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MAGIC search for VHE $\gamma$-ray emission from AE Aquarii in a multiwavelength context

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arxiv 1407.3707 v1 pith:FMXW2F2S submitted 2014-07-14 astro-ph.HE

J. Aleksić (1) , S. Ansoldi (2) , L. A. Antonelli (3) , P. Antoranz (4) , A. Babic (5) , P. Bangale (6) , J. A. Barrio (7) , J. Becerra González (8
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25) W. Bednarek (9) E. Bernardini (10) B. Biasuzzi (2) A. Biland (11) O. Blanch (1) S. Bonnefoy (7) G. Bonnoli (3) F. Borracci (6) T. Bretz (12 26) E. Carmona (13) A. Carosi (3) P. Colin (6) E. Colombo (8) J. L. Contreras (7) J. Cortina (1) S. Covino (3) P. Da Vela (4) F. Dazzi (6) A. De Angelis (2) G. De Caneva (10) B. De Lotto (2) E. de Oña Wilhelmi (14) C. Delgado Mendez (13) M. Doert (15) D. Dominis Prester (5) D. Dorner (12) M. Doro (16) S. Einecke (15) D. Eisenacher (12) D. Elsaesser (12) M. V. Fonseca (7) L. Font (17) K. Frantzen (15) C. Fruck (6) D. Galindo (18) R. J. García López (8) M. Garczarczyk (10) D. Garrido Terrats (17) M. Gaug (17) N. Godinović (5) A. González Muñoz (1) S. R. Gozzini (10) D. Hadasch (14 27) Y. Hanabata (19) M. Hayashida (19) J. Herrera (8) D. Hildebrand (11) J. Hose (6) D. Hrupec (5) W. Idec (9) V. Kadenius (20) H. Kellermann (6) K. Kodani (19) Y. Konno (19) J. Krause (6) H. Kubo (19) J. Kushida (19) A. La Barbera (3) D. Lelas (5) N. Lewandowska (12) E. Lindfors (20 28) S. Lombardi (3) M. López (7) R. López-Coto (1) A. López-Oramas (1) E. Lorenz (6) I. Lozano (7) M. Makariev (21) K. Mallot (10) G. Maneva (21) N. Mankuzhiyil (2 29) K. Mannheim (12) L. Maraschi (3) B. Marcote (18) M. Mariotti (16) M. Martínez (1) D. Mazin (6) U. Menzel (6) J. M. Miranda (4) R. Mirzoyan (6) A. Moralejo (1) P. Munar-Adrover (18) D. Nakajima (19) A. Niedzwiecki (9) K. Nilsson (20 K. Nishijima (19) K. Noda (6) N. Nowak (6) R. Orito (19) A. Overkemping (15) S. Paiano (16) M. Palatiello (2) D. Paneque (6) R. Paoletti (4) J. M. Paredes (18) X. Paredes-Fortuny (18) M. Persic (2 30) P. G. Prada Moroni (22) E. Prandini (11) S. Preziuso (4) I. Puljak (5) R. Reinthal (20) W. Rhode (15) M. Ribó (18) J. Rico (1) J. Rodriguez Garcia (6) S. Rügamer (12) A. Saggion (16) T. Saito (19) K. Saito (19) K. Satalecka (7) V. Scalzotto (16) V. Scapin (7) C. Schultz (16) T. Schweizer (6) A. Sillanpää (20) J. Sitarek (1) I. Snidaric (5) D. Sobczynska (9) F. Spanier (12) V. Stamatescu (1 31) A. Stamerra (3) T. Steinbring (12) J. Storz (12) M. Strzys (6) L. Takalo (20) H. Takami (19) F. Tavecchio (3) P. Temnikov (21) T. Terzić (5) D. Tescaro (8) M. Teshima (6) J. Thaele (15) O. Tibolla (12) D. F. Torres (23) T. Toyama (6) A. Treves (24) M. Uellenbeck (15) P. Vogler (11) R. M. Wagner (6 32) R. Zanin (18) M. Bogosavljevic (33) Z. Ioannou (34) C.W. Mauche (35) E.V. Palaiologou (36) M.A. Pérez-Torres (37) T. Tuominen (20) ((1) IFAE Campus UAB E-08193 Bellaterra Spain (2) Università di Udine INFN Trieste I-33100 Udine Italy (3) INAF National Institute for Astrophysics I-00136 Rome (4) Università di Siena INFN Pisa I-53100 Siena (5) Croatian MAGIC Consortium Rudjer Boskovic Institute University of Rijeka University of Split HR-10000 Zagreb Croatia (6) Max-Planck-Institut für Physik D-80805 München Germany (7) Universidad Complutense E-28040 Madrid (8) Inst. de Astrofísica de Canarias E-38200 La Laguna Tenerife (9) University of Lódź PL-90236 Lodz Poland (10) Deutsches Elektronen-Synchrotron (DESY) D-15738 Zeuthen (11) ETH Zurich CH-8093 Zurich Switzerland (12) Universität Würzburg D-97074 Würzburg (13) Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (14) Institute of Space Sciences E-08193 Barcelona (15) Technische Universität Dortmund D-44221 Dortmund (16) Università di Padova INFN I-35131 Padova (17) Unitat de Física de les Radiacions Departament de Física CERES-IEEC Universitat Autònoma de Barcelona (18) Universitat de Barcelona ICC IEEC-UB E-08028 Barcelona (19) Japanese MAGIC Consortium Division of Physics Astronomy Kyoto University Japan (20) Finnish MAGIC Consortium Tuorla Observatory University of Turku Department of Physics University of Oulu Finland (21) Inst. for Nucl. Research Nucl. Energy BG-1784 Sofia Bulgaria (22) Università di Pisa I-56126 Pisa (23) ICREA Institute of Space Sciences (24) Università dell'Insubria INFN Milano Bicocca Como I-22100 Como (25) now at: NASA Goddard Space Flight Center Greenbelt MD 20771 USA Department of Astronomy University of Maryland College Park MD 20742 (26) now at Ecole polytechnique fédérale de Lausanne (EPFL) Lausanne (27) now at: Institut für Astro- und Teilchenphysik Leopold-Franzens-Universität Innsbruck A-6020 Innsbruck Austria (28) now at Finnish Centre for Astronomy with ESO (FINCA) Turku (29) now at Astrophysics Science Division Bhabha Atomic Research Centre Mumbai 400085 India (30) also at INAF-Trieste (31) now at School of Chemistry Physics University of Adelaide Adelaide 5005 Australia (32) now at Stockholm University Oskar Klein Centre for Cosmoparticle Physics SE-106 91 Stockholm Sweden (33) Astronomical Observatory Belgrade 11060 Belgrade Serbia (34) Physics Department College of Science Sultan Qaboos University P.O. Box 36 PC-123 Muscat Oman (35) Lawrence Livermore National Laboratory 7000 East Ave. Livermore CA 95125 (36) Physics Department University of Crete P.O. Box 2208 GR-71003 Heraklion Greece (37) Inst. de Astrofísica de Andalucía (CSIC) E-18080 Granada Spain)
This is my paper · ORCID
classification astro-ph.HE
keywords emissionuppergamma-raydifferentlimitspulsedsourceabove
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

