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Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT

Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi L... Full description

Journal Title: Science (New York N.Y.), 14 August 2009, Vol.325(5942), pp.840-4
Main Author: Abdo, A A
Other Authors: Ackermann, M , Ajello, M , Anderson, B , Atwood, W B , Axelsson, M , Baldini, L , Ballet, J , Barbiellini, G , Baring, M G , Bastieri, D , Baughman, B M , Bechtol, K , Bellazzini, R , Berenji, B , Bignami, G F , Blandford, R D , Bloom, E D , Bonamente, E , Borgland, A W , Bregeon, J , Brez, A , Brigida, M , Bruel, P , Burnett, T H , Caliandro, G A , Cameron, R A , Caraveo, P A , Casandjian, J M , Cecchi, C , Celik, O , Chekhtman, A , Cheung, C C , Chiang, J , Ciprini, S , Claus, R , Cohen-Tanugi, J , Conrad, J , Cutini, S , Dermer, C D , De Angelis, A , De Luca, A , De Palma, F , Digel, S W , Dormody, M , Do Couto E Silva, E , Drell, P S , Dubois, R , Dumora, D , Farnier, C , Favuzzi, C , Fegan, S J , Fukazawa, Y , Funk, S , Fusco, P , Gargano, F , Gasparrini, D , Gehrels, N , Germani, S , Giebels, B , Giglietto, N , Giommi, P , Giordano, F , Glanzman, T , Godfrey, G , Grenier, I A , Grondin, M-H , Grove, J E , Guillemot, L , Guiriec, S , Gwon, C , Hanabata, Y , Harding, A K , Hayashida, M , Hays, E , Hughes, R E , Jóhannesson, G , Johnson, R P , Johnson, T J , Johnson, W N , Kamae, T , Katagiri, H , Kataoka, J , Kawai, N , Kerr, M , Knödlseder, J , Kocian, M L , Kuss, M , Lande, J , Latronico, L , Lemoine-Goumard, M , Longo, F , Loparco, F , Lott, B , Lovellette, M N , Lubrano, P , Madejski, G M , Makeev, A , Marelli, M , Mazziotta, M N , Mcconville, W , Mcenery, J E , Meurer, C , Michelson, P F , Mitthumsiri, W , Mizuno, T , Monte, C , Monzani, M E , Morselli, A , Moskalenko, I V , Murgia, S , Nolan, P L , Norris, J P , Nuss, E , Ohsugi, T , Omodei, N , Orlando, E , Ormes, J F , Paneque, D , Parent, D , Pelassa, V , Pepe, M , Pesce-Rollins, M , Pierbattista, M , Piron, F , Porter, T A , Primack, J R , Rainò, S , Rando, R , Ray, P S , Razzano, M , Rea, N , Reimer, A , Reimer, O , Reposeur, T , Ritz, S , Rochester, L S , Rodriguez, A Y , Romani, R W , Ryde, F , Sadrozinski, H F-W , Sanchez, D , Sander, A , Saz Parkinson, P M , Scargle, J D , Sgrò, C , Siskind, E J , Smith, D A , Smith, P D , Spandre, G , Spinelli, P , Starck, J-L , Strickman, M S , Suson, D J , Tajima, H , Takahashi, H , Takahashi, T , Tanaka, T , Thayer, J G , Thompson, D J , Tibaldo, L , Tibolla, O , Torres, D F , Tosti, G , Tramacere, A , Uchiyama, Y , Usher, T L , Van Etten, A , Vasileiou, V , Vilchez, N , Vitale, V , Waite, A P , Wang, P , Watters, K , Winer, B L , Wolff, M T , Wood, K S , Ylinen, T , Ziegler, M
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; PMID: 19574346 Version:1 ; DOI: 10.1126/science.1175558
Link: http://pubmed.gov/19574346
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title: Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
format: Article
creator:
  • Abdo, A A
  • Ackermann, M
  • Ajello, M
  • Anderson, B
  • Atwood, W B
  • Axelsson, M
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Baring, M G
  • Bastieri, D
  • Baughman, B M
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Bignami, G F
  • Blandford, R D
  • Bloom, E D
  • Bonamente, E
