The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters
Mallory S.E. Roberts (Eureka Scientific), C. Brogan (NRAO), S. Ransom, (NRAO), M. Lyutikov (Purdue), E. de O\~na Wilhelmi (APC), A. Djannati-Ata\"i, (APC), R. Terrier (APC), S.M. Dougherty (HIA-DRAO), E.D. Grundstrom, (Vanderbilt), J.W.T. Hessels (Univ. of Amsterdam)
TL;DR
This paper reviews multi-wavelength observations of Galactic sources emitting across 19 orders of magnitude in energy, highlighting recent findings and presenting new observational data.
Contribution
It provides a comprehensive overview of the spectral properties of Galactic sources from radio to TeV energies and includes new observational results.
Findings
Identification of probable counterparts to GeV sources
Characterization of emission properties across the spectrum
New observational data on selected sources
Abstract
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.
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