Crab pulsar 50-400GeV light curve Virtual Observatory Resource

Authors

1. Aleksic J.
2. Saito T.Y.
3. Zanin R.
4. Bonnefoy S.
5. Hirotani K.,Ansoldi S.
6. Antonelli L.A.
7. Antoranz P.
8. Babic A.
9. Bangale P.,Barres de Almeida U.
10. Barrio J.A.
11. Becerra Gonzalez J.
12. Bednarek W.,Bernardini E.
13. Biasuzzi B.
14. Biland A.
15. Blanch O.
16. Bonnoli G.
17. Borracci F.,Bretz T.
18. Carmona E.
19. Carosi A.
20. Colin P.
21. Colombo E.
22. Contreras J.L.,Cortina J.
23. Covino S.
24. Da Vela P.
25. Dazzi F.
26. De Angelis A.
27. De Caneva G.,De Lotto B.
28. Delgado Mendez C.
29. Doert M.
30. Dominis Prester D.
31. Dorner D.,Doro M.
32. Einecke S.
33. Eisenacher D.
34. Elsaesser D.
35. Farina E.
36. Ferenc D.,Fidalgo D.
37. Fonseca M.V.
38. Font L.
39. Frantzen K.
40. Fruck C.
41. Garcia Lopez R.J.,Garczarczyk M.
42. Garrido Terrats D.
43. Gaug M.
44. Godinovic N.,Gonzalez Munoz A.
45. Gozzini S.R.
46. Hadasch D.
47. Hayashida M.
48. Herrera J.,Herrero A.
49. Hildebrand D.
50. Hose J.
51. Hrupec D.
52. Idec W.
53. Kadenius V.,Kellermann H.
54. Kodani K.
55. Konno Y.
56. Krause J.
57. Kubo H.
58. Kushida J.,La Barbera A.
59. Lelas D.
60. Lewandowska N.
61. Lindfors E.
62. Lombardi S.
63. Lopez M.,Lopez-Coto R.
64. Lopez-Oramas A.
65. Lorenz E.
66. Lozano I.
67. Makariev M.,Mallot K.
68. Maneva G.
69. Mankuzhiyil N.
70. Mannheim K.
71. Maraschi L.
72. Marcote B.,Mariotti M.
73. Martinez M.
74. Mazin D.
75. Menzel U.
76. Miranda J.M.
77. Mirzoyan R.,Moralejo A.
78. Munar-Adrover P.
79. Nakajima D.
80. Niedzwiecki A.
81. Nilsson K.,Nishijima K.
82. Noda K.
83. Nowak N.
84. Orito R.
85. Overkemping A.
86. Paiano S.,Palatiello M.
87. Paneque D.
88. Paoletti R.
89. Paredes J.M.
90. Paredes-Fortuny X.,Partini S.
91. Persic M.
92. Prada Moroni P.G.
93. Prandini E.
94. Preziuso S.,Puljak I.
95. Reinthal R.
96. Rhode W.
97. Ribo M.
98. Rico J.
99. Rodriguez Garcia J.,Rugamer S.
100. Saggion A.
101. Saito K.
102. Satalecka K.
103. Scalzotto V.
104. Scapin V.,Schultz C.
105. Schweizer T.
106. Shore S.N.
107. Sillanpaa A.
108. Sitarek J.
109. Snidaric I.,Sobczynska D.
110. Spanier F.
111. Stamatescu V.
112. Stamerra A.
113. Steinbring T.,Storz J.
114. Strzys M.
115. Sun S.
116. Suric T.
117. Takalo L.
118. Takami H.
119. Tavecchio F.,Temnikov P.
120. Terzic T.
121. Tescaro D.
122. Teshima M.
123. Thaele J.
124. Tibolla O.,Torres D.F.
125. Toyama T.
126. Treves A.
127. Uellenbeck M.
128. Vogler P.
129. Wagner R.M.

Published by

CDS

Abstract

The Crab pulsar is the only astronomical pulsed source detected at very high energy (VHE, E>100GeV) gamma rays. The emission mechanism of VHE pulsation is not yet fully understood, although several theoretical models have been proposed. In order to test new models, we measured the light curve and the spectra of the Crab pulsar with high precision by means of deep observations. We analyzed 135h of selected MAGIC data taken between 2009 and 2013 in stereoscopic mode. In order to discuss the spectral shape in connection with lower energies, 5.5 years of Fermi-LAT data were also analyzed

Keywords

1. gamma-ray-astronomy
2. pulsars

Bibliographic source Bibcode

2014A&A...565L..12A

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/565/L12

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/565/L12

Document Object Identifer DOI

doi:10.26093/cds/vizier.35659012

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/565/L12
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/565/L12
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/565/L12

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