It has been claimed that the nova-like cataclysmic variable (CV) AE Aquarii (AE Aqr) is a very-high-energy (VHE, $E>$100 GeV) source both on observational and theoretical grounds. We aim to search for VHE gamma-ray emission from AE Aqr during different states of the source at several wavelengths to confirm or rule out previous claims of detection of gamma-ray emission from this object. We report on observations of AE Aqr performed by MAGIC. The source was observed during 12 hours as part of a multiwavelength campaign carried out between May and June 2012 covering the optical, X-ray, and gamma-ray ranges. Besides MAGIC, the other facilities involved were the KVA, Skinakas, and Vidojevica telescopes in the optical and Swift in X-rays. We calculated integral upper limits coincident with different states of the source in the optical. We computed upper limits to the pulsed emission limiting the signal region to 30% of the phaseogram and we also searched for pulsed emission at different frequencies applying the Rayleigh test. AE Aqr was not detected at VHE energies during the multiwavelength campaign. We establish integral upper limits at the 95\% confidence level for the steady emission assuming the differential flux proportional to a power-law function d\phi/dE \propto E^{-Gamma}, with a Crab-like photon spectral index of Gamma=2.6. The upper limit above 200 GeV is 6.4\times10^{-12} cm^{-2}s^{-1} and above 1 TeV is 7.4\times10^{-13} cm^{-2}s^{-1}. We obtained an upper limit for the pulsed emission of 2.6\times10^{-12} cm^{-2}s^{-1} for energies above 200 GeV. Applying the Rayleigh test for pulsed emission at different frequencies we did not find any significant signal. Our results indicate that AE Aqr is not a VHE gamma-ray emitter at the level of emission previously claimed. We have established the most constraining upper limits for the VHE gamma-ray emission of AE Aqr.

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