DISCOVERY OF PULSATIONS FROM THE PULSAR J0205+6449 IN SNR 3C 58 WITH THE FERMI GAMMA-RAY SPACE TELESCOPE
DISCOVERY OF PULSATIONS FROM THE PULSAR J0205+6449 IN SNR 3C 58 WITH THE FERMI GAMMA-RAY SPACE TELESCOPE
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DOI：
10.1088/0004-637x/699/2/l102
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发表时间：
2009-07
期刊：
影响因子：
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通讯作者：
A. Abdo;M. Ackermann;M. Ajello;W. Atwood;M. Axelsson;L. Baldini;J. Ballet;G. Barbiellini;D. Bastieri;B. Baughman;K. Bechtol;R. Bellazzini;B. Berenji;R. Blandford;E. Bloom;E. Bonamente;A. Borgland;A. Bouvier;J. Bregeon;A. Brez;M. Brigida;P. Bruel;T. Burnett;G. Caliandro;R. Cameron;F. Camilo;P. Caraveo;J. Casandjian;C. Cecchi;O. Celik;A. Chekhtman;C. C. Cheung-C.;J. Chiang;S. Ciprini;R. Claus;I. Cognard;J. Cohen-Tanugi;J. Conrad;C. Dermer;A. Angelis;F. Palma;S. Digel;M. Dormody;E. Silva;P. Drell;R. Dubois;D. Dumora;Y. Edmonds;C. Espinoza;C. Farnier;C. Favuzzi;W. Focke;M. Frailis;P. Freire;Y. Fukazawa;P. Fusco;F. Gargano;N. Gehrels;S. Germani;B. Giebels;N. Giglietto;F. Giordano;T. Glanzman;G. Godfrey;I. Grenier;M. Grondin;J. Grove;L. Guillemot;S. Guiriec;Y. Hanabata;A. Harding;M. Hayashida;E. Hays;G. Hobbs;R. Hughes;G. Jóhannesson;A. Johnson;R. Johnson;T. Johnson;W. Johnson;S. Johnston;T. Kamae;V. Kaspi;H. Katagiri;J. Kataoka;N. Kawai;M. Keith;M. Kerr;J. Knödlseder;M. Kramer;F. Kuehn;M. Kuss;J. Lande;L. Latronico;M. Lemoine-Goumard;M. Livingstone;F. Longo;F. Loparco;B. Lott;M. Lovellette;P. Lubrano;A. Lyne;A. Makeev;R. Manchester;M. Marelli;M. Mazziotta;J. Mcenery;C. Meurer;P. Michelson;W. Mitthumsiri;T. Mizuno;A. Moiseev;C. Monte;M. Monzani;A. Morselli;I. Moskalenko;S. Murgia;P. Nolan;E. Nuss;T. Ohsugi;N. Omodei;E. Orlando;J. Ormes;D. Paneque;J. Panetta;D. Parent;V. Pelassa;M. Pepe;M. Pesce-Rollins;M. Pierbattista;F. Piron;T. Porter;S. Rainò;R. Rando;S. Ransom;M. Razzano;A. Reimer;O. Reimer;T. Reposeur;S. Ritz;L. Rochester;A. Rodríguez;R. Romani;F. Ryde;H. Sadrozinski;D. Sanchez;A. Sander;P. Parkinson;C. Sgro’;E. Siskind;D. Smith;P. Smith;G. Spandre;P. Spinelli;B. Stappers;E. Striani;M. Strickman;D. Suson;H. Tajima;H. Takahashi;Takaaki Tanaka;J. Thayer;J. Thayer;G. Theureau;D. Thompson;S. Thorsett;L. Tibaldo;D. Torres;G. Tosti;A. Tramacere;Y. Uchiyama;T. Usher;A. V. Etten;V. Vasileiou;N. Vilchez;V. Vitale;A. Waite;Pengfei Wang;K. Watters;P. Weltevrede;B. Winer;K. Wood;T. Ylinen;M. Ziegler
中科院分区：
文献类型：
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作者：
A. Abdo;M. Ackermann;M. Ajello;W. Atwood;M. Axelsson;L. Baldini;J. Ballet;G. Barbiellini;D. Bastieri;B. Baughman;K. Bechtol;R. Bellazzini;B. Berenji;R. Blandford;E. Bloom;E. Bonamente;A. Borgland;A. Bouvier;J. Bregeon;A. Brez;M. Brigida;P. Bruel;T. Burnett;G. Caliandro;R. Cameron;F. Camilo;P. Caraveo;J. Casandjian;C. Cecchi;O. Celik;A. Chekhtman;C. C. Cheung-C.;J. Chiang;S. Ciprini;R. Claus;I. Cognard;J. Cohen-Tanugi;J. Conrad;C. Dermer;A. Angelis;F. Palma;S. Digel;M. Dormody;E. Silva;P. Drell;R. Dubois;D. Dumora;Y. Edmonds;C. Espinoza;C. Farnier;C. Favuzzi;W. Focke;M. Frailis;P. Freire;Y. Fukazawa;P. Fusco;F. Gargano;N. Gehrels;S. Germani;B. Giebels;N. Giglietto;F. Giordano;T. Glanzman;G. Godfrey;I. Grenier;M. Grondin;J. Grove;L. Guillemot;S. Guiriec;Y. Hanabata;A. Harding;M. Hayashida;E. Hays;G. Hobbs;R. Hughes;G. Jóhannesson;A. Johnson;R. Johnson;T. Johnson;W. Johnson;S. Johnston;T. Kamae;V. Kaspi;H. Katagiri;J. Kataoka;N. Kawai;M. Keith;M. Kerr;J. Knödlseder;M. Kramer;F. Kuehn;M. Kuss;J. Lande;L. Latronico;M. Lemoine-Goumard;M. Livingstone;F. Longo;F. Loparco;B. Lott;M. Lovellette;P. Lubrano;A. Lyne;A. Makeev;R. Manchester;M. Marelli;M. Mazziotta;J. Mcenery;C. Meurer;P. Michelson;W. Mitthumsiri;T. Mizuno;A. Moiseev;C. Monte;M. Monzani;A. Morselli;I. Moskalenko;S. Murgia;P. Nolan;E. Nuss;T. Ohsugi;N. Omodei;E. Orlando;J. Ormes;D. Paneque;J. Panetta;D. Parent;V. Pelassa;M. Pepe;M. Pesce-Rollins;M. Pierbattista;F. Piron;T. Porter;S. Rainò;R. Rando;S. Ransom;M. Razzano;A. Reimer;O. Reimer;T. Reposeur;S. Ritz;L. Rochester;A. Rodríguez;R. Romani;F. Ryde;H. Sadrozinski;D. Sanchez;A. Sander;P. Parkinson;C. Sgro’;E. Siskind;D. Smith;P. Smith;G. Spandre;P. Spinelli;B. Stappers;E. Striani;M. Strickman;D. Suson;H. Tajima;H. Takahashi;Takaaki Tanaka;J. Thayer;J. Thayer;G. Theureau;D. Thompson;S. Thorsett;L. Tibaldo;D. Torres;G. Tosti;A. Tramacere;Y. Uchiyama;T. Usher;A. V. Etten;V. Vasileiou;N. Vilchez;V. Vitale;A. Waite;Pengfei Wang;K. Watters;P. Weltevrede;B. Winer;K. Wood;T. Ylinen;M. Ziegler
我们报告了在银河系超新星遗迹3C 58中发现的年轻射电和X射线脉冲星PSR J 0205 + 6449的γ射线脉动（~ 0.1 GeV）。γ射线波段的数据是由费米伽马射线太空望远镜上的大面积望远镜（以前的GLAST）获得的，而用于折叠γ射线的无线电旋转星历是由位于约德雷尔班克的绿色班克望远镜和洛弗尔望远镜获得的。光变曲线由两个峰组成，间隔0.49 ± 0.01 ± 0.01个周期，与X射线峰对齐。第一个γ射线峰比射电脉冲滞后0.08 ± 0.01 ± 0.01，但其振幅随能量的增加而减小。脉冲γ射线发射的光谱分析表明，其指数为−2.1 ± 0.1 ± 0.2，指数截止值为3.0+1.1−0.7 ± 0.4 GeV。第一个不确定性是统计的，第二个是系统的。在0.1 GeV以上的积分γ射线光子通量为（13.7 ± 1.4 ± 3.0）× 10−8 cm−2 s−1，这意味着对于3.2 kpc的距离，假设一个宽的扇形光束，光度为8.3 × 1034 erg s−1，效率η为0.3%。最后，我们报告了一个95%的上限通量为1.7 × 10−8 cm−2 s−1的关闭脉冲发射的对象。
We report the discovery of γ-ray pulsations (⩾0.1 GeV) from the young radio and X-ray pulsar PSR J0205 + 6449 located in the Galactic supernova remnant 3C 58. Data in the γ-ray band were acquired by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope (formerly GLAST), while the radio rotational ephemeris used to fold γ-rays was obtained using both the Green Bank Telescope and the Lovell telescope at Jodrell Bank. The light curve consists of two peaks separated by 0.49 ± 0.01 ± 0.01 cycles which are aligned with the X-ray peaks. The first γ-ray peak trails the radio pulse by 0.08 ± 0.01 ± 0.01, while its amplitude decreases with increasing energy as for the other γ-ray pulsars. Spectral analysis of the pulsed γ-ray emission suggests a simple power law of index −2.1 ± 0.1 ± 0.2 with an exponential cutoff at 3.0+1.1−0.7 ± 0.4 GeV. The first uncertainty is statistical and the second is systematic. The integral γ-ray photon flux above 0.1 GeV is (13.7 ± 1.4 ± 3.0) × 10−8 cm−2 s−1, which implies for a distance of 3.2 kpc and assuming a broad fan-like beam a luminosity of 8.3 × 1034 erg s−1 and an efficiency η of 0.3%. Finally, we report a 95% upper limit on the flux of 1.7 × 10−8 cm−2 s−1 for off-pulse emission from the object.