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A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope

Context. Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. The observation of this emission provides a powerful tool to assess the millisecond pulsar population of a cluster, is essential for understa... Full description

Journal Title: Astronomy & Astrophysics 12/2010, Vol.524, p.A75
Main Author: Abdo, A. A.
Other Authors: Ackermann, M. , Ajello, M. , Baldini, L. , Ballet, J. , Barbiellini, G. , Bastieri, D. , Bellazzini, R. , Blandford, R. D. , Bloom, E. D. , Bonamente, E. , Borgland, A. W. , Bouvier, A. , Brandt, T. J. , Bregeon, J. , Brigida, M. , Bruel, P. , Buehler, R. , Buson, S. , Caliandro, G. A. , Cameron, R. A. , Caraveo, P. A. , Carrigan, S. , Casandjian, J. M. , Charles, E. , Chaty, S. , Chekhtman, A. , Cheung, C. C. , Chiang, J. , Ciprini, S. , Claus, R. , Cohen-Tanugi, J. , Conrad, J. , Decesar, M. E. , Dermer, C. D. , de Palma, F. , Digel, S. W. , Do Couto E Silva, E. , Drell, P. S. , Dubois, R. , Dumora, D. , Favuzzi, C. , Fortin, P. , Frailis, M. , Fukazawa, Y. , Fusco, P. , Gargano, F. , Gasparrini, D. , Gehrels, N. , Germani, S. , Giglietto, N. , Giordano, F. , Glanzman, T. , Godfrey, G. , Grenier, I. , Grondin, M.-H. , Grove, J. E. , Guillemot, L. , Guiriec, S. , Hadasch, D. , Harding, A. K. , Hays, E. , Jean, P. , Jóhannesson, G. , Johnson, T. J. , Johnson, W. N. , Kamae, T. , Katagiri, H. , Kataoka, J. , Kerr, M. , Knödlseder, J. , Kuss, M. , Lande, J. , Latronico, L. , Lee, S.-H. , Lemoine-Goumard, M. , Llena Garde, M. , Longo, F. , Loparco, F. , Lovellette, M. N. , Lubrano, P. , Makeev, A. , Mazziotta, M. N. , Michelson, P. F. , Mitthumsiri, W. , Mizuno, T. , Monte, C. , Monzani, M. E. , Morselli, A. , Moskalenko, I. V. , Murgia, S. , Naumann-Godo, M. , Nolan, P. L. , Norris, J. P. , Nuss, E. , Ohsugi, T. , Omodei, N. , Orlando, E. , Ormes, J. F. , Pancrazi, B. , Parent, D. , Pepe, M. , Pesce-Rollins, M. , Piron, F. , Porter, T. A. , Rainò, S. , Rando, R. , Reimer, A. , Reimer, O. , Reposeur, T. , Ripken, J. , Romani, R. W. , Roth, M. , Sadrozinski, H. F.-W. , Saz Parkinson, P. M. , Sgrò, C. , Siskind, E. J. , Smith, D. A. , Spinelli, P. , Strickman, M. S. , Suson, D. J. , Takahashi, H. , Takahashi, T. , Tanaka, T. , Thayer, J. B. , Thayer, J. G. , Tibaldo, L. , Torres, D. F. , Tosti, G. , Tramacere, A. , Uchiyama, Y. , Usher, T. L. , Vasileiou, V. , Venter, C. , Vilchez, N. , Vitale, V. , Waite, A. P. , Wang, P. , Webb, N. , Winer, B. L. , Yang, Z. , Ylinen, T. , Ziegler, M.
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: ISSN: 0004-6361 ; E-ISSN: 1432-0746 ; DOI: http://dx.doi.org/10.1051/0004-6361/201014458
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title: A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
format: Article
creator:
  • Abdo, A. A.
  • Ackermann, M.
  • Ajello, M.
  • Baldini, L.
  • Ballet, J.
  • Barbiellini, G.
  • Bastieri, D.
  • Bellazzini, R.
  • Blandford, R. D.
  • Bloom, E. D.
  • Bonamente, E.
  • Borgland, A. W.
  • Bouvier, A.
  • Brandt, T. J.
  • Bregeon, J.
  • Brigida, M.
  • Bruel, P.
  • Buehler, R.
  • Buson, S.
  • Caliandro, G. A.
  • Cameron, R. A.
  • Caraveo, P. A.
  • Carrigan, S.
  • Casandjian, J. M.
  • Charles, E.
  • Chaty, S.
  • Chekhtman, A.
  • Cheung, C. C.
  • Chiang, J.
  • Ciprini, S.
  • Claus, R.
