High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope
Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its~1 us absolute time tagging capability coupled with a good sensitivity in the 30MeV-30 GeV range, with simultaneous X-ray monitoring in the18-60 keV band, makes it perfectly suited for the study of gamma-ray pulsa...
| Main Authors: | , , , , , |
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| Format: | Journal Article |
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The American Astronomical Society
2009
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| Subjects: | |
| Online Access: | http://hdl.handle.net/20.500.11937/10563 |
| _version_ | 1848747567191425024 |
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| author | Pellizzoni, A. Pilia, M. Possenti, A. Fornari, F. Caraveo, P. Hotan, Aidan |
| author_facet | Pellizzoni, A. Pilia, M. Possenti, A. Fornari, F. Caraveo, P. Hotan, Aidan |
| author_sort | Pellizzoni, A. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its~1 us absolute time tagging capability coupled with a good sensitivity in the 30MeV-30 GeV range, with simultaneous X-ray monitoring in the18-60 keV band, makes it perfectly suited for the study of gamma-ray pulsars following up on the Compton Gamma Ray Observatory/EGRET heritage. In this paper, we present the first AGILE timing results on the known gamma-raypulsars Vela, Crab, Geminga, and B1706-44. The data were collected from 2007 July to 2008 April, exploiting the mission Science Verification Phase, the Instrument Timing Calibration, and the early Observing Pointing Program. Thanks to its large field of view, AGILE collected a large number of gamma-ray photons from these pulsars(~ 10,000 pulsed counts for Vela) in only few months of observations. The coupling of AGILE timing capabilities, simultaneous radio/X-ray monitoring, and new tools aimed at precise photon phasing, also exploiting timing noise correction, unveiled new interesting features at the submillisecond level in the pulsars' high-energy light curves. |
| first_indexed | 2025-11-14T06:51:12Z |
| format | Journal Article |
| id | curtin-20.500.11937-10563 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T06:51:12Z |
| publishDate | 2009 |
| publisher | The American Astronomical Society |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-105632017-09-13T16:02:37Z High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope Pellizzoni, A. Pilia, M. Possenti, A. Fornari, F. Caraveo, P. Hotan, Aidan Crab gamma rays PSR B - 1706-44) stars pulsars neutron Geminga general individual (Vela observations Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its~1 us absolute time tagging capability coupled with a good sensitivity in the 30MeV-30 GeV range, with simultaneous X-ray monitoring in the18-60 keV band, makes it perfectly suited for the study of gamma-ray pulsars following up on the Compton Gamma Ray Observatory/EGRET heritage. In this paper, we present the first AGILE timing results on the known gamma-raypulsars Vela, Crab, Geminga, and B1706-44. The data were collected from 2007 July to 2008 April, exploiting the mission Science Verification Phase, the Instrument Timing Calibration, and the early Observing Pointing Program. Thanks to its large field of view, AGILE collected a large number of gamma-ray photons from these pulsars(~ 10,000 pulsed counts for Vela) in only few months of observations. The coupling of AGILE timing capabilities, simultaneous radio/X-ray monitoring, and new tools aimed at precise photon phasing, also exploiting timing noise correction, unveiled new interesting features at the submillisecond level in the pulsars' high-energy light curves. 2009 Journal Article http://hdl.handle.net/20.500.11937/10563 10.1088/0004-637X/691/2/1618 The American Astronomical Society fulltext |
| spellingShingle | Crab gamma rays PSR B - 1706-44) stars pulsars neutron Geminga general individual (Vela observations Pellizzoni, A. Pilia, M. Possenti, A. Fornari, F. Caraveo, P. Hotan, Aidan High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title | High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title_full | High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title_fullStr | High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title_full_unstemmed | High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title_short | High-resolution timing observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope |
| title_sort | high-resolution timing observations of spin-powered pulsars with the agile gamma-ray telescope |
| topic | Crab gamma rays PSR B - 1706-44) stars pulsars neutron Geminga general individual (Vela observations |
| url | http://hdl.handle.net/20.500.11937/10563 |