  • Borgland, A W
  • Bregeon, J
  • Brez, A
  • Brigida, M
  • Bruel, P
  • Burnett, T H
  • Caliandro, G A
  • Cameron, R A
  • Caraveo, P A
  • Casandjian, J M
  • Cecchi, C
  • Celik, O
  • Chekhtman, A
  • Cheung, C C
  • Chiang, J
  • Ciprini, S
  • Claus, R
  • Cohen-Tanugi, J
  • Conrad, J
  • Cutini, S
  • Dermer, C D
  • De Angelis, A
  • De Luca, A
  • De Palma, F
  • Digel, S W
  • Dormody, M
  • Do Couto E Silva, E
  • Drell, P S
  • Dubois, R
  • Dumora, D
  • Farnier, C
  • Favuzzi, C
  • Fegan, S J
  • Fukazawa, Y
  • Funk, S
  • Fusco, P
  • Gargano, F
  • Gasparrini, D
  • Gehrels, N
  • Germani, S
  • Giebels, B
  • Giglietto, N
  • Giommi, P
  • Giordano, F
  • Glanzman, T
  • Godfrey, G
  • Grenier, I A
  • Grondin, M-H
  • Grove, J E
  • Guillemot, L
  • Guiriec, S
  • Gwon, C
  • Hanabata, Y
  • Harding, A K
  • Hayashida, M
  • Hays, E
  • Hughes, R E
  • Jóhannesson, G
  • Johnson, R P
  • Johnson, T J
  • Johnson, W N
  • Kamae, T
  • Katagiri, H
  • Kataoka, J
  • Kawai, N
  • Kerr, M
  • Knödlseder, J
  • Kocian, M L
  • Kuss, M
  • Lande, J
  • Latronico, L
  • Lemoine-Goumard, M
  • Longo, F
  • Loparco, F
  • Lott, B
  • Lovellette, M N
  • Lubrano, P
  • Madejski, G M
  • Makeev, A
  • Marelli, M
  • Mazziotta, M N
  • Mcconville, W
  • Mcenery, J E
  • Meurer, C
  • Michelson, P F
  • Mitthumsiri, W
  • Mizuno, T
  • Monte, C
  • Monzani, M E
  • Morselli, A
  • Moskalenko, I V
  • Murgia, S
  • Nolan, P L
  • Norris, J P
  • Nuss, E
  • Ohsugi, T
  • Omodei, N
  • Orlando, E
  • Ormes, J F
  • Paneque, D
  • Parent, D
  • Pelassa, V
  • Pepe, M
  • Pesce-Rollins, M
  • Pierbattista, M
  • Piron, F
  • Porter, T A
  • Primack, J R
  • Rainò, S
  • Rando, R
  • Ray, P S
  • Razzano, M
  • Rea, N
  • Reimer, A
  • Reimer, O
  • Reposeur, T
  • Ritz, S
  • Rochester, L S
  • Rodriguez, A Y
  • Romani, R W
  • Ryde, F
  • Sadrozinski, H F-W
  • Sanchez, D
  • Sander, A
  • Saz Parkinson, P M
  • Scargle, J D
  • Sgrò, C
  • Siskind, E J
  • Smith, D A
  • Smith, P D
  • Spandre, G
  • Spinelli, P
  • Starck, J-L
  • Strickman, M S
  • Suson, D J
  • Tajima, H
  • Takahashi, H
  • Takahashi, T
  • Tanaka, T
  • Thayer, J G
  • Thompson, D J
  • Tibaldo, L
  • Tibolla, O
  • Torres, D F
  • Tosti, G
  • Tramacere, A
  • Uchiyama, Y
  • Usher, T L
  • Van Etten, A
  • Vasileiou, V
  • Vilchez, N
  • Vitale, V
  • Waite, A P
  • Wang, P
  • Watters, K
  • Winer, B L
  • Wolff, M T
  • Wood, K S
  • Ylinen, T
  • Ziegler, M
subjects:
  • Astrophysics - Galaxy Astrophysics
  • Astrophysics - High Energy Astrophysical Phenomena
ispartof: Science (New York, N.Y.), 14 August 2009, Vol.325(5942), pp.840-4
description: Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
language: eng
source:
identifier: E-ISSN: 1095-9203 ; PMID: 19574346 Version:1 ; DOI: 10.1126/science.1175558
fulltext: fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