  • Cohen-Tanugi, J.
  • Conrad, J.
  • Decesar, M. E.
  • Dermer, C. D.
  • de Palma, F.
  • Digel, S. W.
  • Do Couto E Silva, E.
  • Drell, P. S.
  • Dubois, R.
  • Dumora, D.
  • Favuzzi, C.
  • Fortin, P.
  • Frailis, M.
  • Fukazawa, Y.
  • Fusco, P.
  • Gargano, F.
  • Gasparrini, D.
  • Gehrels, N.
  • Germani, S.
  • Giglietto, N.
  • Giordano, F.
  • Glanzman, T.
  • Godfrey, G.
  • Grenier, I.
  • Grondin, M.-H.
  • Grove, J. E.
  • Guillemot, L.
  • Guiriec, S.
  • Hadasch, D.
  • Harding, A. K.
  • Hays, E.
  • Jean, P.
  • Jóhannesson, G.
  • Johnson, T. J.
  • Johnson, W. N.
  • Kamae, T.
  • Katagiri, H.
  • Kataoka, J.
  • Kerr, M.
  • Knödlseder, J.
  • Kuss, M.
  • Lande, J.
  • Latronico, L.
  • Lee, S.-H.
  • Lemoine-Goumard, M.
  • Llena Garde, M.
  • Longo, F.
  • Loparco, F.
  • Lovellette, M. N.
  • Lubrano, P.
  • Makeev, A.
  • Mazziotta, M. N.
  • Michelson, P. F.
  • Mitthumsiri, W.
  • Mizuno, T.
  • Monte, C.
  • Monzani, M. E.
  • Morselli, A.
  • Moskalenko, I. V.
  • Murgia, S.
  • Naumann-Godo, M.
  • Nolan, P. L.
  • Norris, J. P.
  • Nuss, E.
  • Ohsugi, T.
  • Omodei, N.
  • Orlando, E.
  • Ormes, J. F.
  • Pancrazi, B.
  • Parent, D.
  • Pepe, M.
  • Pesce-Rollins, M.
  • Piron, F.
  • Porter, T. A.
  • Rainò, S.
  • Rando, R.
  • Reimer, A.
  • Reimer, O.
  • Reposeur, T.
  • Ripken, J.
  • Romani, R. W.
  • Roth, M.
  • Sadrozinski, H. F.-W.
  • Saz Parkinson, P. M.
  • Sgrò, C.
  • Siskind, E. J.
  • Smith, D. A.
  • Spinelli, P.
  • Strickman, M. S.
  • Suson, D. J.
  • Takahashi, H.
  • Takahashi, T.
  • Tanaka, T.
  • Thayer, J. B.
  • Thayer, J. G.
  • Tibaldo, L.
  • Torres, D. F.
  • Tosti, G.
  • Tramacere, A.
  • Uchiyama, Y.
  • Usher, T. L.
  • Vasileiou, V.
  • Venter, C.
  • Vilchez, N.
  • Vitale, V.
  • Waite, A. P.
  • Wang, P.
  • Webb, N.
  • Winer, B. L.
  • Yang, Z.
  • Ylinen, T.
  • Ziegler, M.
subjects:
  • Astronomy And Astrophysics
  • Astronomy & Astrophysics
  • Physics
ispartof: Astronomy & Astrophysics, 12/2010, Vol.524, p.A75
description: Context. Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. The observation of this emission provides a powerful tool to assess the millisecond pulsar population of a cluster, is essential for understanding the importance of binary systems for the evolution of globular clusters, and provides complementary insights into magnetospheric emission processes. Aims. Our goal is to constrain the millisecond pulsar populations in globular clusters from analysis of gamma-ray observations. Methods. We use 546 days of continuous sky-survey observations obtained with the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope to study the gamma-ray emission towards 13 globular clusters. Results. Steady point-like high-energy gamma-ray emission has been significantly detected towards 8 globular clusters. Five of them (47 Tucanae, Omega Cen, NGC 6388, Terzan 5, and M 28) show hard spectral power indices (0.7 < Γ < 1.4) and clear evidence for an exponential cut-off in the range 1.0 - 2.6 GeV, which is the characteristic signature of magnetospheric emission from MSPs. Three of them (M 62, NGC 6440 and NGC 6652) also show hard spectral indices (1.0 < Γ < 1.7), however the presence of an exponential cut-off can not be unambiguously established. Three of them (Omega Cen, NGC 6388, NGC 6652) have no known radio or X-ray MSPs yet still exhibit MSP spectral properties. From the observed gamma-ray luminosities, we estimate the total number of MSPs that is expected to be present in these globular clusters. We show that our estimates of the MSP population correlate with the stellar encounter rate and we estimate 2600 - 4700 MSPs in Galactic globular clusters, commensurate with previous estimates. Conclusions. The observation of high-energy gamma-ray emission from globular clusters thus provides a reliable independent method to assess their millisecond pulsar populations.
