activity
19982010
most citedDetailed Radio View on Two Stellar Explosions and Their Host Galaxy: XRF080109/SN2008D and SN2007uy in NGC2770

24 citations · 24 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2010★ 24 cited

Detailed Radio View on Two Stellar Explosions and Their Host Galaxy: XRF080109/SN2008D and SN2007uy in NGC2770

A. J. van der Horst, A. P. Kamble, Z. Paragi +16

The galaxy NGC2770 hosted two core-collapse supernova explosions, SN2008D and SN2007uy, within 10 days of each other and 9 years after the first supernova of the same type, SN1999e…

astro-ph2002

The Broadband Afterglow of GRB980329

S. A. Yost, D. A. Frail, F. A. Harrison +15

We present radio observations of the afterglow of the bright gamma-ray burst GRB980329 made between one month and several years after the burst, a re-analysis of previously publish…

astro-ph2001

Phase Calibration Sources in the Northern Sky at Galactic Latitudes $\mid b \mid < 2.5\arcdeg$

J. M. Wrobel, G. B. Taylor, P. C. Gregory

The Jodrell Bank - VLA Astrometric Survey (JVAS) of flat-spectrum sources yielded a catalog of 2118 compact radio sources in the northern sky. Those sources are being used as phase…

astro-ph2001

VLBA Polarimetry of Three Powerful Radio Galaxy Cores

G. B. Taylor, D. H. Hough, T. Venturi

We present sensitive, high dynamic range, Very Long Baseline Array (VLBA) polarimetric observations of the cores of three powerful radio galaxies: 3C166, 3C236 and 3C390.3. Signifi…

astro-ph2001

GRB 000418: A Hidden Jet Revealed?

E. Berger, A. Diercks, D. A. Frail +14

We report on optical, near-infrared and centimeter radio observations of GRB000418 which allow us to follow the evolution of the afterglow from 2 to 200 days after the gamma-ray bu…

astro-ph2000

The Rapidly Fading Afterglow from the Gamma-Ray Burst of 1999 May 6

G. B. Taylor, J. S. Bloom, D. A. Frail +3

We report on the discovery of the radio afterglow from the gamma-ray burst (GRB) of 1999 May 6 (GRB 990506) using the Very Large Array (VLA). The radio afterglow was detected at ea…