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An Optical Counterpart to the Anomalous X-ray Pulsar 4U 0142+61
F. Hulleman, M. H. van Kerkwijk, S. R. Kulkarni
The energy source of the anomalous X-ray pulsars is not well understood, hence their designation as anomalous. Unlike binary X-ray pulsars, no companions are seen, so the energy ca…
Sensitivity of the Radial Velocity Technique in Detecting Outer Planets
J. A. Eisner, S. R. Kulkarni
The technique of radial velocity (RV) has produced spectacular discoveries of short-period Jovian mass objects around a fraction (5 to 10%) of nearby G stars. Although we expect Jo…
The Redshift and the Host Galaxy of GRB 980613: A Gamma-Ray Burst From a Merger-Induced Starburst?
S. G. Djorgovski, J. S. Bloom, S. R. Kulkarni
We present optical and near-IR identification and spectroscopy of the host galaxy of GRB 980613. The burst was apparently associated with the optically (restframe UV) brightest com…
The redshift and the ordinary host galaxy of GRB 970228
J. S. Bloom, S. G. Djorgovski, S. R. Kulkarni
The gamma-ray burst of 28 February 1997 (GRB 970228) ushered in the discovery of the afterglow phenomenon. Despite intense study of the host galaxy, however, the nature of the host…
The Bright Gamma-Ray Burst 991208 - Tight Constraints on Afterglow Models from Observations of the Early-Time Radio Evolution
T. J. Galama, M. Bremer, F. Bertoldi +13
The millimeter wavelength emission from GRB 991208 is the second brightest ever detected, yielding a unique data set. We present here well-sampled spectra and light curves over mor…
A Jet Model for the Afterglow Emission from GRB000301C
E. Berger, R. Sari, D. A. Frail +11
We present broad-band radio observations of the afterglow of GRB000301C, spanning from 1.4 to 350 GHz for the period of 3 to 83 days after the burst. This radio data, in addition t…