language: eng
source:
identifier: ISSN: 0004-6361 ; E-ISSN: 1432-0746 ; DOI: http://dx.doi.org/10.1051/0004-6361/201014458
fulltext: no_fulltext
issn:
  • 00046361
  • 0004-6361
  • 14320746
  • 1432-0746
url: Link


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titleA population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
creatorAbdo, A. A. ; Ackermann, M. ; Ajello, M. ; Baldini, L. ; Ballet, J. ; Barbiellini, G. ; Bastieri, D. ; Bellazzini, R. ; Blandford, R. D. ; Bloom, E. D. ; Bonamente, E. ; Borgland, A. W. ; Bouvier, A. ; Brandt, T. J. ; Bregeon, J. ; Brigida, M. ; Bruel, P. ; Buehler, R. ; Buson, S. ; Caliandro, G. A. ; Cameron, R. A. ; Caraveo, P. A. ; Carrigan, S. ; Casandjian, J. M. ; Charles, E. ; Chaty, S. ; Chekhtman, A. ; Cheung, C. C. ; Chiang, J. ; Ciprini, S. ; Claus, R. ; Cohen-Tanugi, J. ; Conrad, J. ; Decesar, M. E. ; Dermer, C. D. ; de Palma, F. ; Digel, S. W. ; Do Couto E Silva, E. ; Drell, P. S. ; Dubois, R. ; Dumora, D. ; Favuzzi, C. ; Fortin, P. ; Frailis, M. ; Fukazawa, Y. ; Fusco, P. ; Gargano, F. ; Gasparrini, D. ; Gehrels, N. ; Germani, S. ; Giglietto, N. ; Giordano, F. ; Glanzman, T. ; Godfrey, G. ; Grenier, I. ; Grondin, M.-H. ; Grove, J. E. ; Guillemot, L. ; Guiriec, S. ; Hadasch, D. ; Harding, A. K. ; Hays, E. ; Jean, P. ; Jóhannesson, G. ; Johnson, T. J. ; Johnson, W. N. ; Kamae, T. ; Katagiri, H. ; Kataoka, J. ; Kerr, M. ; Knödlseder, J. ; Kuss, M. ; Lande, J. ; Latronico, L. ; Lee, S.-H. ; Lemoine-Goumard, M. ; Llena Garde, M. ; Longo, F. ; Loparco, F. ; Lovellette, M. N. ; Lubrano, P. ; Makeev, A. ; Mazziotta, M. N. ; Michelson, P. F. ; Mitthumsiri, W. ; Mizuno, T. ; Monte, C. ; Monzani, M. E. ; Morselli, A. ; Moskalenko, I. V. ; Murgia, S. ; Naumann-Godo, M. ; Nolan, P. L. ; Norris, J. P. ; Nuss, E. ; Ohsugi, T. ; Omodei, N. ; Orlando, E. ; Ormes, J. F. ; Pancrazi, B. ; Parent, D. ; Pepe, M. ; Pesce-Rollins, M. ; Piron, F. ; Porter, T. A. ; Rainò, S. ; Rando, R. ; Reimer, A. ; Reimer, O. ; Reposeur, T. ; Ripken, J. ; Romani, R. W. ; Roth, M. ; Sadrozinski, H. F.-W. ; Saz Parkinson, P. M. ; Sgrò, C. ; Siskind, E. J. ; Smith, D. A. ; Spinelli, P. ; Strickman, M. S. ; Suson, D. J. ; Takahashi, H. ; Takahashi, T. ; Tanaka, T. ; Thayer, J. B. ; Thayer, J. G. ; Tibaldo, L. ; Torres, D. F. ; Tosti, G. ; Tramacere, A. ; Uchiyama, Y. ; Usher, T. L. ; Vasileiou, V. ; Venter, C. ; Vilchez, N. ; Vitale, V. ; Waite, A. P. ; Wang, P. ; Webb, N. ; Winer, B. L. ; Yang, Z. ; Ylinen, T. ; Ziegler, M.
