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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 1998Show all

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astro-ph1998★ 88 cited

The Discovery and Broad-band Follow-up of the Transient Afterglow of GRB 980703

J. S. Bloom, D. A. Frail, S. R. Kulkarni +14

We report on the discovery of the radio, infrared and optical transient coincident with an X-ray transient proposed to be the afterglow of GRB 980703. At later times when the trans…

astro-ph1998★ 194 cited

Spectroscopy of the Host Galaxy of the Gamma--Ray Burst 980703

S. G. Djorgovski, S. R. Kulkarni, J. S. Bloom +4

We present spectroscopic observations of the host galaxy of the gamma-ray burst (GRB) 980703. Several emission and absorption features are detected, making the redshift, z = 0.966,…

astro-ph1998★ 187 cited

The Host Galaxy of GRB 970508

J. S. Bloom, S. G. Djorgovski, S. R. Kulkarni +1

We present late-time imaging and spectroscopic observations of the optical transient (OT) of gamma-ray burst (GRB) 970508. Imaging observations roughly 200 and 300 days after the b…

astro-ph1998★ 84 cited

The Discovery of the Radio Afterglow From the Optically Dim Gamma-Ray Burst of March 29, 1998

G. B. Taylor, D. A. Frail, S. R. Kulkarni +3

We report on the discovery of a variable radio source, VLA J070238.0+385044, associated with the proposed x-ray counterpart, 1SAX J0702.6+3850 of GRB 980329. The source was monitor…

astro-ph1998★ 7 cited

No Radio Afterglow from the Gamma-Ray Burst of February 28, 1997

D. A. Frail, S. R. Kulkarni, D. S. Shepherd +1

We present radio observations of the gamma-ray burster GRB 970228 made with the Very Large Array (VLA) and the Owens Valley Radio Observatory (OVRO) spanning a range of postburst t…

astro-ph1998★ 68 cited

Optical Observations of the Isolated Neutron Star RX J0720.4-3125

S. R. Kulkarni, M. H. van Kerkwijk

RX J0720.4-3125 is an unidentified bright soft X-ray source which shows pulsations at a 8.39 s period and has a thermal spectrum. We present deep B and R band images of its X-ray l…