Institutional Repository of Radio Astronomy Research Laboratory
| 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
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| 2010-04-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
 |
| Volume | 187Issue:2Pages:460-494 |
| Contribution Rank | 67 |
| Abstract | The 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. |
| Keyword | Catalogs Gamma Rays: General Pulsars: General Stars: Neutron |
| Subtype | Article |
| Subject Area | 致密天体、高能和基础物理 |
| DOI | 10.1088/0067-0049/187/2/460 |
| WOS Headings | Science & Technology ; Physical Sciences |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | SUPERNOVA 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 Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000276841500007 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://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 |
| Affiliation | 1.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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| The First Fermi Larg（4930KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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