中文版 | English
YNAO OpenIR  > 星系类星体研究组
The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars
Smith, D. A.1,2; Abdollahi, S.3; Ajello, M.4; Bailes, M.5; Baldini, L.6; Ballet, J.7; Baring, M. G.8; Bassa, C.9; Gonzalez, J. Becerra10; Bellazzini, R.11; Berretta, A.12; Bhattacharyya, B.13; Bissaldi, E.14,15; Bonino, R.16,17; Bottacini, E.18,19; Bregeon, J.20; Bruel, P.21; Burgay, M.22; Burnett, T. H.23; Cameron, R. A.19; Camilo, F.24; Caputo, R.25; Caraveo, P. A.26; Cavazzuti, E.27; Chiaro, G.26; Ciprini, S.28,29; Clark, C. J.30,31; Cognard, I.32,33; Corongiu, A.22; Orestano, P. Cristarella12,34; Crnogorcevic, M.25,35; Cuoco, A.16,17; Cutini, S.34; D'Ammando, F.36; Angelis, A. de37; DeCesar, M. E.38; Gaetano, S. De14,15; Menezes, R. de16,39; Deneva, J.38; Palma, F. de40,41; Lalla, N. Di19; Dirirsa, F.42; Venere, L. Di15; Domínguez, A.43; Dumora, D.1; Fegan, S. J.21; Ferrara, E. C.25,35,44; Fiori, A.6; Fleischhack, H.25,44,45; Flynn, C.5,46; Franckowiak, A.47; Freire, P. C. C.48; Fukazawa, Y.49; Fusco, P.14,15; Galanti, G.26; Gammaldi, V.50,51; Gargano, F.15; Gasparrini, D.28,29; Giacchino, F.28,29; Giglietto, N.14,15; Giordano, F.14,15; Giroletti, M.36; Green, D.52; Grenier, I. A.53; Guillemot, L.32,33; Guiriec, S.25,54; Gustafsson, M.55; Harding, A. K.56; Hays, E.25; Hewitt, J. W.57; Horan, D.21; Hou X(侯贤)58,59; Jankowski, F.32; Johnson, R. P.60; Johnson, T. J.38; Johnston, S.61; Kataoka, J.62; Keith, M. J.63; Kerr, M.64; Kramer, M.48,63,65; Kuss, M.11; Latronico, L.16; Lee, S.-H.66; Li, D.67,68; Li, J.69,70; Limyansky, B.60; Longo, F.71,72; Loparco, F.14,15; Lorusso, L.14,15; Lovellette, M. N.73; Lower, M.61; Lubrano, P.34; Lyne, A. G.63; Maan, Y.13; Maldera, S.16; Manchester, R. N.61; Manfreda, A.6; Marelli, M.26; Martí-Devesa, G.74; Mazziotta, M. N.15; McEnery, J. E.25,35; Mereu, I.12,34; Michelson, P. F.19; Mickaliger, M.63; Mitthumsiri, W.75; Mizuno, T.76; Moiseev, A. A.35,44; Monzani, M. E.19,77; Morselli, A.28; Negro, M.25,78; Nemmen, R.39; Nieder, L.30,31; Nuss, E.79; Omodei, N.19; Orienti, M.36; Orlando, E.19,80; Ormes, J. F.81; Palatiello, M.37,71,72,82; Paneque, D.52; Panzarini, G.14,15; Parthasarathy, A.48; Persic, M.72,83; Pesce-Rollins, M.11; Pillera, R.14,15; Poon, H.49; Porter, T. A.19; Possenti, A.22; Principe, G.36,71,72; Rainò, S.14,15; Rando, R.18,84,85; Ransom, S. M.86; Ray, P. S.64; Razzano, M.6; Razzaque, S.54,87; Reimer, A.74; Reimer, O.74; Renault-Tinacci, N.88; Romani, R. W.19; Sánchez-Conde, M.50,51; Parkinson, P. M. Saz60; Scotton, L.79; Serini, D.15; Sgrò, C.11; Shannon, R.46; Sharma, V.44; Shen, Z.89; Siskind, E. J.90; Spandre, G.11; Spinelli, P.14,15; Stappers, B. W.63; Stephens, T. E.25,91; Suson, D. J.92; Tabassum, S.93; Tajima, H.94,95; Tak, D.96; Theureau, G.32,33; Thompson, D. J.25; Tibolla, O.97; Torres, D. F.98,99,100; Valverde, J.25,78; Venter, C.101; Wadiasingh, Z.25; Wang, N.102; Wang, N.102; Wang, P.103,104; Weltevrede, P.63; Wood, K.105; Yan, J.103; Zaharijas, G.106; Zhang, C.103; Zhu, W.103,104
发表期刊ASTROPHYSICAL JOURNAL
2023-12-01
卷号958期号:2
DOI10.3847/1538-4357/acee67
产权排序第58完成单位
收录类别SCI
摘要We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems colocated with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to <= 11 known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with six undetected in radio. Overall, >= 236 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power E decreases to its observed minimum near 1033 erg s-1, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties, and fit results to guide and be compared with modeling results.
