A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization
Very high-energy (VHE; E > 100 GeV) γ-rays have been detected in a wide range of astronomical objects, such as pulsar wind nebulae (PWNe), supernova remnants (SNRs), giant molecular clouds, γ-ray binaries, the Galactic center, active galactic nuclei (AGN), radio galaxies, starburst galaxies, and...
| Main Authors: | , , , |
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| Format: | Journal Article |
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EDP Sciences
2010
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| Online Access: | http://hdl.handle.net/20.500.11937/25936 |
| _version_ | 1848751844247994368 |
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| author | Tam, P. Wagner, S. Tibolla, Omar Chaves, R. |
| author_facet | Tam, P. Wagner, S. Tibolla, Omar Chaves, R. |
| author_sort | Tam, P. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Very high-energy (VHE; E > 100 GeV) γ-rays have been detected in a wide range of astronomical objects, such as pulsar wind nebulae (PWNe), supernova remnants (SNRs), giant molecular clouds, γ-ray binaries, the Galactic center, active galactic nuclei (AGN), radio galaxies, starburst galaxies, and possibly star-forming regions. At lower energies, observations using the Large Area Telescope (LAT) onboard Fermi provide a rich set of data that can be used to study the behavior of cosmic accelerators in the MeV to TeV energy bands. In particular, the improved angular resolution of current telescopes in both bands compared to previous instruments significantly reduces source confusion and facilitates identification of associated counterparts at lower energies. In this paper, a comprehensive search for VHE γ-ray sources that are spatially coincident with Galactic Fermi/LAT bright sources is performed, and the available MeV to TeV spectra of coincident sources compared. It is found that bright LAT GeV sources are correlated with TeV sources, in contrast to previous studies using EGRET data. Moreover, a single spectral component seems unable to describe the MeV to TeV spectra of many coincident GeV/TeV sources. It has been suggested that γ-ray pulsars may be accompanied by VHE γ-ray emitting nebulae, a hypothesis that can be tested with VHE observations of these pulsars. |
| first_indexed | 2025-11-14T07:59:11Z |
| format | Journal Article |
| id | curtin-20.500.11937-25936 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T07:59:11Z |
| publishDate | 2010 |
| publisher | EDP Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-259362017-09-13T15:24:21Z A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization Tam, P. Wagner, S. Tibolla, Omar Chaves, R. Very high-energy (VHE; E > 100 GeV) γ-rays have been detected in a wide range of astronomical objects, such as pulsar wind nebulae (PWNe), supernova remnants (SNRs), giant molecular clouds, γ-ray binaries, the Galactic center, active galactic nuclei (AGN), radio galaxies, starburst galaxies, and possibly star-forming regions. At lower energies, observations using the Large Area Telescope (LAT) onboard Fermi provide a rich set of data that can be used to study the behavior of cosmic accelerators in the MeV to TeV energy bands. In particular, the improved angular resolution of current telescopes in both bands compared to previous instruments significantly reduces source confusion and facilitates identification of associated counterparts at lower energies. In this paper, a comprehensive search for VHE γ-ray sources that are spatially coincident with Galactic Fermi/LAT bright sources is performed, and the available MeV to TeV spectra of coincident sources compared. It is found that bright LAT GeV sources are correlated with TeV sources, in contrast to previous studies using EGRET data. Moreover, a single spectral component seems unable to describe the MeV to TeV spectra of many coincident GeV/TeV sources. It has been suggested that γ-ray pulsars may be accompanied by VHE γ-ray emitting nebulae, a hypothesis that can be tested with VHE observations of these pulsars. 2010 Journal Article http://hdl.handle.net/20.500.11937/25936 10.1051/0004-6361/200913717 EDP Sciences unknown |
| spellingShingle | Tam, P. Wagner, S. Tibolla, Omar Chaves, R. A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title | A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title_full | A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title_fullStr | A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title_full_unstemmed | A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title_short | A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization |
| title_sort | search for vhe counterparts of galactic fermi bright sources and mev to tev spectral characterization |
| url | http://hdl.handle.net/20.500.11937/25936 |