ispartofAstronomy & Astrophysics, 12/2010, Vol.524, p.A75
identifier
languageeng
source
descriptionContext. Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. The observation of this emission provides a powerful tool to assess the millisecond pulsar population of a cluster, is essential for understanding the importance of binary systems for the evolution of globular clusters, and provides complementary insights into magnetospheric emission processes. Aims. Our goal is to constrain the millisecond pulsar populations in globular clusters from analysis of gamma-ray observations. Methods. We use 546 days of continuous sky-survey observations obtained with the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope to study the gamma-ray emission towards 13 globular clusters. Results. Steady point-like high-energy gamma-ray emission has been significantly detected towards 8 globular clusters. Five of them (47 Tucanae, Omega Cen, NGC 6388, Terzan 5, and M 28) show hard spectral power indices (0.7 < Γ < 1.4) and clear evidence for an exponential cut-off in the range 1.0 - 2.6 GeV, which is the characteristic signature of magnetospheric emission from MSPs. Three of them (M 62, NGC 6440 and NGC 6652) also show hard spectral indices (1.0 < Γ < 1.7), however the presence of an exponential cut-off can not be unambiguously established. Three of them (Omega Cen, NGC 6388, NGC 6652) have no known radio or X-ray MSPs yet still exhibit MSP spectral properties. From the observed gamma-ray luminosities, we estimate the total number of MSPs that is expected to be present in these globular clusters. We show that our estimates of the MSP population correlate with the stellar encounter rate and we estimate 2600 - 4700 MSPs in Galactic globular clusters, commensurate with previous estimates. Conclusions. The observation of high-energy gamma-ray emission from globular clusters thus provides a reliable independent method to assess their millisecond pulsar populations.
subjectAstronomy And Astrophysics ; Astronomy & Astrophysics ; Physics;
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1Ackermann, M.
2Ajello, M.
3Baldini, L.
4Ballet, J.
5Barbiellini, G.
6Bastieri, D.
7Bellazzini, R.
8Blandford, R. D.
9Bloom, E. D.
10Bonamente, E.
11Borgland, A. W.
12Bouvier, A.
13Brandt, T. J.
14Bregeon, J.
15Brigida, M.
16Bruel, P.
17Buehler, R.
18Buson, S.
19Caliandro, G. A.
20Cameron, R. A.
21Caraveo, P. A.
22Carrigan, S.
23Casandjian, J. M.
24Charles, E.
25Chaty, S.
26Chekhtman, A.
27Cheung, C. C.
28Chiang, J.
29Ciprini, S.
30Claus, R.
31Cohen-Tanugi, J.
32Conrad, J.
33Decesar, M. E.
34Dermer, C. D.
35de Palma, F.
36Digel, S. W.
37Do Couto E Silva, E.
38Drell, P. S.
39Dubois, R.
40Dumora, D.
41Favuzzi, C.
42Fortin, P.
43Frailis, M.
44Fukazawa, Y.
45Fusco, P.
46Gargano, F.
47Gasparrini, D.
48Gehrels, N.
49Germani, S.
50Giglietto, N.
51Giordano, F.
52Glanzman, T.
53Godfrey, G.
54Grenier, I.
55Grondin, M.-H.
56Grove, J. E.
57Guillemot, L.
58Guiriec, S.
59Hadasch, D.
60Harding, A. K.
61Hays, E.
62Jean, P.
63Jóhannesson, G.
64Johnson, T. J.
65Johnson, W. N.
66Kamae, T.
67Katagiri, H.
68Kataoka, J.
69Kerr, M.
70Knödlseder, J.
71Kuss, M.
72Lande, J.
73Latronico, L.
74Lee, S.-H.
75Lemoine-Goumard, M.
76Llena Garde, M.
77Longo, F.
78Loparco, F.
79Lovellette, M. N.
80Lubrano, P.
81Makeev, A.
82Mazziotta, M. N.
83Michelson, P. F.
84Mitthumsiri, W.
85Mizuno, T.
86Monte, C.
87Monzani, M. E.
88Morselli, A.
89Moskalenko, I. V.
90Murgia, S.
91Naumann-Godo, M.
92Nolan, P. L.
93Norris, J. P.
94Nuss, E.
95Ohsugi, T.
96Omodei, N.
97Orlando, E.
98Ormes, J. F.
99Pancrazi, B.
