activity
20032010
most citedDiscovery and identification of the very high redshift afterglow of GRB 050904

119 citations · 290 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2010

New results with Swift on Supergiant Fast X-ray Transients

L. Sidoli, P. Romano, L. Ducci +11

We report here on the most recent results obtained on a new class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients. Since October 2007, we have been performing a m…

astro-ph2006★ 27 cited

Discovery of a Candidate Central Compact Object in the Galactic Nonthermal SNR G330.2+1.0

Sangwook Park, Koji Mori, Oleg Kargaltsev +5

We report on the discovery of a pointlike source (CXOU J160103.1513353) at the center of a Galactic supernova remnant (SNR) G330.2+1.0 with {\it Chandra X-Ray Observatory}. The…

astro-ph2005★ 119 cited

Discovery and identification of the very high redshift afterglow of GRB 050904

J. Haislip, M. Nysewander, D. Reichart +39

In 2000, Lamb and Reichart predicted that gamma-ray bursts (GRBs) and their afterglows occur in sufficient numbers and at sufficient brightnesses at very high redshifts (z > 5) to…

astro-ph2005★ 30 cited

Swift-UVOT detection of GRB 050318

M. Still, P. W. A. Roming, K. O. Mason +27

We present observations of GRB 050318 by the Ultra-Violet and Optical Telescope (UVOT) on-board the Swift observatory. The data are the first detections of a Gamma Ray Burst (GRB)…

astro-ph2005★ 73 cited

Detection of a huge explosion in the early Universe

G. Cusumano, V. Mangano, G. Chincarini +29

Gamma-ray Bursts (GRBs) are bright flashes of high energy photons that can last from about 10 milliseconds to 10 minutes. Their origin and nature have puzzled the scientific commun…

astro-ph2003★ 41 cited

0103-72.6: A New Oxygen-Rich Supernova Remnant in the Small Magellanic Cloud

Sangwook Park, John P. Hughes, David N. Burrows +3

010372.6, the second brightest X-ray supernova remnant (SNR) in the Small Magellanic Cloud (SMC), has been observed with the {\it Chandra X-Ray Observatory}. Our {\it Chandra} o…