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Pulsar timing for the Fermi gamma-ray space telescope
Smith, D. A.1,2; Guillemot, L.1,2; Camilo, F.3; Cognard, I.4,5; Dumora, D.1,2; Espinoza, C.7; Freire, P. C. C.8; Gotthelf, E. V.3; Harding, A. K.9; Hobbs, G. B.10; Johnston, S.10; Kaspi, V. M.11; Kramer, M.7; Livingstone, M. A.11; Lyne, A. G.7; Manchester, R. N.10; Marshall, F. E.9; McLaughlin, M. A.12; Noutsos, A.7; Ransom, S. M.13; Roberts, M. S. E.14; Romani, R. W.15; Stappers, B. W.7; Theureau, G.4,5,6; Thompson, D. J.9; Thorsett, S. E.16; Wang, N.17; Weltevrede, P.10
2008-12-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume492Issue:3Pages:923-931
Contribution Rank17
AbstractWe describe a comprehensive pulsar monitoring campaign for the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope ( formerly GLAST). The detection and study of pulsars in gamma rays give insights into the populations of neutron stars and supernova rates in the Galaxy, into particle acceleration mechanisms in neutron star magnetospheres, and into the "engines" driving pulsar wind nebulae. LAT's unprecedented sensitivity between 20 MeV and 300 GeV together with its 2.4 sr field-of-view makes detection of many gamma-ray pulsars likely, justifying the monitoring of over two hundred pulsars with large spin-down powers. To search for gamma-ray pulsations from most of these pulsars requires a set of phase-connected timing solutions spanning a year or more to properly align the sparse photon arrival times. We describe the choice of pulsars and the instruments involved in the campaign. Attention is paid to verifications of the LAT pulsar software, using for example giant radio pulses from the Crab and from PSR B1937+21 recorded at Nancay, and using X-ray data on PSR J0218+4232 from XMM-Newton. We demonstrate accuracy of the pulsar phase calculations at the microsecond level.
KeywordSpace Vehicles: Instruments Stars: Pulsars: General Gamma-rays: Observations Ephemerides
SubtypeArticle
DOI10.1051/0004-6361:200810285
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordRAPIDLY SPINNING PULSARS ; GIANT RADIO PULSES ; MILLISECOND PULSARS ; HIGH-ENERGY ; BINARY PULSAR ; CRAB PULSAR ; PRECISION ; RADIATION ; MODEL ; DISCOVERY
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000261697900032
Citation statistics
Cited Times:94[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/821
Collection射电天文研究室_脉冲星研究团组
其它
Corresponding AuthorSmith, D. A.
Affiliation1.Univ Bordeaux, Ctr Etud Nucl Bordeaux Gradignan, UMR 5797, F-33175 Gradignan, France
2.Ctr Etud Nucl Bordeaux Gradignan, IN2P3, CNRS, UMR 5797, F-33175 Gradignan, France
3.Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
4.CNRS INSU, UMR 6115, LPCE, F-45071 Orleans, France
5.CNRS INSU, Observ Paris, Stn Radioastron Nancay, F-18330 Nancay, France
6.Univ Paris Diderot, CNRS, Observ Paris, GEPI, F-92190 Meudon, France
7.Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
8.Arecibo Observ, Arecibo, PR 00612 USA
9.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
10.CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
11.McGill Univ, Montreal, PQ, Canada
12.W Virginia Univ, Dept Phys, Morgantown, WV 26506 USA
13.Natl Radio Astron Observ, Charlottesville, VA 22903 USA
14.Eureka Sci Inc, Oakland, CA 94602 USA
15.Stanford Univ, Dept Phys, Stanford, CA 94305 USA
16.Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
17.Chinese Acad Sci, Natl Astron Observ, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Smith, D. A.,Guillemot, L.,Camilo, F.,et al. Pulsar timing for the Fermi gamma-ray space telescope[J]. ASTRONOMY & ASTROPHYSICS,2008,492(3):923-931.
APA Smith, D. A..,Guillemot, L..,Camilo, F..,Cognard, I..,Dumora, D..,...&Weltevrede, P..(2008).Pulsar timing for the Fermi gamma-ray space telescope.ASTRONOMY & ASTROPHYSICS,492(3),923-931.
MLA Smith, D. A.,et al."Pulsar timing for the Fermi gamma-ray space telescope".ASTRONOMY & ASTROPHYSICS 492.3(2008):923-931.
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