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D. Lamb

23 papers hereh-index 111.1k citations23 works total

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

author position
  • first author2
  • middle author9
  • last author6

Across the 17 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph22
  • astro-ph.HE1
same name
  • D. Lamb — 143 papers, h 66
  • D. Lamb — 21 papers, h 18
  • D. Lamb — 12 papers, h 4
  • D. Lamb — 6 papers, h 2
  • D. Lamb — 5 papers, h 50
  • D. Lamb — 5 papers, h 5

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
20002010
most citedA Possible Cepheid-Like Luminosity Estimator for the Long Gamma-Ray Bursts

260 citations · 944 across the 19 of their papers we have counts for

collaborators
Showing 2003Show all

3 papers · 1 filter

astro-ph2003★ 137 cited

A Unified Jet Model of X-Ray Flashes, X-Ray-Rich Gamma-Ray Bursts, and Gamma-Ray Bursts: I. Power-Law-Shaped Universal and Top-Hat-Shaped Variable Opening-Angle Jet Models

D. Q. Lamb, T. Q. Donaghy, C. Graziani

HETE-2 has provided strong evidence that the properties of X-Ray Flashes (XRFs), X-ray-rich GRBs, and GRBs form a continuum, and therefore that these three kinds of bursts are the…

astro-ph2003★ 30 cited

Design and Performance of the Wide-Field X-Ray Monitor on Board the High-Energy Transient Explorer 2

Y. Shirasaki, N. Kawai, A. Yoshida +18

The Wide-field X-ray Monitor (WXM) is one of the scientific instruments carried on the High Energy Transient Explorer 2 (HETE-2) satellite launched on 2000 October 9. HETE-2 is an…

astro-ph2003★ 56 cited

The X-ray Afterglows of GRB 020813 and GRB 021004 with Chandra HETGS: Possible Evidence for a Supernova Prior to GRB 020813

Nathaniel R. Butler, Herman L. Marshall, George R. Ricker +5

We report on the detection of an emission line near 1.3 keV, which we associate with blue-shifted hydrogen-like sulfur (S XVI), in a 76.8 ksec Chandra HETGS spectrum of the aftergl…

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