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Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations

Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive b... Full description

Journal Title: arXiv.org Nov 26, 2012
Main Author: Pletsch, H
Other Authors: Guillemot, L , Fehrmann, H , Allen, B , Kramer, M , Aulbert, C , Ackermann, M , Ajello, M , de Angelis, A , Atwood, W , Baldini, L , Ballet, J , Barbiellini, G , Bastieri, D , Bechtol, K , Bellazzini, R , Borgland, A , Bottacini, E , Brandt, T , Bregeon, J , Brigida, M , Bruel, P , Buehler, R , Buson, S , Caliandro, G , Cameron, R , Caraveo, P , Casandjian, J , Cecchi, C , Celik, Ö , Charles, E , Chaves, R , Cheung, C , Chiang, J , Ciprini, S , Claus, R , Cohen-Tanugi, J , Conrad, J , Cutini, S , D'Ammando, F , Dermer, C , Digel, S , Drell, P , Drlica-Wagner, A , Dubois, R , Dumora, D , Favuzzi, C , Ferrara, E , Franckowiak, A , Fukazawa, Y , Fusco, P , Gargano, F , Gehrels, N , Germani, S , Giglietto, N , Giordano, F , Giroletti, M , Godfrey, G , Grenier, I , Grove, J , Guiriec, S , Hadasch, D , Hanabata, Y , Harding, A , Den Hartog, P , Hayashida, M , Hays, E , Hill, A , Hou, X , Hughes, R , Johannesson, G , Jackson, M , Jogler, T , Johnson, A , Johnson, W , Kataoka, J , Kerr, M , Knödlseder, J , Kuss, M , Lande, J , Larsson, S , Latronico, L , Lemoine-Goumard, M , Longo, F , Loparco, F , Lovellette, M , Lubrano, P , Massaro, F , Mayer, M , Mazziotta, M , Mcenery, J , Mehault, J , Michelson, P , Mitthumsiri, W , Mizuno, T , Monzani, M , Morselli, A , Moskalenko, I , Murgia, S , Nakamori, T , Nemmen, R , Nuss, E , Ohno, M , Ohsugi, T , Omodei, N , Orienti, M , Orlando, E , de Palma, F , Paneque, D , Perkins, J , Piron, F , Pivato, G , Porter, T , Raino, S , Rando, R , Ray, P , Razzano, M , Reimer, A , Reimer, O , Reposeur, T , Ritz, S , Romani, R , Romoli, C , Sanchez, D , Saz Parkinson, P , Schulz, A , Sgro, C , Siskind, E , Smith, D , Spandre, G , Spinelli, P , Suson, D , Takahashi, H , Tanaka, T , Thayer, J , Thayer, J , Thompson, D , Tibaldo, L , Tinivella, M , Troja, E , Usher, T , Vandenbroucke, J , Vasileiou, V , Vianello, G , Vitale, V , Waite, A , Winer, B , Wood, K , Wood, M , Yang, Z , Zimmer, S
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: DOI: 10.1126/science.1229054
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title: Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
format: Article
creator:
  • Pletsch, H
  • Guillemot, L
  • Fehrmann, H
  • Allen, B
  • Kramer, M
  • Aulbert, C
  • Ackermann, M
  • Ajello, M
  • de Angelis, A
  • Atwood, W
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Bastieri, D
  • Bechtol, K
  • Bellazzini, R
  • Borgland, A
  • Bottacini, E
  • Brandt, T
  • Bregeon, J
  • Brigida, M
  • Bruel, P
  • Buehler, R
  • Buson, S
  • Caliandro, G
  • Cameron, R
  • Caraveo, P
  • Casandjian, J
  • Cecchi, C
  • Celik, Ö
  • Charles, E
  • Chaves, R
  • Cheung, C
  • Chiang, J
  • Ciprini, S
  • Claus, R
