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THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
Abdo, A. A.1,2; Ackermann, M.3,4; Ajello, M.3,4; Atwood, W. B.5,6; Axelsson, M.7,8; Baldini, L.9; Ballet, J.10; Barbiellini, G.11,12; Baring, M. G.13; Bastieri, D.14,15; Baughman, B. M.16; Bechtol, K.3,4; Bellazzini, R.9; Berenji, B.3,4; Blandford, R. D.3,4; Bloom, E. D.3,4; Bonamente, E.17,18; Borgland, A. W.3,4; Bregeon, J.9; Brez, A.9; Brigida, M.19,20,21; Bruel, P.22; Burnett, T. H.23; Buson, S.15; Caliandro, G. A.19,20,21; Cameron, R. A.3,4; Camilo, F.24; Caraveo, P. A.25; Casandjian, J. M.10; Cecchi, C.17,18; Celik, Oe26,27; Charles, E.19,20,21; Chekhtman, A.1,28; Cheung, C. C.; Chiang, J.3,4; Ciprini, S.17,18; Claus, R.3,4; Cognard, I.29,30; Cohen-Tanugi, J.31; Cominsky, L. R.32; Conrad, J.8,33; Corbet, R.27; Cutini, S.34; den Hartog, P. R.3,4; Dermer, C. D.1; de Angelis, A.35,36; de Luca, A.25,37; de Palma, F.19,20,21; Digel, S. W.3,4; Dormody, M.5,6; do Couto e Silva, E.3,4; Drell, P. S.3,4; Dubois, R.3,4; Dumora, D.38,39; Espinoza, C.40; Farnier, C.31; Favuzzi, C.19,20,21; Fegan, S. J.22; Ferrara, E. C.; Focke, W. B.3,4; Fortin, P.22; Frailis, M.35,36; Freire, P. C. C.41; Fukazawa, Y.42; Funk, S.3,4; Fusco, P.19,20,21; Gargano, F.21; Gasparrini, D.34; Gehrels, N.43; Germani, S.17,18; Giavitto, G.44; Giebels, B.22; Giglietto, N.19,20,21; Giommi, P.34; Giordano, F.19,20,21; Glanzman, T.3,4; Godfrey, G.3,4; Gotthelf, E. V.24; Grenier, I. A.10; Grondin, M. -H.38,39; Grove, J. E.1; Guillemot, L.38,39; Guiriec, S.45; Gwon, C.1; Hanabata, Y.42; Harding, A. K.; Hayashida, M.3,4; Hays, E.; Hughes, R. E.16; Jackson, M. S.8,33,46; Johannesson, G.3,4; Johnson, A. S.3,4; Johnson, R. P.5,6; Johnson, T. J.43; Johnson, W. N.1; Johnston, S.47; Kamae, T.3,4; Kanbach, G.48; Kaspi, V. M.49; Katagiri, H.42; Kataoka, J.50,51; Kawai, N.50,52; Kerr, M.23; Knoedlseder, J.53; Kocian, M. L.3,4; Kramer, M.40,54; Kuss, M.9; Lande, J.3,4; Latronico, L.9; Lemoine-Goumard, M.38,39; Livingstone, M.49; Longo, F.11,12; Loparco, F.19,20,21; Lott, B.38,39; Lovellette, M. N.1; Lubrano, P.17,18; Lyne, A. G.40; Madejski, G. M.3,4; Makeev, A.1,28; Manchester, R. N.47; Marelli, M.25; Mazziotta, M. N.21; McConville, W.43; McEnery, J. E.; McGlynn, S.8,46; Meurer, C.8,33; Michelson, P. F.3,4; Mineo, T.55; Mitthumsiri, W.3,4; Mizuno, T.42; Moiseev, A. A.26,43; Monte, C.19,20,21; Monzani, M. E.3,4; Morselli, A.56; Moskalenko, I. V.3,4; Murgia, S.3,4; Nakamori, T.50; Nolan, P. L.3,4; Norris, J. P.57; Noutsos, A.40; Nuss, E.31; Ohsugi, T.42; Omodei, N.9; Orlando, E.48; Ormes, J. F.57; Ozaki, M.58; Paneque, D.3,4; Panetta, J. H.3,4; Parent, D.38,39; Pelassa, V.31; Pepe, M.17,18; Pesce-Rollins, M.9; Piron, F.31; Porter, T. A.5,6; Raino, S.19,20,21; Rando, R.14,15; Ransom, S. M.59; Ray, P. S.1; Razzano, M.9; Rea, N.60,61; Reimer, A.3,4,62,63; Reimer, O.3,4,62,63; Reposeur, T.38,39; Ritz, S.5,6; Rodriguez, A. Y.60; Romani, R. W.3,4; Roth, M.23; Ryde, F.8,46; Sadrozinski, H. F. -W.5,6; Sanchez, D.22; Sander, A.16; Parkinson, P. M. Saz5,6; Scargle, J. D.64; Schalk, T. L.5,6; Sellerholm, A.8,33; Sgro, C.9; Siskind, E. J.65; Smith, D. A.38,39; Smith, P. D.16; Spandre, G.9; Spinelli, P.19,20,21; Stappers, B. W.40; Starck, J. -L.10; Striani, E.56,66; Strickman, M. S.1; Strong, A. W.48; Suson, D. J.67; Tajima, H.3,4; Takahashi, H.42; Takahashi, T.58; Tanaka, T.3,4; Thayer, J. B.3,4; Thayer, J. G.3,4; Theureau, G.29,30; Thompson, D. J.; Thorsett, S. E.5,6; Tibaldo, L.10,14,15; Tibolla, O.68; Torres, D. F.60,69; Tosti, G.17,18; Tramacere, A.3,4; Uchiyama, Y.3,4,58; Usher, T. L.3,4; Van