100...
titleA population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
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titleA population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
authorAbdo, A. A. ; Ackermann, M. ; Ajello, M. ; Baldini, L. ; Ballet, J. ; Barbiellini, G. ; Bastieri, D. ; Bellazzini, R. ; Blandford, R. D. ; Bloom, E. D. ; Bonamente, E. ; Borgland, A. W. ; Bouvier, A. ; Brandt, T. J. ; Bregeon, J. ; Brigida, M. ; Bruel, P. ; Buehler, R. ; Buson, S. ; Caliandro, G. A. ; Cameron, R. A. ; Caraveo, P. A. ; Carrigan, S. ; Casandjian, J. M. ; Charles, E. ; Chaty, S. ; Chekhtman, A. ; Cheung, C. C. ; Chiang, J. ; Ciprini, S. ; Claus, R. ; Cohen-Tanugi, J. ; Conrad, J. ; Decesar, M. E. ; Dermer, C. D. ; de Palma, F. ; Digel, S. W. ; Do Couto E Silva, E. ; Drell, P. S. ; Dubois, R. ; Dumora, D. ; Favuzzi, C. ; Fortin, P. ; Frailis, M. ; Fukazawa, Y. ; Fusco, P. ; Gargano, F. ; Gasparrini, D. ; Gehrels, N. ; Germani, S. ; Giglietto, N. ; Giordano, F. ; Glanzman, T. ; Godfrey, G. ; Grenier, I. ; Grondin, M.-H. ; Grove, J. E. ; Guillemot, L. ; Guiriec, S. ; Hadasch, D. ; Harding, A. K. ; Hays, E. ; Jean, P. ; Jóhannesson, G. ; Johnson, T. J. ; Johnson, W. N. ; Kamae, T. ; Katagiri, H. ; Kataoka, J. ; Kerr, M. ; Knödlseder, J. ; Kuss, M. ; Lande, J. ; Latronico, L. ; Lee, S.-H. ; Lemoine-Goumard, M. ; Llena Garde, M. ; Longo, F. ; Loparco, F. ; Lovellette, M. N. ; Lubrano, P. ; Makeev, A. ; Mazziotta, M. N. ; Michelson, P. F. ; Mitthumsiri, W. ; Mizuno, T. ; Monte, C. ; Monzani, M. E. ; Morselli, A. ; Moskalenko, I. V. ; Murgia, S. ; Naumann-Godo, M. ; Nolan, P. L. ; Norris, J. P. ; Nuss, E. ; Ohsugi, T. ; Omodei, N. ; Orlando, E. ; Ormes, J. F. ; Pancrazi, B. ; Parent, D. ; Pepe, M. ; Pesce-Rollins, M. ; Piron, F. ; Porter, T. A. ; Rainò, S. ; Rando, R. ; Reimer, A. ; Reimer, O. ; Reposeur, T. ; Ripken, J. ; Romani, R. W. ; Roth, M. ; Sadrozinski, H. F.-W. ; Saz Parkinson, P. M. ; Sgrò, C. ; Siskind, E. J. ; Smith, D. A. ; Spinelli, P. ; Strickman, M. S. ; Suson, D. J. ; Takahashi, H. ; Takahashi, T. ; Tanaka, T. ; Thayer, J. B. ; Thayer, J. G. ; Tibaldo, L. ; Torres, D. F. ; Tosti, G. ; Tramacere, A. ; Uchiyama, Y. ; Usher, T. L. ; Vasileiou, V. ; Venter, C. ; Vilchez, N. ; Vitale, V. ; Waite, A. P. ; Wang, P. ; Webb, N. ; Winer, B. L. ; Yang, Z. ; Ylinen, T. ; Ziegler, M.
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0Abdo, A. A.
1Ackermann, M.
2Ajello, M.
3Baldini, L.
4Ballet, J.
5Barbiellini, G.
6Bastieri, D.
7Bellazzini, R.
8Blandford, R. D.
9Bloom, E. D.
10Bonamente, E.
11Borgland, A. W.
12Bouvier, A.
13Brandt, T. J.
14Bregeon, J.
15Brigida, M.
16Bruel, P.
17Buehler, R.
18Buson, S.
19Caliandro, G. A.
20Cameron, R. A.
21Caraveo, P. A.
22Carrigan, S.
23Casandjian, J. M.
24Charles, E.
25Chaty, S.
26Chekhtman, A.
27Cheung, C. C.
28Chiang, J.
29Ciprini, S.
30Claus, R.
31Cohen-Tanugi, J.
32Conrad, J.
33Decesar, M. E.
34Dermer, C. D.
35de Palma, F.
36Digel, S. W.
37Do Couto E Silva, E.
38Drell, P. S.
39Dubois, R.
40Dumora, D.
41Favuzzi, C.
42Fortin, P.
43Frailis, M.
44Fukazawa, Y.
45Fusco, P.
46Gargano, F.
47Gasparrini, D.
48Gehrels, N.
49Germani, S.
50Giglietto, N.
51Giordano, F.
52Glanzman, T.
53Godfrey, G.
54Grenier, I.
55Grondin, M.-H.
56Grove, J. E.