  • Cohen-Tanugi, J
  • Conrad, J
  • Cutini, S
  • D'Ammando, F
  • Dermer, C
  • Digel, S
  • Drell, P
  • Drlica-Wagner, A
  • Dubois, R
  • Dumora, D
  • Favuzzi, C
  • Ferrara, E
  • Franckowiak, A
  • Fukazawa, Y
  • Fusco, P
  • Gargano, F
  • Gehrels, N
  • Germani, S
  • Giglietto, N
  • Giordano, F
  • Giroletti, M
  • Godfrey, G
  • Grenier, I
  • Grove, J
  • Guiriec, S
  • Hadasch, D
  • Hanabata, Y
  • Harding, A
  • Den Hartog, P
  • Hayashida, M
  • Hays, E
  • Hill, A
  • Hou, X
  • Hughes, R
  • Johannesson, G
  • Jackson, M
  • Jogler, T
  • Johnson, A
  • Johnson, W
  • Kataoka, J
  • Kerr, M
  • Knödlseder, J
  • Kuss, M
  • Lande, J
  • Larsson, S
  • Latronico, L
  • Lemoine-Goumard, M
  • Longo, F
  • Loparco, F
  • Lovellette, M
  • Lubrano, P
  • Massaro, F
  • Mayer, M
  • Mazziotta, M
  • Mcenery, J
  • Mehault, J
  • Michelson, P
  • Mitthumsiri, W
  • Mizuno, T
  • Monzani, M
  • Morselli, A
  • Moskalenko, I
  • Murgia, S
  • Nakamori, T
  • Nemmen, R
  • Nuss, E
  • Ohno, M
  • Ohsugi, T
  • Omodei, N
  • Orienti, M
  • Orlando, E
  • de Palma, F
  • Paneque, D
  • Perkins, J
  • Piron, F
  • Pivato, G
  • Porter, T
  • Raino, S
  • Rando, R
  • Ray, P
  • Razzano, M
  • Reimer, A
  • Reimer, O
  • Reposeur, T
  • Ritz, S
  • Romani, R
  • Romoli, C
  • Sanchez, D
  • Saz Parkinson, P
  • Schulz, A
  • Sgro, C
  • Siskind, E
  • Smith, D
  • Spandre, G
  • Spinelli, P
  • Suson, D
  • Takahashi, H
  • Tanaka, T
  • Thayer, J
  • Thayer, J
  • Thompson, D
  • Tibaldo, L
  • Tinivella, M
  • Troja, E
  • Usher, T
  • Vandenbroucke, J
  • Vasileiou, V
  • Vianello, G
  • Vitale, V
  • Waite, A
  • Winer, B
  • Wood, K
  • Wood, M
  • Yang, Z
  • Zimmer, S
subjects:
  • Neutrons
  • Gamma Rays
  • Circular Orbits
  • Binary Stars
  • Radio Emission
  • Deposition
  • Companion Stars
  • Gamma Rays
  • Pulsars
  • Stellar Rotation
  • Rotation
  • Neutron Stars
  • Millisecond Pulsars
  • High Energy Astrophysical Phenomena
  • Astrophysics of Galaxies
ispartof: arXiv.org, Nov 26, 2012
description: Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.
language: eng
source:
identifier: DOI: 10.1126/science.1229054
fulltext: fulltext_linktorsrc
url: Link


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titleBinary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
creatorPletsch, H ; Guillemot, L ; Fehrmann, H ; Allen, B ; Kramer, M ; Aulbert, C ; Ackermann, M ; Ajello, M ; de Angelis, A ; Atwood, W ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Borgland, A ; Bottacini, E ; Brandt, T ; Bregeon, J ; Brigida, M ; Bruel, P ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caraveo, P ; Casandjian, J ; Cecchi, C ; Celik, Ö ; Charles, E ; Chaves, R ; Cheung, C ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Cutini, S ; D'Ammando, F ; Dermer, C ; Digel, S ; Drell, P ; Drlica-Wagner, A ; Dubois, R ; Dumora, D ; Favuzzi, C ; Ferrara, E ; Franckowiak, A ; Fukazawa, Y ; Fusco, P ; Gargano, F ; Gehrels, N ; Germani, S ; Giglietto, N ; Giordano, F ; Giroletti, M ; Godfrey, G ; Grenier, I ; Grove, J ; Guiriec, S ; Hadasch, D ; Hanabata, Y ; Harding, A ; Den Hartog, P ; Hayashida, M ; Hays, E ; Hill, A ; Hou, X ; Hughes, R ; Johannesson, G ; Jackson, M ; Jogler, T ; Johnson, A ; Johnson, W ; Kataoka, J ; Kerr, M ; Knödlseder, J ; Kuss, M ; Lande, J ; Larsson, S ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lovellette, M ; Lubrano, P ; Massaro, F ; Mayer, M ; Mazziotta, M ; Mcenery, J ; Mehault, J ; Michelson, P ; Mitthumsiri, W ; Mizuno, T ; Monzani, M ; Morselli, A ; Moskalenko, I ; Murgia, S ; Nakamori, T ; Nemmen, R ; Nuss, E ; Ohno, M ; Ohsugi, T ; Omodei, N ; Orienti, M ; Orlando, E ; de Palma, F ; Paneque, D ; Perkins, J ; Piron, F ; Pivato, G ; Porter, T ; Raino, S ; Rando, R ; Ray, P ; Razzano, M ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Romani, R ; Romoli, C ; Sanchez, D ; Saz Parkinson, P ; Schulz, A ; Sgro, C ; Siskind, E ; Smith, D ; Spandre, G ; Spinelli, P ; Suson, D ; Takahashi, H ; Tanaka, T ; Thayer, J ; Thayer, J ; Thompson, D ; Tibaldo, L ; Tinivella, M ; Troja, E ; Usher, T ; Vandenbroucke, J ; Vasileiou, V ; Vianello, G ; Vitale, V ; Waite, A ; Winer, B ; Wood, K ; Wood, M ; Yang, Z ; Zimmer, S
contributorZimmer, S (pacrepositoryorg)
ispartofarXiv.org, Nov 26, 2012
identifierDOI: 10.1126/science.1229054
subjectNeutrons ; Gamma Rays ; Circular Orbits ; Binary Stars ; Radio Emission ; Deposition ; Companion Stars ; Gamma Rays ; Pulsars ; Stellar Rotation ; Rotation ; Neutron Stars ; Millisecond Pulsars ; High Energy Astrophysical Phenomena ; Astrophysics of Galaxies
descriptionMillisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.
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21Bruel, P
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26Caraveo, P
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28Cecchi, C
29Celik, Ö
30Charles, E
31Chaves, R
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33Chiang, J
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35Claus, R
36Cohen-Tanugi, J
37Conrad, J
38Cutini, S
39D'Ammando, F
40Dermer, C
41Digel, S
42Drell, P
43Drlica-Wagner, A
44Dubois, R
45Dumora, D
46Favuzzi, C
47Ferrara, E
48Franckowiak, A
49Fukazawa, Y
50Fusco, P
51Gargano, F
52Gehrels, N
53Germani, S
54Giglietto, N
55Giordano, F
56Giroletti, M
57Godfrey, G
58Grenier, I
59Grove, J
60Guiriec, S
61Hadasch, D
62Hanabata, Y
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64Den Hartog, P
65Hayashida, M
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82Lemoine-Goumard, M
83Longo, F
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87Massaro, F
88Mayer, M
89Mazziotta, M
90Mcenery, J
91Mehault, J
92Michelson, P
93Mitthumsiri, W
94Mizuno, T
95Monzani, M
96Morselli, A
97Moskalenko, I
98Murgia, S
99Nakamori, T
100...
titleBinary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
descriptionMillisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.