Etten, A.3,4; Vasileiou, V.26,27; Venter, C.71; Vilchez, N.53; Vitale, V.56,66; Waite, A. P.3,4; Wang, P.3,4; Wang, N.72; Watters, K.3,4; Weltevrede, P.47; Winer, B. L.16; Wood, K. S.1; Ylinen, T.8,46,73; Ziegler, M.5,6
2010-04-01
Source PublicationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume187Issue:2Pages:460-494
Contribution Rank67
AbstractThe dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a sizable population of these high-energy objects. This catalog summarizes 46 high-confidence pulsed detections using the first six months of data taken by the Large Area Telescope (LAT), Fermi's main instrument. Sixteen previously unknown pulsars were discovered by searching for pulsed signals at the positions of bright gamma-ray sources seen with the LAT, or at the positions of objects suspected to be neutron stars based on observations at other wavelengths. The dimmest observed flux among these gamma-ray-selected pulsars is 6.0 x 10(-8) ph cm(-2) s(-1) (for E > 100 MeV). Pulsed gamma-ray emission was discovered from 24 known pulsars by using ephemerides (timing solutions) derived from monitoring radio pulsars. Eight of these new gamma-ray pulsars are millisecond pulsars. The dimmest observed flux among the radio-selected pulsars is 1.4 x 10(-8) ph cm(-2) s(-1) (for E > 100 MeV). The remaining six gamma-ray pulsars were known since the Compton Gamma Ray Observatory mission, or before. The limiting flux for pulse detection is non-uniform over the sky owing to different background levels, especially near the Galactic plane. The pulsed energy spectra can be described by a power law with an exponential cutoff, with cutoff energies in the range similar to 1-5 GeV. The rotational energy-loss rate ((E) over dot) of these neutron stars spans five decades, from similar to 3 x 10(33) erg s(-1) to 5 x 10(38) erg s(-1), and the apparent efficiencies for conversion to gammaray emission range from similar to 0.1% to similar to unity, although distance uncertainties complicate efficiency estimates. The pulse shapes show substantial diversity, but roughly 75% of the gamma-ray pulse profiles have two peaks, separated by greater than or similar to 0.2 of rotational phase. For most of the pulsars, gamma-ray emission appears to come mainly from the outer magnetosphere, while polar-cap emission remains plausible for a remaining few. Spatial associations imply that many of these pulsars power pulsar wind nebulae. Finally, these discoveries suggest that gamma-ray-selected young pulsars are born at a rate comparable to that of their radio-selected cousins and that the birthrate of all young gamma-ray-detected pulsars is a substantial fraction of the expected Galactic supernova rate.
