Curvature in the very-high energy gamma-ray spectrum of M 87

Aharonian F, Ait Benkhali F, Aschersleben J, Ashkar H, Backes M, Martins VB, Batzofin R, Becherini Y, Berge D, Bernlohr K, Bottcher M, Boisson C, Bolmont J, De Lavergne MDB, Bradascio F, Brose R, Brun F, Bruno B, Bulik T, Burger-Scheidlin C, Bylund T, Casanova S, Cecil R, Celic J, Cerruti M, Chand T, Chandra S, Chen A, Chibueze J, Chibueze O, Collins T, Cotter G, Mbarubucyeye JD, Djannati-Atai A, Djuvsland J, Dmytriiev A, Egberts K, Einecke S, Fegan S, Fontaine G, Funk S, Gabici S, Glicenstein JF, Glombitza J, Grolleron G, Haerer L, Hofmann W, Holch TL, Holler M, Horns D, Jamrozy M, Jankowsky F, Joshi V, Jung-Richardt I, Kasai E, Katarzyński K, Khatoon R, Khelifi B, Kluźniak W, Komin N, Kosack K, Kostunin D, Kundu A, Guedes Lang R, Le Stum S, Leitl F, Lemiere A, Lemoine-Goumard M, Lenain JP, Lypova I, Luashvili A, MacKey J, Malyshev D, Marti-Devesa G, Marx R, Mehta A, Meyer M, Mitchell A, Moderski R, Moghadam MO, Mohrmann L, Montanari A, Moulin E, Murach T, De Naurois M, Niemiec J, Ohm S, Olivera-Nieto L, Wilhelmi EDO, Panny S, Panter M, Parsons RD, Pensec U, Pita S, Puhlhofer G, Punch M, Quirrenbach A, Regeard M, Reimer A, Reimer O, Ren H, Reville B, Rieger F, Rudak B, Ruiz-Velasco E, Sahakian V, Salzmann H, Santangelo A, Sasaki M, Schussler F, Schutte HM, Shapopi JN, Sol H, Spencer S, Stawarz L, Steenkamp R, Steinmassl S, Steppa C, Streil K, Takahashi T, Tanaka T, Taylor AM, Terrier R, Tsirou M, van Eldik C, Venter C, Vink J, Wach T, Wagner SJ, Wierzcholska A, Zacharias M, Zdziarski AA, Zech A, Zilberman P, Zywucka N (2024)


Publication Type: Journal article

Publication year: 2024

Journal

Book Volume: 685

Article Number: A96

DOI: 10.1051/0004-6361/202348913

Abstract

The radio galaxy M 87 is a variable very-high energy (VHE) gamma-ray source, exhibiting three major flares, which were reported in 2005, 2008, and 2010. Despite extensive studies, the origin of the VHE gamma-ray emission is not yet fully understood. In this study, we investigate the VHE gamma-ray spectrum of M 87 during states of high gamma-ray activity, utilizing 20.2 h of H.E.S.S. observations. Our findings indicate a preference for a curved spectrum, characterized by a log-parabola model with extra-galactic background light (EBL) model above 0.3 TeV at the 4σ level, compared to a power-law spectrum with EBL. We investigate the degeneracy between the absorption feature and the EBL normalization and derive upper limits on EBL models that are mainly sensitive in the wavelength range of 12.4 μm-40 μm.

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Involved external institutions

Ruprecht-Karls-Universität Heidelberg DE Germany (DE) Deutsches Elektronen-Synchrotron DESY DE Germany (DE) Max-Planck-Institut für Kernphysik (MPIK) / Max Planck Institute for Nuclear Physics DE Germany (DE) Noordwes-Universiteit / North-West University ZA South Africa (ZA) Laboratoire Univers et Théories (LUTH) / Laboratory of the Universe and Theories FR France (FR) Université Paris-Saclay FR France (FR) University of Warsaw / Uniwersytet Warszawski PL Poland (PL) Institute of Nuclear Physics Polish Academy of Sciences / Instytut Fizyki Jądrowej im. Henryka Niewodniczańskiego Polskiej Akademii Nauk PL Poland (PL) Universität Hamburg (UHH) DE Germany (DE) University of the Witwatersrand (WITS) ZA South Africa (ZA) University of Namibia (UNAM) NA Namibia (NA) Universität Potsdam DE Germany (DE) Université Paris-Sud FR France (FR) Sorbonne Université FR France (FR) Leopold-Franzens-Universität Innsbruck / University of Innsbruck AT Austria (AT) Nicolaus Copernicus University (NCU) / Uniwersytet Mikołaja Kopernika w Toruniu (UMK) PL Poland (PL) Dublin Institute for Advanced Studies (DIAS) IE Ireland (IE) Eberhard Karls Universität Tübingen DE Germany (DE) Laboratoire Leprince-Ringuet (LLR) FR France (FR) University of Groningen / Rijksuniversiteit Groningen NL Netherlands (NL) Institut national de physique nucléaire et de physique des particules (IN2P3) FR France (FR) Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences PL Poland (PL) Université de Bordeaux FR France (FR) Institute of Research into the Fundamental Laws of the Universe / Institut de recherche sur les lois fondamentales de l'univers (IRFU) FR France (FR) University of Amsterdam NL Netherlands (NL) Jagiellonian University / Uniwersytet Jagielloński (UJ) PL Poland (PL) Humboldt-Universität zu Berlin DE Germany (DE) Yerevan Physics Institute (YerPhI) / Երևանի Ֆիզիկայի Ինստիտուտ AM Armenia (AM) University of Tokyo JP Japan (JP) Konan University / 甲南大学 JP Japan (JP) University of Oxford GB United Kingdom (GB) University of Adelaide AU Australia (AU)

How to cite

APA:

Aharonian, F., Ait Benkhali, F., Aschersleben, J., Ashkar, H., Backes, M., Martins, V.B.,... Zywucka, N. (2024). Curvature in the very-high energy gamma-ray spectrum of M 87. Astronomy & Astrophysics, 685. https://doi.org/10.1051/0004-6361/202348913

MLA:

Aharonian, F., et al. "Curvature in the very-high energy gamma-ray spectrum of M 87." Astronomy & Astrophysics 685 (2024).

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