 89 cited

Accurate Calorimetry of GRB 030329

D. A. Frail, A. M. Soderberg, S. R. Kulkarni +4

We report late-time observations of the radio afterglow of GRB 030329. The light curves show a clear achromatic flattening at 50 days after the explosion. We interpret this flatten…

astro-ph2004★ 112 cited

Dynamical Masses of the Binary Brown Dwarf GJ 569Bab

M. R. Zapatero Osorio, B. L. Lane, Ya. Pavlenko +3

We have obtained new images and high-resolution (R ~ 22400) near-infrared (1.2400-1.2575 micron) spectra of each component of the brown dwarf binary GJ 569Bab using the Adaptive Op…

astro-ph2004★ 58 cited

The Non-Relativistic Evolution of GRBs 980703 and 970508: Beaming-Independent Calorimetry

E. Berger, S. R. Kulkarni, D. A. Frail

We use the Sedov-Taylor self-similar solution to model the radio emission from the gamma-ray bursts (GRBs) 980703 and 970508, when the blastwave has decelerated to non-relativistic…

astro-ph2004★ 79 cited

An X-ray Search for Compact Central Sources in Supernova Remnants I: SNRs G093.3+6.9, G315.4-2.3, G084.2+0.8, & G127.1+0.5

D. L. Kaplan, D. A. Frail, B. M. Gaensler +4

Less than half of the SNRs within 5 kpc have identified central sources, and only three are identified as the remnants of Type Ia SNe. Here, we report a systematic effort to search…