资助项目Istituto Nazionale diAstrofisica in Italy; Centre National d'Etudes Spatialesin France; DOE[DE-AC02-76SF00515]; Commonwealth Government; ISSI (Bern, Switzerland)
项目资助者Istituto Nazionale diAstrofisica in Italy ; Centre National d'Etudes Spatialesin France ; DOE[DE-AC02-76SF00515] ; Commonwealth Government ; ISSI (Bern, Switzerland)
语种英语
学科领域天文学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001117603900001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]HIGH-ENERGY EMISSION ; TRANSITIONAL MILLISECOND PULSAR ; NEUTRON-STAR BINARY ; MAGNETAR-LIKE PULSAR ; MIDDLE-AGED PULSAR ; BLACK-WIDOW PULSAR ; AT-HOME DISCOVERY ; X-RAY ; SUPERNOVA REMNANT ; MULTIWAVELENGTH OBSERVATIONS
引用统计
被引频次：33[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26445
专题星系类星体研究组
中国科学院天体结构与演化重点实验室
作者单位1.Université Bordeaux, CNRS, LP2I Bordeaux, UMR 5797, F-33170 Gradignan, France; [email protected];
2.Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, F-33615 Pessac, France;
3.IRAP, Université de Toulouse, CNRS, UPS, CNES, F-31028 Toulouse, France;
4.Department of Physics and Astronomy, Clemson University, Kinard Lab of Physics, Clemson, SC 29634-0978, USA;
5.Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn Victoria 3122, Australia;
6.Università di Pisa and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa I-56127 Pisa, Italy;
7.Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette Cedex, France;
8.Rice University, Department of Physics and Astronomy, MS-108, P.O. Box 1892, Houston, TX 77251, USA;
9.ASTRON, The Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, The Netherlands;
10.Instituto de Astrofísica de Canarias and Universidad de La Laguna, Dpto. Astrofísica, E-38200 La Laguna, Tenerife, Spain;
11.Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy;
12.Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy;
13.National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune 411 007, India;
14.Dipartimento di Fisica "M. Merlin" dell'Università e del Politecnico di Bari, via Amendola 173, I-70126 Bari, Italy;
15.Istituto Nazionale di Fisica Nucleare, Sezione di Bari, I-70126 Bari, Italy;
16.Istituto Nazionale di Fisica Nucleare, Sezione di Torino, I-10125 Torino, Italy;
17.Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy;
18.Dipartimento di Fisica e Astronomia "G. Galilei,"Università di Padova, Via F. Marzolo, 8, I-35131 Padova, Italy;
19.W.W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA;
20.CNRS-IN2P3, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Grenoble, France;
21.Laboratoire Leprince-Ringuet, CNRS/IN2P3, École polytechnique, Institut Polytechnique de Paris, F-91120 Palaiseau, France; [email protected];
22.INAF—Cagliari Astronomical Observatory, I-09012 Capoterra (CA), Italy;
23.Department of Physics, University of Washington, Seattle, WA 98195-1560, USA;
24.South African Radio Astronomy Observatory, 2 Fir Street, Observatory, 7925, South Africa;
25.NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA;
26.INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano, via E. Bassini 15, I-20133 Milano, Italy;
27.Italian Space Agency, Via del Politecnico snc, I-00133 Roma, Italy;
28.Istituto Nazionale di Fisica Nucleare, Sezione di Roma "Tor Vergata," I-00133 Roma, Italy;
29.Space Science Data Center—Agenzia Spaziale Italiana, Via del Politecnico, snc, I-00133, Roma, Italy;
30.Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany; [email protected];
31.Leibniz Universität Hannover, D-30167 Hannover, Germany;
32.Laboratoire de Physique et Chimie de l'Environnement et de l'Espace—Université d'Orléans/CNRS, F-45071 Orléans Cedex 02, France; [email protected];
33.Station de radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, F-18330 Nançay, France;
34.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy;
35.Department of Astronomy, University of Maryland, College Park, MD 20742, USA;
36.INAF Istituto di Radioastronomia, I-40129 Bologna, Italy;
37.Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I-33100 Udine, Italy;
38.College of Science, George Mason University, Fairfax, VA 22030, resident at Naval Research Laboratory, Washington, DC 20375, USA;
39.Instituto de Astronomia, Geofísica e Cincias Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, São Paulo—SP 05508-090, Brazil;
40.Dipartimento di Matematica e Fisica "E. De Giorgi,"Università del Salento, Lecce, Italy;
41.Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, I-73100 Lecce, Italy;
42.Astronomy and Astrophysics Research Development Department, Entoto Observatory and Research Center, Space Science and Geospatial Institute, Addis Ababa, Ethiopia;
43.Grupo de Altas Energías, Universidad Complutense de Madrid, E-28040 Madrid, Spain;
44.Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA;
45.Catholic University of America, Washington, DC 20064, USA;
46.ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Centre for Astrophysics and Supercomputing, Mail H29, Swinburne University of Technology, P.O. Box 218, Hawthorn, VIC 3122, Australia;
47.Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute (AIRUB), D-44780 Bochum, Germany;
48.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany;
49.Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan;
50.Departamento de Física Teórica, Universidad Autónoma de Madrid, E-28049 Madrid, Spain;
51.Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, E-28049 Madrid, Spain;
52.Max-Planck-Institut für Physik, D-80805 München, Germany;