57Guillemot, L.
58Guiriec, S.
59Hadasch, D.
60Harding, A. K.
61Hays, E.
62Jean, P.
63Jóhannesson, G.
64Johnson, T. J.
65Johnson, W. N.
66Kamae, T.
67Katagiri, H.
68Kataoka, J.
69Kerr, M.
70Knödlseder, J.
71Kuss, M.
72Lande, J.
73Latronico, L.
74Lee, S.-H.
75Lemoine-Goumard, M.
76Llena Garde, M.
77Longo, F.
78Loparco, F.
79Lovellette, M. N.
80Lubrano, P.
81Makeev, A.
82Mazziotta, M. N.
83Michelson, P. F.
84Mitthumsiri, W.
85Mizuno, T.
86Monte, C.
87Monzani, M. E.
88Morselli, A.
89Moskalenko, I. V.
90Murgia, S.
91Naumann-Godo, M.
92Nolan, P. L.
93Norris, J. P.
94Nuss, E.
95Ohsugi, T.
96Omodei, N.
97Orlando, E.
98Ormes, J. F.
99Pancrazi, B.
100...
jtitleAstronomy & Astrophysics
toplevelpeer_reviewed
delivery
delcategoryRemote Search Resource
fulltextno_fulltext
addata
aulast
0Abdo
1Ackermann
2Ajello
3Baldini
4Ballet
5Barbiellini
6Bastieri
7Bellazzini
8Blandford
9Bloom
10Bonamente
11Borgland
12Bouvier
13Brandt
14Bregeon
15Brigida
16Bruel
17Buehler
18Buson
19Caliandro
20Cameron
21Caraveo
22Carrigan
23Casandjian
24Charles
25Chaty
26Chekhtman
27Cheung
28Chiang
29Ciprini
30Claus
31Cohen-Tanugi
32Conrad
33Decesar
34Dermer
35de Palma
36Digel
37Do Couto E Silva
38Drell
39Dubois
40Dumora
41Favuzzi
42Fortin
43Frailis
44Fukazawa
45Fusco
46Gargano
47Gasparrini
48Gehrels
49Germani
50Giglietto
51Giordano
52Glanzman
53Godfrey
54Grenier
55Grondin
56Grove
57Guillemot
58Guiriec
59Hadasch
60Harding
61Hays
62Jean
63Jóhannesson
64Johnson
65Kamae
66Katagiri
67Kataoka
68Kerr
69Knödlseder
70Kuss
71Lande
72Latronico
73Lee
74Lemoine-Goumard
75Llena Garde
76Longo
77Loparco
78Lovellette
79Lubrano
80Makeev
81Mazziotta
82Michelson
83Mitthumsiri
84Mizuno
85Monte
86Monzani
87Morselli
88Moskalenko
89Murgia
90Naumann-Godo
91Nolan
92Norris
93Nuss
94Ohsugi
95Omodei
96Orlando
97Ormes
98Pancrazi
99Parent
100...
aufirst
0A. A.
1M.
2L.
3J.
4G.
5D.
6R.
7R. D.
8E. D.
9E.
10A. W.
11A.
12T. J.
13P.
14S.
15G. A.
16R. A.
17P. A.
18J. M.
19C. C.
20M. E.
21C. D.
22F.
23S. W.
24P. S.
25C.
26Y.
27N.
28T.
29I.
30M.-H.
31J. E.
32A. K.
33W. N.
34H.
35S.-H.
36M. N.
37P. F.
38W.
39I. V.
40P. L.
41J. P.
42J. F.
43B.
44T. A.
45O.
46R. W.
47H. F.-W.
48P. M.
49E. J.
50D. A.
51M. S.
52D. J.
53J. B.
54J. G.
55D. F.
56T. L.
57V.
58A. P.
59B. L.
60Z.
au
0Abdo, A. A.
1Ackermann, M.
2Ajello, M.
3Baldini, L.
4Ballet, J.
5Barbiellini, G.
6Bastieri, D.
7Bellazzini, R.
8Blandford, R. D.
9Bloom, E. D.
10Bonamente, E.
11Borgland, A. W.
12Bouvier, A.
13Brandt, T. J.
14Bregeon, J.
15Brigida, M.
16Bruel, P.
17Buehler, R.
18Buson, S.
19Caliandro, G. A.
20Cameron, R. A.
21Caraveo, P. A.
22Carrigan, S.
23Casandjian, J. M.
24Charles, E.
25Chaty, S.
26Chekhtman, A.
27Cheung, C. C.
28Chiang, J.
29Ciprini, S.
30Claus, R.
