The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

Mallory S.E. Roberts, C. Brogan, S. Ransom, M. Lyutikov, E. De Oña Wilhelmi, A. Djannati-Ataï, R. Terrier, S. M. Dougherty, E. D. Grundstrom, J. W.T. Hessels, S. Johnston, M. V. McSwain, P. S. Ray, K. S. Wood, G. G. Pooley, A. Weinstein

Research output: Contribution to journalConference articlepeer-review


Multi-wavelength studies at radio, infrared, optical, X-ray, and TeV wavelengths have discovered probable counterparts to many Galactic sources of GeV emission detected by EGRET. These include pulsar wind nebulae, high mass X-ray binaries, and mixed morphology supernova remnants. Here we provide an overview of the observational properties of Galactic sources which emit across 19 orders of magnitude in energy. We also present new observations of several sources.

Original languageEnglish (US)
Pages (from-to)328-331
Number of pages4
JournalAIP Conference Proceedings
StatePublished - 2009
Event4th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg, Germany
Duration: Jul 7 2008Jul 11 2008


  • ATCA
  • Binary
  • Gamma-ray
  • HESS
  • LS 5039
  • MGRO J1908+06
  • PSR J2021+3651
  • Pulsar
  • Pulsar wind nebula
  • RCW 49
  • Supernova remnant
  • VLA
  • XMM-Newton

ASJC Scopus subject areas

  • General Physics and Astronomy


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