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D. Moffett

12 papers hereh-index 181.4k citations47 works total

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

author position
  • first author2
  • middle author5
  • last author3

Across the 10 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph8
  • astro-ph.HE3
  • astro-ph.GA1
same name
  • D. Moffett — 4 papers, h 2

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
19962017
most citedCosmic Ray Acceleration at the Forward Shock in Tycho's Supernova Remnant: Evidence from Chandra X-ray Observations

313 citations · 1.1k across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2017★ 19 cited

The fading of Cassiopeia A, and improved models for the absolute spectrum of primary radio calibration sources

A. S. Trotter, D. E. Reichart, R. E. Egger +20

Based on five years of observations with the 40-foot telescope at Green Bank Observatory (GBO), Reichart & Stephens (2000) found that the radio source Cassiopeia A had either faded…

astro-ph.HE2012★ 46 cited

A Broadband Study of the Emission from the Composite Supernova Remnant MSH 11-62

Patrick Slane, John P. Hughes, Tea Temim +10

MSH 11-62 (G291.1-0.9) is a composite supernova remnant for which radio and X-ray observations have identified the remnant shell as well as its central pulsar wind nebula. The obse…

astro-ph.HE2011★ 103 cited

Evidence For Particle Acceleration to the Knee of the Cosmic Ray Spectrum in Tycho's Supernova Remnant

Kristoffer A. Eriksen, John P. Hughes, Carles Badenes +7

Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 10^15 eV, accelerating particles to relativistic energ…

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