31Cohen-Tanugi, J.
32Conrad, J.
33Decesar, M. E.
34Dermer, C. D.
35de Palma, F.
36Digel, S. W.
37Do Couto E Silva, E.
38Drell, P. S.
39Dubois, R.
40Dumora, D.
41Favuzzi, C.
42Fortin, P.
43Frailis, M.
44Fukazawa, Y.
45Fusco, P.
46Gargano, F.
47Gasparrini, D.
48Gehrels, N.
49Germani, S.
50Giglietto, N.
51Giordano, F.
52Glanzman, T.
53Godfrey, G.
54Grenier, I.
55Grondin, M.-H.
56Grove, J. E.
57Guillemot, L.
58Guiriec, S.
59Hadasch, D.
60Harding, A. K.
61Hays, E.
62Jean, P.
63Jóhannesson, G.
64Johnson, T. J.
65Johnson, W. N.
66Kamae, T.
67Katagiri, H.
68Kataoka, J.
69Kerr, M.
70Knödlseder, J.
71Kuss, M.
72Lande, J.
73Latronico, L.
74Lee, S.-H.
75Lemoine-Goumard, M.
76Llena Garde, M.
77Longo, F.
78Loparco, F.
79Lovellette, M. N.
80Lubrano, P.
81Makeev, A.
82Mazziotta, M. N.
83Michelson, P. F.
84Mitthumsiri, W.
85Mizuno, T.
86Monte, C.
87Monzani, M. E.
88Morselli, A.
89Moskalenko, I. V.
90Murgia, S.
91Naumann-Godo, M.
92Nolan, P. L.
93Norris, J. P.
94Nuss, E.
95Ohsugi, T.
96Omodei, N.
97Orlando, E.
98Ormes, J. F.
99Pancrazi, B.
100...
atitleA population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope
jtitleAstronomy & Astrophysics
stitleA&A
risdate201012
adddate
0201012
12010
220102010111224
volume524
spageA75
issn0004-6361
eissn1432-0746
formatjournal
genrearticle
ristypeJOUR
doi10.1051/0004-6361/201014458
lad012
citing
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1$$t=2$$K1=2009$$K4=325$$K6=848$$K7=science$$K15=abdo$$K16=abdo$$K18=abdo
2$$t=2$$K1=2009$$K4=325$$K6=845$$K7=science$$K15=abdo$$K16=abdo$$K18=abdo
3$$t=2$$K1=2009$$K4=325$$K6=840$$K7=science$$K15=abdo$$K16=abdo$$K18=abdo
4$$t=2$$K1=2010$$K4=187$$K6=460$$K7=apjs$$K15=abdo$$K16=abdo$$K18=abdo
5$$t=2$$K1=2010$$K4=188$$K6=405$$K7=apjs$$K15=abdo$$K16=abdo$$K18=abdo
6$$t=2$$K1=2010$$K4=328$$K6=725$$K7=science$$K15=abdo$$K16=abdo$$K18=abdo
7$$t=2$$K1=2010$$K4=715$$K6=429$$K7=apj$$K15=abdo$$K16=abdo$$K18=abdo
8$$t=2$$K1=1992$$K4=300$$K6=728$$K7=nature$$K15=alpar$$K16=alpar$$K18=alpar
9$$t=2$$K1=2009$$K4=697$$K6=1071$$K7=apj$$K15=atwood$$K16=atwood$$K18=atwood
10$$t=2$$K1=2006$$K4=131$$K6=2551$$K7=apj$$K15=beccari$$K16=beccari$$K18=beccari
11$$t=2$$K1=2006$$K4=646$$K6=1104$$K7=apj$$K15=bogdanov$$K16=bogdanov$$K18=bogdanov
12$$t=2$$K1=2008$$K4=686$$K6=L87$$K7=apj$$K15=bono$$K16=bono$$K18=bono
13$$t=2$$K1=2005$$K4=328$$K6=147$$K7=aspc$$K15=camilo$$K16=camilo$$K18=camilo
14$$t=2$$K1=2000$$K4=120$$K6=3102$$K7=aj$$K15=chaboyer$$K16=chaboyer$$K18=chaboyer
15$$t=2$$K1=1975$$K4=199$$K6=L143$$K7=apj$$K15=clark$$K16=clark$$K18=clark
16$$t=2$$K1=2002$$K4=570$$K6=89$$K7=apj$$K15=d’amico$$K16=d’amico$$K18=d’amico
17$$t=2$$K1=1992$$K4=396$$K6=587$$K7=apj$$K15=distefano$$K16=stefanodi$$K18=stefano
