activity
19962020
most citedRelativistic ejecta from XRF 060218 and the rate of cosmic explosions

513 citations · 3.5k across the 40 of their papers we have counts for

collaborators
Showing 2001Show all

6 papers · 1 filter

astro-ph2001★ 215 cited

Hard X-ray states and radio emission in GRS 1915+105

M. Klein-Wolt, R. P. Fender, G. G. Pooley +4

We have compared simultaneous Ryle Telescope radio and Rossi X-Ray Timing Explorer X-ray observations of the galactic microquasar GRS 1915+105, using the classification of the X-ra…

astro-ph2001

Wide-band X-ray variability of GRS 1915+105 observed with BeppoSAX

P. Casella, M. Feroci, E. Massaro +9

The Galactic Microquasar GRS 1915+105 was observed by the Narrow Field Instruments onboard BeppoSAX in two pointings during year 2000. We present the preliminary results of wide-ba…

astro-ph2001★ 133 cited

Complete and Simultaneous Spectral Observations of the Black-Hole X-ray Nova XTE J1118+480

J. E. McClintock, C. A. Haswell, M. R. Garcia +13

The X-ray nova XTE J1118+480 suffers minimal extinction (b = 62 degrees) and therefore represents an outstanding opportunity for multiwavelength studies. Hynes et al. (2000) conduc…

astro-ph2001

Broadband Observations of the Afterglow of GRB 000926: Observing the Effect of Inverse Compton Scattering and Evidence for a High-Density Environment

F. A. Harrison, S. A. Yost, R. Sari +21

GRB 000926 has one of the best-studied afterglows to-date, with multiple X-ray observations, as well as extensive multi-frequency optical and radio coverage. Broadband afterglow ob…

astro-ph2001★ 22 cited

Mapping of the SZ effect in the cluster Cl 0016+16 with the Ryle Telescope

K. Grainge, W. F. Grainger, M. E. Jones +3

We have mapped the high-redshift (z = 0.546) cluster Cl 0016+16 with the Ryle Telescope at 15 GHz. The Sunyaev-Zel'dovich decrement is clearly detected, and resolved. We combine ou…

astro-ph2001★ 57 cited

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…