KeywordCatalogs Gamma Rays: General Pulsars: General Stars: Neutron
SubtypeArticle
Subject Area致密天体、高能和基础物理
DOI10.1088/0067-0049/187/2/460
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordSUPERNOVA REMNANT G292.0+1.8 ; EGRET ERROR BOXES ; TIME-DIFFERENCING TECHNIQUE ; ROTATING NEUTRON STARS ; SOURCE 3EG J2227+6122 ; GREEN-BANK-TELESCOPE ; HIGH-ENERGY EMISSION ; X-RAY ; MILLISECOND PULSARS ; RADIO PULSARS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000276841500007
Citation statistics
Cited Times:356[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/189
Collection射电天文研究室_脉冲星研究团组
其它
Affiliation1.USN, Res Lab, Div Space Sci, Washington, DC 20375 USA
2.Natl Acad Sci, Natl Res Council Res Associate, Washington, DC 20001 USA
3.Stanford Univ, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Dept Phys, Stanford, CA 94305 USA
4.Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA
5.Univ Calif Santa Cruz, Dept Phys, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
6.Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
7.Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
8.Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden
9.Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
10.Univ Paris Diderot, Lab AIM, CEA IRFU, CEA Saclay,CNRS,Serv Astrophys, F-91191 Gif Sur Yvette, France
11.Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
12.Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy
13.Rice Univ, Dept Phys & Astron, Houston, TX 77251 USA
14.Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
15.Univ Padua, Dipartimento Fis G Galilei, I-35131 Padua, Italy
16.Ohio State Univ, Dept Phys, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
17.Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
18.Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy
19.Univ Bari, Dipartimento Fis M Merlin, I-70126 Bari, Italy
20.Politecn Bari, I-70126 Bari, Italy
21.Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
22.Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France
23.Univ Washington, Dept Phys, Seattle, WA 98195 USA
24.Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
25.Ist Astrofis Spaziale & Fis Cosm, INAF, I-20133 Milan, Italy
26.NASA, Goddard Space Flight Ctr, CRESST, Greenbelt, MD 20771 USA
27.Univ Maryland Baltimore Cty, Baltimore, MD 21250 USA
28.George Mason Univ, Fairfax, VA 22030 USA
29.CNRS, LPCE, UMR 6115, F-45071 Orleans 02, France
30.INSU, CNRS, Observ Paris, Stn Radioastron Nancay, F-18330 Nancay, France
31.Univ Montpellier 2, CNRS, IN2P3, Lab Phys Theor & Astroparticules, Montpellier, France
32.Sonoma State Univ, Dept Phys & Astron, Rohnert Pk, CA 94928 USA
33.Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden
34.Agenzia Spaziale Italiana Sci Data Ctr, I-00044 Frascati, Roma, Italy
35.Univ Udine, Dipartimento Fis, I-33100 Udine, Italy
36.Ist Nazl Fis Nucl, Sez Trieste, Grp Coll Udine, I-33100 Udine, Italy
37.IUSS, I-27100 Pavia, Italy
38.Univ Bordeaux, CEN Bordeaux Gradignan, UMR 5797, F-33175 Gradignan, France
39.CEN Bordeaux Gradignan, CNRS, IN2P3, UMR 5797, F-33175 Gradignan, France
40.Univ Manchester, Sch Phys & Astron, Ctr Astrophys, Jodrell Bank, Manchester M13 9PL, Lancs, England
41.Arecibo Observ, Arecibo, PR 00612 USA
42.Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan
43.Univ Maryland, College Pk, MD 20742 USA
44.Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
45.Univ Alabama, Huntsville, AL 35899 USA
46.Royal Inst Technol KTH, Dept Phys, SE-10691 Stockholm, Sweden
47.CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
48.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
49.McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
50.Tokyo Inst Technol, Dept Phys, Meguro, Tokyo 1528551, Japan
51.Waseda Univ, Shinjuku Ku, Tokyo 1698050, Japan
52.RIKEN, Inst Phys & Chem Res, Cosm Radiat Lab, Wako, Saitama 3510198, Japan
53.UPS, CNRS, Ctr Etud Spatiale Rayonnements, F-30128 Toulouse 4, France
54.Max Planck Inst Radioastron, D-53121 Bonn, Germany
55.IASF Palermo, I-90146 Palermo, Italy
56.Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy
57.Univ Denver, Dept Phys & Astron, Denver, CO 80208 USA
58.JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
59.Natl Radio Astron Observ, Charlottesville, VA 22903 USA
60.CSIC, IEEC, Inst Ciencies Espai, Barcelona 08193, Spain
61.Sterrenkundig Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
62.Leopold Franzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria
63.Leopold Franzens Univ Innsbruck, Inst Theoret Phys, A-6020 Innsbruck, Austria
64.NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
65.NYCB Real Time Comp Inc, Lattingtown, NY 11560 USA
66.Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy
67.Purdue Univ Calumet, Dept Chem & Phys, Hammond, IN 46323 USA
68.Max Planck Inst Kernphys, D-69029 Heidelberg, Germany
69.Inst Catalana Recerca & Estudis Avancats, Barcelona, Spain
70.CIFS, I-10133 Turin, Italy
71.North West Univ, ZA-2520 Potchefstroom, South Africa
72.CAS, Natl Astron Observ, Urumqi 830011, Peoples R China
73.Univ Kalmar, Sch Pure & Appl Nat Sci, SE-39182 Kalmar, Sweden
Recommended Citation
GB/T 7714
Abdo, A. A.,Ackermann, M.,Ajello, M.,et al. THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2010,187(2):460-494.
APA Abdo, A. A..,Ackermann, M..,Ajello, M..,Atwood, W. B..,Axelsson, M..,...&Ziegler, M..(2010).THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,187(2),460-494.
MLA Abdo, A. A.,et al."THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 187.2(2010):460-494.
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