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. 2013 Jan 25;110(4):041301.
doi: 10.1103/PhysRevLett.110.041301. Epub 2013 Jan 22.

Search for photon-linelike signatures from dark matter annihilations with H.E.S.S

A Abramowski  1 F Acero  2 F Aharonian  3 A G Akhperjanian  4 G Anton  5 S Balenderan  6 A Balzer  7 A Barnacka  8 Y Becherini  9 J Becker Tjus  10 K Bernlöhr  11 E Birsin  12 J Biteau  13 A Bochow  14 C Boisson  15 J Bolmont  16 P Bordas  17 J Brucker  5 F Brun  13 P Brun  18 T Bulik  19 S Carrigan  14 S Casanova  20 M Cerruti  15 P M Chadwick  6 R C G Chaves  21 A Cheesebrough  6 S Colafrancesco  22 G Cologna  23 J Conrad  24 C Couturier  16 M Dalton  25 M K Daniel  6 I D Davids  26 B Degrange  13 C Deil  14 P deWilt  27 H J Dickinson  24 A Djannati-Ataï  28 W Domainko  14 L O'C Drury  29 G Dubus  30 K Dutson  31 J Dyks  32 M Dyrda  33 K Egberts  34 P Eger  5 P Espigat  28 L Fallon  29 C Farnier  24 S Fegan  13 F Feinstein  2 M V Fernandes  1 D Fernandez  2 A Fiasson  35 G Fontaine  13 A Förster  14 M Füßling  12 M Gajdus  12 Y A Gallant  2 T Garrigoux  16 H Gast  14 B Giebels  13 J F Glicenstein  18 B Glück  5 D Göring  5 M-H Grondin  36 S Häffner  5 J D Hague  14 J Hahn  14 D Hampf  1 J Harris  6 S Heinz  5 G Heinzelmann  1 G Henri  30 G Hermann  14 A Hillert  14 J A Hinton  31 W Hofmann  14 P Hofverberg  14 M Holler  37 D Horns  1 A Jacholkowska  16 C Jahn  5 M Jamrozy  38 I Jung  5 M A Kastendieck  1 K Katarzyński  39 U Katz  5 S Kaufmann  23 B Khélifi  13 S Klepser  40 D Klochkov  17 W Kluźniak  32 T Kneiske  1 Nu Komin  35 K Kosack  18 R Kossakowski  35 F Krayzel  35 P P Krüger  20 H Laffon  13 G Lamanna  35 J Lefaucheur  28 M Lemoine-Goumard  41 J-P Lenain  28 D Lennarz  14 T Lohse  12 A Lopatin  5 C-C Lu  14 V Marandon  14 A Marcowith  2 J Masbou  35 G Maurin  35 N Maxted  27 M Mayer  37 T J L McComb  6 M C Medina  18 J Méhault  42 U Menzler  10 R Moderski  32 M Mohamed  23 E Moulin  18 C L Naumann  16 M Naumann-Godo  18 M de Naurois  13 D Nedbal  43 D Nekrassov  14 N Nguyen  1 J Niemiec  33 S J Nolan  6 S Ohm  44 E de Oña Wilhelmi  14 B Opitz  1 M Ostrowski  38 I Oya  12 M Panter  14 R D Parsons  14 M Paz Arribas  12 N W Pekeur  45 G Pelletier  30 J Perez  34 P-O Petrucci  30 B Peyaud  18 S Pita  28 G Pühlhofer  17 M Punch  28 A Quirrenbach  23 M Raue  1 A Reimer  34 O Reimer  34 M Renaud  2 R de Los Reyes  14 F Rieger  14 J Ripken  24 L Rob  43 S Rosier-Lees  35 G Rowell  27 B Rudak  32 C B Rulten  6 V Sahakian  4 D A Sanchez  14 A Santangelo  17 R Schlickeiser  10 A Schulz  40 U Schwanke  12 S Schwarzburg  17 S Schwemmer  23 F Sheidaei  46 J L Skilton  14 H Sol  15 G Spengler  12 L Stawarz  38 R Steenkamp  26 C Stegmann  7 F Stinzing  5 K Stycz  40 I Sushch  12 A Szostek  38 J-P Tavernet  16 R Terrier  28 M Tluczykont  1 C Trichard  35 K Valerius  5 C van Eldik  47 G Vasileiadis  2 C Venter  45 A Viana  18 P Vincent  16 H J Völk  14 F Volpe  14 S Vorobiov  2 M Vorster  45 S J Wagner  23 M Ward  6 R White  31 A Wierzcholska  38 D Wouters  18 M Zacharias  10 A Zajczyk  48 A A Zdziarski  32 A Zech  15 H-S Zechlin  1 HESS Collaboration
Affiliations

Search for photon-linelike signatures from dark matter annihilations with H.E.S.S

A Abramowski et al. Phys Rev Lett. .

Abstract

Gamma-ray line signatures can be expected in the very-high-energy (E(γ)>100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily distinguishable from astrophysical γ-ray sources that in most cases produce continuous spectra that span over several orders of magnitude in energy. Using data collected with the H.E.S.S. γ-ray instrument, upper limits on linelike emission are obtained in the energy range between ∼ 500 GeV and ∼ 25 TeV for the central part of the Milky Way halo and for extragalactic observations, complementing recent limits obtained with the Fermi-LAT instrument at lower energies. No statistically significant signal could be found. For monochromatic γ-ray line emission, flux limits of (2 × 10(-7) -2 × 10(-5)) m(-2) s(-1) sr(-1) and (1 × 10(-8) -2 × 10(-6)) m(-2) s(-1)sr(-1) are obtained for the central part of the Milky Way halo and extragalactic observations, respectively. For a DM particle mass of 1 TeV, limits on the velocity-averaged DM annihilation cross section ⟨σv⟩(χχ → γγ) reach ∼ 10(-27) cm(3)s(-1), based on the Einasto parametrization of the Galactic DM halo density profile.

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