creatorAbdo, A A ; Ackermann, M ; Ajello, M ; Anderson, B ; Atwood, W B ; Axelsson, M ; Baldini, L ; Ballet, J ; Barbiellini, G ; Baring, M G ; Bastieri, D ; Baughman, B M ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bignami, G F ; Blandford, R D ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Caliandro, G A ; Cameron, R A ; Caraveo, P A ; Casandjian, J M ; Cecchi, C ; Celik, O ; Chekhtman, A ; Cheung, C C ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Cutini, S ; Dermer, C D ; De Angelis, A ; De Luca, A ; De Palma, F ; Digel, S W ; Dormody, M ; Do Couto E Silva, E ; Drell, P S ; Dubois, R ; Dumora, D ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giebels, B ; Giglietto, N ; Giommi, P ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grondin, M-H ; Grove, J E ; Guillemot, L ; Guiriec, S ; Gwon, C ; Hanabata, Y ; Harding, A K ; Hayashida, M ; Hays, E ; Hughes, R E ; Jóhannesson, G ; Johnson, R P ; Johnson, T J ; Johnson, W N ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kocian, M L ; Kuss, M ; Lande, J ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Madejski, G M ; Makeev, A ; Marelli, M ; Mazziotta, M N ; Mcconville, W ; Mcenery, J E ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Paneque, D ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Pierbattista, M ; Piron, F ; Porter, T A ; Primack, J R ; Rainò, S ; Rando, R ; Ray, P S ; Razzano, M ; Rea, N ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Rochester, L S ; Rodriguez, A Y ; Romani, R W ; Ryde, F ; Sadrozinski, H F-W ; Sanchez, D ; Sander, A ; Saz Parkinson, P M ; Scargle, J D ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Starck, J-L ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Takahashi, T ; Tanaka, T ; Thayer, J G ; Thompson, D J ; Tibaldo, L ; Tibolla, O ; Torres, D F ; Tosti, G ; Tramacere, A ; Uchiyama, Y ; Usher, T L ; Van Etten, A ; Vasileiou, V ; Vilchez, N ; Vitale, V ; Waite, A P ; Wang, P ; Watters, K ; Winer, B L ; Wolff, M T ; Wood, K S ; Ylinen, T ; Ziegler, M
ispartofScience (New York, N.Y.), 14 August 2009, Vol.325(5942), pp.840-4
identifier
descriptionPulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
languageeng
source
subjectAstrophysics - Galaxy Astrophysics ; Astrophysics - High Energy Astrophysical Phenomena;
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0Abdo, A A
1Ackermann, M
2Ajello, M
3Anderson, B
4Atwood, W B
5Axelsson, M
6Baldini, L
7Ballet, J
8Barbiellini, G
9Baring, M G
10Bastieri, D
11Baughman, B M
12Bechtol, K
13Bellazzini, R
14Berenji, B
15Bignami, G F
16Blandford, R D
17Bloom, E D
18Bonamente, E
19Borgland, A W
20Bregeon, J
21Brez, A
22Brigida, M
23Bruel, P
24Burnett, T H
25Caliandro, G A
26Cameron, R A
27Caraveo, P A
28Casandjian, J M
29Cecchi, C
30Celik, O
31Chekhtman, A
32Cheung, C C
33Chiang, J
34Ciprini, S
35Claus, R
36Cohen-Tanugi, J
37Conrad, J
38Cutini, S
39Dermer, C D
40de Angelis, A
41de Luca, A
42de Palma, F
43Digel, S W
44Dormody, M
45do Couto e Silva, E
46Drell, P S
47Dubois, R
48Dumora, D
49Farnier, C
50Favuzzi, C
51Fegan, S J
52Fukazawa, Y
53Funk, S
54Fusco, P
55Gargano, F
56Gasparrini, D
57Gehrels, N
58Germani, S
59Giebels, B
60Giglietto, N
61Giommi, P
62Giordano, F
63Glanzman, T
64Godfrey, G
65Grenier, I A
66Grondin, M-H
67Grove, J E
68Guillemot, L
69Guiriec, S
70Gwon, C
71Hanabata, Y
72Harding, A K
73Hayashida, M
74Hays, E
75Hughes, R E
76Jóhannesson, G
77Johnson, R P
78Johnson, T J
79Johnson, W N
80Kamae, T
81Katagiri, H
82Kataoka, J
83Kawai, N
84Kerr, M
85Knödlseder, J
86Kocian, M L
87Kuss, M
88Lande, J
89Latronico, L
90Lemoine-Goumard, M
91Longo, F
92Loparco, F
93Lott, B
94Lovellette, M N
95Lubrano, P
96Madejski, G M
97Makeev, A
98Marelli, M
99Mazziotta, M N
100...
titleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
descriptionPulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
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titleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
authorAbdo, A A ; Ackermann, M ; Ajello, M ; Anderson, B ; Atwood, W B ; Axelsson, M ; Baldini, L ; Ballet, J ; Barbiellini, G ; Baring, M G ; Bastieri, D ; Baughman, B M ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bignami, G F ; Blandford, R D ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Caliandro, G A ; Cameron, R A ; Caraveo, P A ; Casandjian, J M ; Cecchi, C ; Celik, O ; Chekhtman, A ; Cheung, C C ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Cutini, S ; Dermer, C D ; De Angelis, A ; De Luca, A ; De Palma, F ; Digel, S W ; Dormody, M ; Do Couto E Silva, E ; Drell, P S ; Dubois, R ; Dumora, D ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giebels, B ; Giglietto, N ; Giommi, P ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grondin, M-H ; Grove, J E ; Guillemot, L ; Guiriec, S ; Gwon, C ; Hanabata, Y ; Harding, A K ; Hayashida, M ; Hays, E ; Hughes, R E ; Jóhannesson, G ; Johnson, R P ; Johnson, T J ; Johnson, W N ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kocian, M L ; Kuss, M ; Lande, J ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Madejski, G M ; Makeev, A ; Marelli, M ; Mazziotta, M N ; Mcconville, W ; Mcenery, J E ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Paneque, D ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Pierbattista, M ; Piron, F ; Porter, T A ; Primack, J R ; Rainò, S ; Rando, R ; Ray, P S ; Razzano, M ; Rea, N ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Rochester, L S ; Rodriguez, A Y ; Romani, R W ; Ryde, F ; Sadrozinski, H F-W ; Sanchez, D ; Sander, A ; Saz Parkinson, P M ; Scargle, J D ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Starck, J-L ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Takahashi, T ; Tanaka, T ; Thayer, J G ; Thompson, D J ; Tibaldo, L ; Tibolla, O ; Torres, D F ; Tosti, G ; Tramacere, A ; Uchiyama, Y ; Usher, T L ; Van Etten, A ; Vasileiou, V ; Vilchez, N ; Vitale, V ; Waite, A P ; Wang, P ; Watters, K ; Winer, B L ; Wolff, M T ; Wood, K S ; Ylinen, T ; Ziegler, M
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3Anderson, B
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6Baldini, L
7Ballet, J
8Barbiellini, G
9Baring, M G
10Bastieri, D
11Baughman, B M
12Bechtol, K
13Bellazzini, R
14Berenji, B
15Bignami, G F
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17Bloom, E D
18Bonamente, E
19Borgland, A W
20Bregeon, J
21Brez, A
22Brigida, M
23Bruel, P
24Burnett, T H
25Caliandro, G A
26Cameron, R A
27Caraveo, P A
28Casandjian, J M
29Cecchi, C
30Celik, O
31Chekhtman, A
32Cheung, C C
33Chiang, J
34Ciprini, S
35Claus, R
36Cohen-Tanugi, J
37Conrad, J
38Cutini, S
39Dermer, C D
40De Angelis, A
41De Luca, A
42De Palma, F
43Digel, S W
44Dormody, M
45Do Couto E Silva, E
46Drell, P S
47Dubois, R
48Dumora, D
49Farnier, C
50Favuzzi, C
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52Fukazawa, Y
53Funk, S
54Fusco, P
55Gargano, F
56Gasparrini, D
57Gehrels, N
58Germani, S
59Giebels, B
60Giglietto, N
61Giommi, P
62Giordano, F
63Glanzman, T
64Godfrey, G
65Grenier, I A
66Grondin, M-H
67Grove, J E
68Guillemot, L
69Guiriec, S
70Gwon, C
71Hanabata, Y
72Harding, A K
73Hayashida, M
74Hays, E
75Hughes, R E
76Jóhannesson, G
77Johnson, R P
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85Knödlseder, J
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87Kuss, M
88Lande, J
89Latronico, L
90Lemoine-Goumard, M
91Longo, F
92Loparco, F
93Lott, B
94Lovellette, M N
95Lubrano, P
96Madejski, G M
97Makeev, A
98Marelli, M
99Mazziotta, M N
100...
