Institutional Repository of Radio Astronomy Research Laboratory
| 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.6,7; Ballet, J.8; Baring, M. G.9; Bassa, C.10; Becerra Gonzalez, J.11,12; Bellazzini, R.7; Berretta, A.13; Bhattacharyya, B.14; Bissaldi, E.15,16; Bonino, R.17,18; Bottacini, E.19,20,21; Bregeon, J.22; Bruel, P.23; Burgay, M.24; Burnett, T. H.25; Cameron, R. A.20,21; Camilo, F.26; Caputo, R.27; Caraveo, P. A.28; Cavazzuti, E.29; Chiaro, G.28; Ciprini, S.30,31; Clark, C. J.32,33; Cognard, I.34,35; Corongiu, A.24; Cristarella Orestano, P.13,36; Crnogorcevic, M.27,37; Cuoco, A.17,18; Cutini, S.36; D'Ammando, F.38; de Angelis, A.39,40; DeCesar, M. E.41,42; De Gaetano, S.15,16; de Menezes, R.17,43; Deneva, J.41,42; de Palma, F.44,45; Di Lalla, N.20,21; Dirirsa, F.46,47; Di Venere, L.16; Dominguez, A.48; Dumora, D.1; Fegan, S. J.23; Ferrara, E. C.27,37,49,50; Fiori, A.6,7; Fleischhack, H.27,49,50,51; Flynn, C.5,52; Franckowiak, A.53; Freire, P. C. C.54; Fukazawa, Y.55; Fusco, P.15,16; Galanti, G.28; Gammaldi, V56,57; Gargano, F.16; Gasparrini, D.30,31; Giacchino, F.30,31; Giglietto, N.15,16; Giordano, F.15,16; Giroletti, M.38; Green, D.58; Grenier, I. A.59; Guillemot, L.34,35; Guiriec, S.27,60; Gustafsson, M.61; Harding, A. K.62; Hays, E.27; Hewitt, J. W.63; Horan, D.23; Hou, X.64,65; Jankowski, F.34; Johnson, R. P.66,67; Johnson, T. J.41,42; Johnston, S.68; Kataoka, J.69; Keith, M. J.70; Kerr, M.71; Kramer, M.54,70,72; Kuss, M.7; Latronico, L.17; Lee, S. -H73; Li, D.74,75; Li, J.76,77; Limyansky, B.66,67; Longo, F.78,79; Loparco, F.15,16; Lorusso, L.15,16; Lovellette, M. N.80; Lower, M.68; Lubrano, P.36; Lyne, A. G.70; Maan, Y.14; Maldera, S.17; Manchester, R. N.68; Manfreda, A.6,7; Marelli, M.28; Marti-Devesa, G.81; Mazziotta, M. N.16; McEnery, J. E.27,37; Mereu, I13,36; Michelson, P. F.20,21; Mickaliger, M.70; Mitthumsiri, W.82; Mizuno, T.83; Moiseev, A. A.27,37,49,50; Monzani, M. E.20,21,84; Morselli, A.30; Negro, M.27,85,86; Nemmen, R.43; Nieder, L.32,33; Nuss, E.87; Omodei, N.20,21; Orienti, M.38; Orlando, E.20,21,88,89; Ormes, J. F.90; Palatiello, M.39,40,78,79,91; Paneque, D.58; Panzarini, G.15,16; Parthasarathy, A.54; Persic, M.79,92; Pesce-Rollins, M.7; Pillera, R.15,16; Poon, H.55; Porter, T. A.20,21; Possenti, A.24; Principe, G.38,78,79; Raino, S.15,16; Rando, R.19,93,94; Ransom, S. M.95; Ray, P. S.71; Razzano, M.6,7; Razzaque, S.60,96,97; Reimer, A.81; Reimer, O.81; Renault-Tinacci, N.98; Romani, R. W.20,21; Sanchez-Conde, M.56,57; Saz Parkinson, P. M.66,67; Scotton, L.87; Serini, D.16; Sgro, C.7; Shannon, R.52; Sharma, V.27,49,50; Shen, Z.99; Siskind, E. J.100; Spandre, G.7; Spinelli, P.15,16; Stappers, B. W.70; Stephens, T. E.27,101; Suson, D. J.102; Tabassum, S.103; Tajima, H.104,105; Tak, D.106; Theureau, G.34,35; Thompson, D. J.27; Tibolla, O.107; Torres, D. F.108,109,110; Valverde, J.27,85,86; Venter, C.111; Wadiasingh, Z.27; Wang, N.112 ; Wang, P.113,114; Weltevrede, P.70; Wood, K.42,115; Yan, J.113; Zaharijas, G.116; Zhang, C.113; Zhu, W.113,114
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| 2023-12-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
 |
| ISSN | 0004-637X |
| Volume | 958Issue:2Pages:191 |
| Contribution Rank | 102 |
| Abstract | 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. |
| DOI | 10.3847/1538-4357/acee67 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | 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 |
| Funding Project | Istituto Nazionale diAstrofisica in Italy ; Centre National d'Etudes Spatialesin France ; DOE[DE-AC02-76SF00515] ; Commonwealth Government ; ISSI (Bern, Switzerland) |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001117603900001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | Istituto Nazionale diAstrofisica in Italy ; Centre National d'Etudes Spatialesin France ; DOE ; Commonwealth Government ; ISSI (Bern, Switzerland) |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5682 |
| Collection | 射电天文研究室_脉冲星研究团组 |
| Corresponding Author | Smith, D. A.; Bruel, P.; Clark, C. J.; Guillemot, L.; Kerr, M. |
| Affiliation | 1.Univ Bordeaux, CNRS, UMR 5797, Bordeaux LP2I, F-33170 Gradignan, France 2.Univ Bordeaux, CNRS, B18N, Lab Astrophys Bordeaux, Allee Geoffroy St Hilaire, F-33615 Pessac, France 3.Univ Toulouse, IRAP, CNRS, UPS, CNES, F-31028 Toulouse, France 4.Clemson Univ, Dept Phys & Astron, Kinard Lab Phys, Clemson, SC 29634 USA 5.Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia 6.Univ Pisa, I-56127 Pisa, Italy 7.Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy 8.Univ Paris Cite, Univ Paris Saclay, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France 9.Rice Univ, Dept Phys & Astron, MS-108,POB 1892, Houston, TX 77251 USA 10.Netherlands Inst Radio Astron, ASTRON, Postbus 2, NL-7990 AA Dwingeloo, Netherlands 11.Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Tenerife, Spain 12.Univ La Guajira, Dpto Astrofis, E-38200 San Cristobal la Laguna, Tenerife, Spain 13.Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy 14.Tata Inst Fundamental Res, 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110.ICREA, E-08010 Barcelona, Spain 111.North West Univ, Ctr Space Res, Potchefstroom Campus,Private Bag X6001, ZA-2520 Potchefstroom, South Africa 112.Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 113.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China 114.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China 115.Praxis Inc, Alexandria, VA 22303 USA 116.Univ Nova Gorica, Ctr Astrophys & Cosmol, Nova Gorica, Slovenia |
| Recommended Citation 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):191. |
| 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),191. |
| MLA | Smith, D. A.,et al."The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars".ASTROPHYSICAL JOURNAL 958.2(2023):191. |
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| Smith-2023-The Third（10775KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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