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Search for Very-High-Energy Gamma Rays from the z = 0.896 Quasar 4C +55.17 with the MAGIC telescopes

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arxiv 1402.0291 v1 pith:6PNAXGLC submitted 2014-02-03 astro-ph.HE astro-ph.GA

MAGIC Collaboration: J. Aleksić (1) , S. Ansoldi (2) , L. A. Antonelli (3) , P. Antoranz (4) , A. Babic (5) , P. Bangale (6) , U. Barres de Almeida (6) , J. A. Barrio (7)
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J. Becerra González (8) W. Bednarek (9) K. Berger (8) E. Bernardini (10) A. Biland (11) O. Blanch (1) R. K. Bock (6) S. Bonnefoy (7) G. Bonnoli (3) F. Borracci (6) T. Bretz (12 25) E. Carmona (13) A. Carosi (3) D. Carreto Fidalgo (12) P. Colin (6) E. Colombo (8) J. L. Contreras (7) J. Cortina (1) S. Covino (3) P. Da Vela (4) F. Dazzi (14) A. De Angelis (2) G. De Caneva (10) B. De Lotto (2) C. Delgado Mendez (13) M. Doert (15) A. Domínguez (16 26) D. Dominis Prester (5) D. Dorner (12) M. Doro (14) S. Einecke (15) D. Eisenacher (12) D. Elsaesser (12) E. Farina (17) D. Ferenc (5) M. V. Fonseca (7) L. Font (18) K. Frantzen (15) C. Fruck (6) R. J. García López (8) M. Garczarczyk (10) D. Garrido Terrats (18) M. Gaug (18) G. Giavitto (1) N. Godinović (5) A. González Mu\ noz (1) S. R. Gozzini (10) D. Hadasch (19) M. Hayashida (20) A. Herrero (8) D. Hildebrand (11) J. Hose (6) D. Hrupec (5) W. Idec (9) V. Kadenius (21) H. Kellermann (6) M. L. Knoetig (11) K. Kodani (20) Y. Konno (20) J. Krause (6) H. Kubo (20) J. Kushida (20) A. La Barbera (3) D. Lelas (5) N. Lewandowska (12) E. Lindfors (21 27) S. Lombardi (3) M. López (7) R. López-Coto (1) A. López-Oramas (1) E. Lorenz (6) I. Lozano (7) M. Makariev (22) K. Mallot (10) G. Maneva (22) N. Mankuzhiyil (2) K. Mannheim (12) L. Maraschi (3) B. Marcote (23) M. Mariotti (14) M. Martínez (1) D. Mazin (6) U. Menzel (6) M. Meucci (4) J. M. Miranda (4) R. Mirzoyan (6) A. Moralejo (1) P. Munar-Adrover (23) D. Nakajima (20) A. Niedzwiecki (9) K. Nilsson (21 K. Nishijima (20) N. Nowak (6) R. Orito (20) A. Overkemping (15) S. Paiano (14) M. Palatiello (2) D. Paneque (6) R. Paoletti (4) J. M. Paredes (23) X. Paredes-Fortuny (23) S. Partini (4) M. Persic (2 28) F. Prada (16 29) P. G. Prada Moroni (24) E. Prandini (14) S. Preziuso (4) I. Puljak (5) R. Reinthal (21) W. Rhode (15) M. Ribó (23) J. Rico (1) J. Rodriguez Garcia (6) S. Rügamer (12) A. Saggion (14) T. Saito (20) K. Saito (20) M. Salvati (3) K. Satalecka (7) V. Scalzotto (14) V. Scapin (7) C. Schultz (14) T. Schweizer (6) S. N. Shore (24) A. Sillanpää (21) J. Sitarek (1) I. Snidaric (5) D. Sobczynska (9) F. Spanier (12) V. Stamatescu (1) A. Stamerra (3) T. Steinbring (12) J. Storz (12) S. Sun (6) T. Surić (5) L. Takalo (21) H. Takami (20) F. Tavecchio (3) P. Temnikov (22) T. Terzić (5) D. Tescaro (8) M. Teshima (6) J. Thaele (15) O. Tibolla (12) D. F. Torres (19) T. Toyama (6) A. Treves (17) P. Vogler (11) R. M. Wagner (6 30) F. Zandanel (16 31) R. Zanin (23) ((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 {L}ódź PL-90236 Lódź 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) Università di Padova INFN I-35131 Padova (15) Technische Universität Dortmund D-44221 Dortmund (16) Inst. de Astrofísica de Andalucía (CSIC) E-18080 Granada (17) Università dell'Insubria Como I-22100 Como (18) Unitat de Física de les Radiacions Departament de Física CERES-IEEC Universitat Autònoma de Barcelona (19) Institut de Ciències de l'Espai (IEEC-CSIC) (20) Japanese MAGIC Consortium Division of Physics Astronomy Kyoto University Japan (21) Finnish MAGIC Consortium Tuorla Observatory University of Turku Department of Physics University of Oulu Finland (22) Inst. for Nucl. Research Nucl. Energy BG-1784 Sofia Bulgaria (23) Universitat de Barcelona (ICC IEEC-UB) E-08028 Barcelona (24) Università di Pisa I-56126 Pisa (25) now at Ecole polytechnique fédérale de Lausanne (EPFL) Lausanne (26) now at Department of Physics & Astronomy UC Riverside CA 92521 USA (27) now at Finnish Centre for Astronomy with ESO (FINCA) Turku (28) also at INAF-Trieste (29) also at Instituto de Fisica Teorica UAM/CSIC E-28049 Madrid (30) now at: Stockholm University Oskar Klein Centre for Cosmoparticle Physics SE-106 91 Stockholm Sweden (31) now at GRAPPA Institute University of Amsterdam 1098XH Amsterdam Netherlands)
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classification astro-ph.HEastro-ph.GA
keywords gamma-raysourcedistantgammalimitsraysupperattenuation
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abstract

The bright gamma-ray quasar 4C +55.17 is a distant source ($z = 0.896$) with a hard spectrum at GeV energies as observed by the Large Area Telescope (LAT) on board the {{\it Fermi}} satellite. This source is identified as a good source candidate for very-high-energy (VHE; $> 30$ GeV) gamma rays. In general VHE gamma rays from distant sources provide an unique opportunity to study the extragalactic background light (EBL) and underlying astrophysics. The flux intensity of this source in the VHE range is investigated. Then, constraints on the EBL are derived from the attenuation of gamma-ray photons coming from the distant blazar. We searched for a gamma-ray signal from this object using the 35-hour observations taken by the MAGIC telescopes between November 2010 and January 2011. No significant VHE gamma-ray signal was detected. We computed the upper limits of the integrated gamma-ray flux at $95\%$ confidence level of $9.4 \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ and $2.5 \times 10^{-12}$ cm$^{-2}$ s$^{-1}$ above $100$ GeV and $200$ GeV, respectively. The differential upper limits in four energy bins in the range from $80$ GeV to $500$ GeV are also derived. The upper limits are consistent with the attenuation predicted by low-flux EBL models on the assumption of a simple power-law spectrum extrapolated from LAT data.

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  1. Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars

    astro-ph.HE 2026-07 accept novelty 6.0 of 10

    Systematic Fermi-LAT search detects VHE emission from 14 Compton-dominated blazars (4 new at >5σ) and constrains the emitting region to >1.1–1.4 BLR radii.

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