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41de Luca
42de Palma
43Digel
44Dormody
45Do Couto E Silva
46Drell
47Dubois
48Dumora
49Farnier
50Favuzzi
51Fegan
52Fukazawa
53Funk
54Fusco
55Gargano
56Gasparrini
57Gehrels
58Germani
59Giebels
60Giglietto
61Giommi
62Giordano
63Glanzman
64Godfrey
65Grenier
66Grondin
67Grove
68Guillemot
69Guiriec
70Gwon
71Hanabata
72Harding
73Hayashida
74Hays
75Hughes
76Jóhannesson
77Johnson
78Kamae
79Katagiri
80Kataoka
81Kawai
82Kerr
83Knödlseder
84Kocian
85Kuss
86Lande
87Latronico
88Lemoine-Goumard
89Longo
90Loparco
91Lott
92Lovellette
93Lubrano
94Madejski
95Makeev
96Marelli
97Mazziotta
98Mcconville
99Mcenery
100...
aufirst
0A A
1M
2B
3W B
4L
5J
6G
7M G
8D
9B M
10K
11R
12G F
13R D
14E D
15E
16A W
17A
18P
19T H
20G A
21R A
22P A
23J M
24C
25O
26C C
27S
28C D
29F
30S W
31P S
32S J
33Y
34N
35T
36I A
37M-H
38J E
39A K
40R E
41R P
42T J
43W N
44H
45M L
46M N
47G M
48W
49P F
50M E
51I V
52P L
53J P
54J F
55V
56T A
57J R
58L S
59A Y
60R W
61H F-W
62P M
63J D
64E J
65D A
66P D
67J-L
68M S
69D J
70J G
71D F
72T L
73A P
74B L
75M T
76K S
au
0Abdo, A A
1Ackermann, M
2Ajello, M
3Anderson, B
4Atwood, W B
5Axelsson, M
6Baldini, L
7Ballet, J
8Barbiellini, G
9Baring, M G
10Bastieri, D
11Baughman, B M
12Bechtol, K
13Bellazzini, R
14Berenji, B
15Bignami, G F
16Blandford, R D
17Bloom, E D
18Bonamente, E
19Borgland, A W
20Bregeon, J
21Brez, A
22Brigida, M
23Bruel, P
24Burnett, T H
25Caliandro, G A
26Cameron, R A
27Caraveo, P A
28Casandjian, J M
29Cecchi, C
30Celik, O
31Chekhtman, A
32Cheung, C C
33Chiang, J
34Ciprini, S
35Claus, R
36Cohen-Tanugi, J
37Conrad, J
38Cutini, S
39Dermer, C D
40de Angelis, A
41de Luca, A
42de Palma, F
43Digel, S W
44Dormody, M
45Do Couto E Silva, E
46Drell, P S
47Dubois, R
48Dumora, D
49Farnier, C
50Favuzzi, C
51Fegan, S J
52Fukazawa, Y
53Funk, S
54Fusco, P
55Gargano, F
56Gasparrini, D
57Gehrels, N
58Germani, S
59Giebels, B
60Giglietto, N
61Giommi, P
62Giordano, F
63Glanzman, T
64Godfrey, G
65Grenier, I A
66Grondin, M-H
67Grove, J E
68Guillemot, L
69Guiriec, S
70Gwon, C
71Hanabata, Y
72Harding, A K
73Hayashida, M
74Hays, E
75Hughes, R E
76Jóhannesson, G
77Johnson, R P
78Johnson, T J
79Johnson, W N
80Kamae, T
81Katagiri, H
82Kataoka, J
83Kawai, N
84Kerr, M
85Knödlseder, J
86Kocian, M L
87Kuss, M
88Lande, J
89Latronico, L
90Lemoine-Goumard, M
91Longo, F
92Loparco, F
93Lott, B
94Lovellette, M N
95Lubrano, P
96Madejski, G M
97Makeev, A
98Marelli, M
99Mazziotta, M N
100...
atitleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
jtitleScience (New York, N.Y.)
risdate20090814
volume325
issue5942
spage840
pages840-844
eissn1095-9203
formatjournal
genrearticle
ristypeJOUR
abstractPulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
doi10.1126/science.1175558
pmid19574346
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
issn00368075
oafree_for_read
date2009-08-14