18$$t=2$$K1=1993$$K4=50$$K6=373$$K7=asp conf ser$$K15=djorgovski$$K16=djorgovski$$K18=djorgovski
19$$t=2$$K1=2008$$K4=675$$K6=670$$K7=apj$$K15=freire$$K16=freire$$K18=freire
20$$t=2$$K1=1990$$K4=365$$K6=L63$$K7=apj$$K15=fruchter$$K16=fruchter$$K18=fruchter
21$$t=2$$K1=2000$$K4=536$$K6=865$$K7=apj$$K15=fruchter$$K16=fruchter$$K18=fruchter
22$$t=2$$K1=2003$$K4=403$$K6=11$$K7= a$$K15=gendre$$K16=gendre$$K18=gendre
23$$t=2$$K1=2003$$K4=400$$K6=521$$K7= a$$K15=gendre$$K16=gendre$$K18=gendre
24$$t=2$$K1=2001$$K4=292$$K6=2290$$K7=science$$K15=grindlay$$K16=grindlay$$K18=grindlay
25$$t=2$$K1=2009$$K4=697$$K6=224$$K7=apj$$K15=haggard$$K16=haggard$$K18=haggard
26$$t=2$$K1=1996$$K4=112$$K6=1487$$K7=aj$$K15=harris$$K16=harris$$K18=harris
27$$t=2$$K1=2005$$K4=625$$K6=796$$K7=apj$$K15=heinke$$K16=heinke$$K18=heinke
28$$t=2$$K1=2007$$K4=670$$K6=363$$K7=apj$$K15=hessels$$K16=hessels$$K18=hessels
29$$t=2$$K1=2009$$K4=180$$K6=225$$K7=apjs$$K15=hinshaw$$K16=hinshaw$$K18=hinshaw
30$$t=2$$K1=1992$$K4=104$$K6=981$$K7=pasp$$K15=hut$$K16=hut$$K18=hut
31$$t=2$$K1=2008$$K4=386$$K6=553$$K7=mnras$$K15=ivanova$$K16=ivanova$$K18=ivanova
32$$t=2$$K1=2010$$K4=712$$K6=36$$K7=apj$$K15=kong$$K16=kong$$K18=kong
33$$t=2$$K1=2006$$K4=653$$K6=580$$K7=apj$$K15=knight$$K16=knight$$K18=knight
34$$t=2$$K1=1990$$K4=356$$K6=174$$K7=apj$$K15=kulkarni$$K16=kulkarni$$K18=kulkarni
35$$t=2$$K1=2006$$K4=132$$K6=2171$$K7=aj$$K15=lee$$K16=lee$$K18=lee
36$$t=2$$K1=2004$$K4=348$$K6=1409$$K7=mnras$$K15=mcconnell$$K16=mcconnell$$K18=mcconnell
37$$t=2$$K1=2006$$K4=166$$K6=249$$K7=apjs$$K15=mclaughlin$$K16=mclaughlin$$K18=mclaughlin
38$$t=2$$K1=2009$$K4=493$$K6=539$$K7= a$$K15=moretti$$K16=moretti$$K18=moretti
39$$t=2$$K1=2008$$K4=478$$K6=763$$K7= a$$K15=nucita$$K16=nucita$$K18=nucita
40$$t=2$$K1=1994$$K4=108$$K6=653$$K7= as$$K15=ortolani$$K16=ortolani$$K18=ortolani
41$$t=2$$K1=2007$$K4=470$$K6=1043$$K7= a$$K15=ortolani$$K16=ortolani$$K18=ortolani
42$$t=2$$K1=2009$$K4=695$$K6=115$$K7=apj$$K15=pellizzoni$$K16=pellizzoni$$K18=pellizzoni
43$$t=2$$K1=2008$$K4=983$$K6=415$$K7=aipc$$K15=ransom$$K16=ransom$$K18=ransom
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45$$t=2$$K1=1991$$K4=102$$K6=152$$K7=aj$$K15=rees$$K16=rees$$K18=rees
46$$t=2$$K1=2007$$K4=133$$K6=1658$$K7=aj$$K15=sarajedini$$K16=sarajedini$$K18=sarajedini
47$$t=2$$K1=2006$$K4=445$$K6=513$$K7= a$$K15=vandeven$$K16=vandeven$$K18=vanven
48$$t=2$$K1=2006$$K4=641$$K6=852$$K7=apj$$K15=vandenbosch$$K16=vandenbosch$$K18=vandenbosch
49$$t=2$$K1=1991$$K4=241$$K6=L37$$K7= a$$K15=wijers$$K16=wijers$$K18=wijers
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
date2010-12