53.Université Paris Cité, Université Paris-Saclay, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France;
54.The George Washington University, Department of Physics, 725 21st Street, NW, Washington, DC 20052, USA;
55.Georg-August University Göttingen, Institute for Theoretical Physics—Faculty of Physics, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany;
56.Los Alamos National Laboratory, Los Alamos, NM 87545, USA;
57.University of North Florida, Department of Physics, 1 UNF Drive, Jacksonville, FL 32224, USA;
58.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China;
59.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China;
60.Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA;
61.CSIRO Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia;
62.Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan;
63.Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, M13 9PL, UK;
64.Space Science Division, Naval Research Laboratory, Washington, DC 20375-5352, USA; [email protected];
65.University of Manchester, Manchester, M13 9PL, UK;
66.Department of Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan;
67.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China;
68.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa;
69.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, People's Republic of China;
70.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China;
71.Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy;
72.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy;
73.The Aerospace Corporation, 14745 Lee Road, Chantilly, VA 20151, USA;
74.Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria;
75.Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;
76.Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan;
77.Vatican Observatory, Castel Gandolfo, V-00120, Vatican City State;
78.Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA;
79.Laboratoire Univers et Particules de Montpellier, Université Montpellier, CNRS/IN2P3, F-34095 Montpellier, France;
80.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, and Università di Trieste, I-34127 Trieste, Italy;
81.Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA;
82.Università di Udine, I-33100 Udine, Italy;
83.INAF-Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy;
84.Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy;
85.Center for Space Studies and Activities "G. Colombo,"University of Padova, Via Venezia 15, I-35131 Padova, Italy;
86.National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, NM 87801, USA;
87.Centre for Astro-Particle Physics (CAPP) and Department of Physics, University of Johannesburg, P.O. Box 524, Auckland Park 2006, South Africa;
88.AIM, CEA, CNRS, Université Paris-Saclay, Université de Paris, F-91191 Gif-sur-Yvette, France;
89.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People's Republic of China;
90.NYCB Real-Time Computing Inc., Lattingtown, NY 11560-1025, USA;
91.Department of Physics and Astronomy, Brigham Young University, Provo, UT 84602, USA;
92.Purdue University Northwest, Hammond, IN 46323, USA;
93.Department of Physics and Astronomy, West Virginia University, Morgantown, WV 26506-6315, USA;
94.Nagoya University, Institute for Space-Earth Environmental Research, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan;
95.Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Japan;
96.SNU Astronomy Research Center, Seoul National University, Gwanak-rho, Gwanak-gu, Seoul, Republic of Korea;
97.Mesoamerican Centre for Theoretical Physics (MCTP), Universidad Autónoma de Chiapas (UNACH), Carretera Emiliano Zapata Km. 4, Real del Bosque (Teràn), 29050 Tuxtla Gutiérrez, Chiapas, México;
98.Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Magrans s/n, E-08193 Barcelona, Spain;
99.Institut d'Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain;
100.Institució Catalana de Recerca i Estudis Avançats (ICREA), E-08010 Barcelona, Spain;
101.Centre for Space Research, North-West University, Potchefstroom Campus, Private Bag X6001, Potchefstroom 2520, South Africa;
102.Xinjiang Astronomical Observatory, 150, Science 1-Street, Urumqi, Xinjiang 830011, People's Republic of China;
103.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China;
104.Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China;
105.Praxis Inc., Alexandria, VA 22303, resident at Naval Research Laboratory, Washington, DC 20375, USA;
106.Center for Astrophysics and Cosmology, University of Nova Gorica, Nova Gorica, Slovenia
推荐引用方式
GB/T 7714		 Smith, D. A.,Abdollahi, S.,Ajello, M.,et al. The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars[J]. ASTROPHYSICAL JOURNAL,2023,958(2).
APA Smith, D. A..,Abdollahi, S..,Ajello, M..,Bailes, M..,Baldini, L..,...&Zhu, W..(2023).The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars.ASTROPHYSICAL JOURNAL,958(2).
MLA Smith, D. A.,et al."The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars".ASTROPHYSICAL JOURNAL 958.2(2023).
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
The Third Fermi Larg（11032KB）期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Smith, D. A.]的文章
[Abdollahi, S.]的文章
[Ajello, M.]的文章
百度学术
百度学术中相似的文章
[Smith, D. A.]的文章
[Abdollahi, S.]的文章
[Ajello, M.]的文章
必应学术
必应学术中相似的文章
[Smith, D. A.]的文章
[Abdollahi, S.]的文章
[Ajello, M.]的文章
相关权益政策
暂无数据
收藏/分享
文件名： The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars.pdf
格式： Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。