SEARCH FOR VERY HIGH ENERGY GAMMA-RAY EMISSION FROM PULSAR-PULSAR WIND NEBULA SYSTEMS WITH THE MAGIC TELESCOPE
H. Anderhub
(1)
,
L.A. Antonelli
(2)
,
P. Antoranz
(3)
,
M. Backes
(4)
,
C. Baixeras
(5)
,
S. Balestra
(3)
,
J.A. Barrio
(3)
,
D. Bastieri
(6)
,
J.Becerra González
,
J.K. Becker
(4)
,
W. Bednarek
(7)
,
Al K. Berger
(7)
,
E. Bernardini
,
A. Biland
(1)
,
R.K. Bock
,
G. Bonnoli
,
P. Bordas
,
D. Borla Tridon
,
V. Bosch-Ramon
,
D. Bose
(3)
,
I. Braun
(1)
,
T. Bretz
,
D. Britzger
,
M. Camara
(3)
,
E. Carmona
,
A. Carosi
,
P. Colin
,
S. Commichau
(1)
,
J.L. Contreras
(3)
,
Ismaël Cognard
(8)
1
ETH Zürich -
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich]
2 INAF - Istituto Nazionale di Astrofisica
3 UCM - Universidad Complutense de Madrid = Complutense University of Madrid [Madrid]
4 TU - Technische Universität Dortmund [Dortmund]
5 UAB - Universitat Autònoma de Barcelona
6 Unipd - Università degli Studi di Padova = University of Padua
7 University of Lódź
8 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
2 INAF - Istituto Nazionale di Astrofisica
3 UCM - Universidad Complutense de Madrid = Complutense University of Madrid [Madrid]
4 TU - Technische Universität Dortmund [Dortmund]
5 UAB - Universitat Autònoma de Barcelona
6 Unipd - Università degli Studi di Padova = University of Padua
7 University of Lódź
8 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
M. Backes
- Function : Author
- PersonId : 760162
- ORCID : 0000-0002-9326-6400
J.Becerra González
- Function : Author
E. Bernardini
- Function : Author
- PersonId : 758076
- ORCID : 0000-0003-3108-1141
A. Biland
- Function : Author
- PersonId : 755137
- ORCID : 0000-0002-1288-833X
R.K. Bock
- Function : Author
G. Bonnoli
- Function : Author
- PersonId : 760165
- ORCID : 0000-0003-2464-9077
P. Bordas
- Function : Author
D. Borla Tridon
- Function : Author
V. Bosch-Ramon
- Function : Author
T. Bretz
- Function : Author
D. Britzger
- Function : Author
E. Carmona
- Function : Author
A. Carosi
- Function : Author
P. Colin
- Function : Author
Ismaël Cognard
- Function : Author
- PersonId : 749308
- IdHAL : ismael-cognard
- ORCID : 0000-0002-1775-9692
- IdRef : 113645031
Abstract
The MAGIC collaboration has searched for high-energy gamma-ray emission of some of the most promising pulsar candidates above an energy threshold of 50 GeV, an energy not reachable up to now by other ground-based instruments. Neither pulsed nor steady gamma-ray emission has been observed at energies of 100 GeV from the classical radio pulsars PSR J0205+6449 and PSR J2229+6114 (and their nebulae 3C58 and Boomerang, respectively) and the millisecond pulsar PSR J0218+4232. Here, we present the flux upper limits for these sources and discuss their implications in the context of current model predictions.