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K. Hurley

4 papers hereh-index 72k citations11 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • K. Hurley — 92 papers, h 50
  • K. Hurley — 88 papers, h 44
  • K. Hurley — 22 papers, h 14
  • K. Hurley — 16 papers
  • K. Hurley — 12 papers, h 12
  • K. Hurley — 11 papers, h 7

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20042007
most citedAn exceptionally bright flare from SGR1806-20 and the origins of short-duration gamma-ray bursts

598 citations · 648 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph2007

Spectral Analysis of GRBs Measured by RHESSI

C. Wigger, W. Hajdas, A. Zehnder +5

The Ge spectrometer of the RHESSI satellite is sensitive to Gamma Ray Bursts (GRBs) from about 40 keV up to 17 MeV, thus ideally complementing the Swift/BAT instrument whose sensit…

astro-ph2006★ 50 cited

The Giant Flare of December 27, 2004 from SGR 1806-20

Steven E. Boggs, A. Zoglauer, E. Bellm +5

The giant flare of December 27, 2004 from SGR 1806-20 represents one of the most extraordinary events captured in over three decades of monitoring the gamma-ray sky. One measure of…

astro-ph2005★ 598 cited

An exceptionally bright flare from SGR1806-20 and the origins of short-duration gamma-ray bursts

K. Hurley, S. E. Boggs, D. M. Smith +17

Soft-gamma-ray repeaters (SGRs) are galactic X-ray stars that emit numerous short-duration (about 0.1 s) bursts of hard X-rays during sporadic active periods. They are thought to b…

astro-ph2004

The Sample of Gamma-ray Bursts Observed With SPI-ACS

A. Rau, A. von Kienlin, K. Hurley +1

The SPI anticoincidence shield consists of 91 BGO crystals and is operated as a nearly omnidirectional gamma-ray burst detector above ~75 keV. Since the start of the mission 269 ga…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.