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3Binary Stars
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titleBinary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
authorPletsch, H ; Guillemot, L ; Fehrmann, H ; Allen, B ; Kramer, M ; Aulbert, C ; Ackermann, M ; Ajello, M ; de Angelis, A ; Atwood, W ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Borgland, A ; Bottacini, E ; Brandt, T ; Bregeon, J ; Brigida, M ; Bruel, P ; Buehler, R ; Buson, S ; Caliandro, G ; Cameron, R ; Caraveo, P ; Casandjian, J ; Cecchi, C ; Celik, Ö ; Charles, E ; Chaves, R ; Cheung, C ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Cutini, S ; D'Ammando, F ; Dermer, C ; Digel, S ; Drell, P ; Drlica-Wagner, A ; Dubois, R ; Dumora, D ; Favuzzi, C ; Ferrara, E ; Franckowiak, A ; Fukazawa, Y ; Fusco, P ; Gargano, F ; Gehrels, N ; Germani, S ; Giglietto, N ; Giordano, F ; Giroletti, M ; Godfrey, G ; Grenier, I ; Grove, J ; Guiriec, S ; Hadasch, D ; Hanabata, Y ; Harding, A ; Den Hartog, P ; Hayashida, M ; Hays, E ; Hill, A ; Hou, X ; Hughes, R ; Johannesson, G ; Jackson, M ; Jogler, T ; Johnson, A ; Johnson, W ; Kataoka, J ; Kerr, M ; Knödlseder, J ; Kuss, M ; Lande, J ; Larsson, S ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lovellette, M ; Lubrano, P ; Massaro, F ; Mayer, M ; Mazziotta, M ; Mcenery, J ; Mehault, J ; Michelson, P ; Mitthumsiri, W ; Mizuno, T ; Monzani, M ; Morselli, A ; Moskalenko, I ; Murgia, S ; Nakamori, T ; Nemmen, R ; Nuss, E ; Ohno, M ; Ohsugi, T ; Omodei, N ; Orienti, M ; Orlando, E ; de Palma, F ; Paneque, D ; Perkins, J ; Piron, F ; Pivato, G ; Porter, T ; Raino, S ; Rando, R ; Ray, P ; Razzano, M ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Romani, R ; Romoli, C ; Sanchez, D ; Saz Parkinson, P ; Schulz, A ; Sgro, C ; Siskind, E ; Smith, D ; Spandre, G ; Spinelli, P ; Suson, D ; Takahashi, H ; Tanaka, T ; Thayer, J ; Thayer, J ; Thompson, D ; Tibaldo, L ; Tinivella, M ; Troja, E ; Usher, T ; Vandenbroucke, J ; Vasileiou, V ; Vianello, G ; Vitale, V ; Waite, A ; Winer, B ; Wood, K ; Wood, M ; Yang, Z ; Zimmer, S
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99Nemmen
100...
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0Pletsch, H
1Guillemot, L
2Fehrmann, H
3Allen, B
4Kramer, M
5Aulbert, C
6Ackermann, M
7Ajello, M
8de Angelis, A
9Atwood, W
10Baldini, L
11Ballet, J
12Barbiellini, G
13Bastieri, D
14Bechtol, K
15Bellazzini, R
16Borgland, A
17Bottacini, E
18Brandt, T
19Bregeon, J
20Brigida, M
21Bruel, P
22Buehler, R
23Buson, S
24Caliandro, G
25Cameron, R
26Caraveo, P
27Casandjian, J
28Cecchi, C
29Celik, Ö
30Charles, E
31Chaves, R
32Cheung, C
33Chiang, J
34Ciprini, S
35Claus, R
36Cohen-Tanugi, J
37Conrad, J
38Cutini, S
39D'Ammando, F
40Dermer, C
41Digel, S
42Drell, P
43Drlica-Wagner, A
44Dubois, R
45Dumora, D
46Favuzzi, C
47Ferrara, E
48Franckowiak, A
49Fukazawa, Y
50Fusco, P
51Gargano, F
52Gehrels, N
53Germani, S
54Giglietto, N
55Giordano, F
56Giroletti, M
57Godfrey, G
58Grenier, I
59Grove, J
60Guiriec, S
61Hadasch, D
62Hanabata, Y
63Harding, A
64Den Hartog, P
65Hayashida, M
66Hays, E
67Hill, A
68Hou, X
69Hughes, R
70Johannesson, G
71Jackson, M
72Jogler, T
73Johnson, A
74Johnson, W
75Kataoka, J
76Kerr, M
77Knödlseder, J
78Kuss, M
79Lande, J
80Larsson, S
81Latronico, L
82Lemoine-Goumard, M
83Longo, F
84Loparco, F
85Lovellette, M
86Lubrano, P
87Massaro, F
88Mayer, M
89Mazziotta, M
90Mcenery, J
91Mehault, J
92Michelson, P
93Mitthumsiri, W
94Mizuno, T
95Monzani, M
96Morselli, A
97Moskalenko, I
98Murgia, S
99Nakamori, T
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atitleBinary Millisecond Pulsar Discovery via Gamma-Ray Pulsations
jtitlearXiv.org
risdate20121126
formatjournal
genrearticle
ristypeJOUR
abstractMillisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled" rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.
copIthaca
pubCornell University Library, arXiv.org
doi10.1126/science.1229054
urlhttp://search.proquest.com/docview/2086665278/
issue6112
pages1314-1317
orcidid0000-0001-6885-7156
volume338
issn00368075
eissn10959203
oafree_for_read
date2012-12-07