117 citations · 499 across the 9 of their papers we have counts for
9 papers
GRB 090926A and Bright Late-time Fermi LAT GRB Afterglows
C. A. Swenson, A. Maxham, P. W. A. Roming +10
GRB 090926A was detected by both the GBM and LAT instruments on-board the Fermi Gamma-Ray Space Telescope. Swift follow-up observations began ~13 hours after the initial trigger. T…
Correlations of Prompt and Afterglow Emission in Swift Long and Short Gamma Ray Bursts
N. Gehrels, S. D. Barthelmy, D. N. Burrows +12
Correlation studies of prompt and afterglow emissions from gamma-ray bursts (GRBs) between different spectral bands has been difficult to do in the past because few bursts had comp…
An annular gap acceleration model for -ray emission of pulsars
G. J. Qiao, K. J. Lee, B. Zhang +2
If the binding energy of the pulsar's surface is not so high (the case of a neutron star), both the negative and positive charges will flow out freely from the surface of the star.…
GRB 061121: Broadband spectral evolution through the prompt and afterglow phases of a bright burst
K. L. Page, R. Willingale, J. P. Osborne +33
Swift triggered on a precursor to the main burst of GRB 061121 (z=1.314), allowing observations to be made from the optical to gamma-ray bands. Many other telescopes, including Kon…
Early afterglow detection in the Swift observations of GRB 050801
Massimiliano De Pasquale, S. R. Oates, M. J. Page +8
We present results of Swift optical, UV and X-ray observations of the afterglow of GRB 050801. The source is visible over the full optical, UV and X-ray energy range of the Swift U…
Swift detection of all previously undetected blazars in a micro-wave flux-limited sample of WMAP foreground sources
P. Giommi, M. Capalbi, E. Cavazzuti +19
Almost the totality of the bright foreground sources in the WMAP CMB maps are blazars, a class of sources that show usually also X-ray emission. However, 23 objects in a flux-limit…