A SEARCH FOR POINT SOURCES OF EeV PHOTONS

Aab A, Abreu P, Aglietta M, Ahlers M, Ahn EJ, Al Samarai I, Albuquerque IFM, Allekotte I, Allen J, Allison P, Almela A, Castillo JA, Alvarez-Muniz J, Batista RA, Ambrosio M, Aminaei A, Anchordoqui L, Andringa S, Aramo C, Arqueros F, Asorey H, Assis PJS, Aublin J, Ave M, Avenier M, Avila G, Badescu AM, Barber KB, Baeuml J, Baus C, Beatty JJ, Becker KH, Bellido JA, Berat C, Bertou X, Biermann PL, Billoir P, Blanco F, Blanco M, Bleve C, Bluemer H, Bohacova M, Boncioli D, Bonifazi C, Bonino R, Borodai N, Brack J, Brancus I, Brogueira P, Brown WC, Buchholz P, Bueno A, Buscemi M, Caballero-Mora KS, Caccianiga B, Caccianiga L, Candusso M, Caramete L, Caruso R, Castellina A, Cataldi G, Cazon L, Cester R, Chavez AG, Cheng SH, Chiavassa A, Chinellato JA, Chudoba J, Cilmo M, Clay RW, Cocciolo G, Colalillo R, Collica L, Coluccia MR, Conceicao R, Contreras F, Cooper MJ, Coutu S, Covault CE, Criss A, Cronin J, Curutiu A, Dallier R, Daniel B, Dasso S, Daumiller K, Dawson BR, De Almeida RM, De Domenico M, De Jong SJ, Neto JRTDM, De Mitri I, De Oliveira J, De Souza V, Del Peral L, Deligny O, Dembinski H, Dhital N, Di Giulio C, Di Matteo A, Diaz JC, Castro MLD, Diep PN, Diogo F, Dobrigkeit C, Docters W, D'Olivo JC, Dong PN, Dorofeev A, Hasankiadeh QD, Dova MT, Ebr J, Engel R, Erdmann M, Erfani M, Escobar CO, Espadanal J, Etchegoyen A, Luis PFS, Falcke H, Fang K, Farrar G, Fauth AC, Fazzini N, Ferguson AP, Fernandes M, Fick B, Figueira JM, Filevich A, Filipcic A, Fox BD, Fratu O, Froehlich U, Fuchs B, Fuji T, Gaior R, Garcia B, Garcia Roca ST, Garcia-Gamez D, Garcia-Pinto D, Garilli G, Bravo AG, Gate F, Gemmeke H, Ghia PL, Giaccari U, Giammarchi M, Giller M, Glaser C, Glass H, Albarracin FG, Gomez Berisso M, Gomez Vitale PF, Goncalves P, Gonzalez JG, Gookin B, Gorgi A, Gorham P, Gouffon P, Grebe S, Griffith N, Grillo AF, Grubb TD, Guardincerri Y, Guarino F, Guedes GP, Hansen P, Harari D, Harrison TA, Harton JL, Haungs A, Hebbeker T, Heck D, Heimann P, Herve AE, Hill GC, Hojvat C, Hollon N, Holt E, Homola P, Hoerandel JR, Horvath P, Hrabovsky M, Huber D, Huege T, Insolia A, Isar PG, Islo K, Jandt I, Jansen S, Jarne C, Josebachuili M, Kaeaepae A, Kambeitz O, Kampert KH, Kasper P, Katkov I, Kegl B, Keilhauer B, Keivani A, Kemp E, Kieckhafer RM, Klages HO, Kleifges M, Kleinfeller J, Krause R, Krohm N, Kroemer O, Kruppke-Hansen D, Kuempel D, Kunka N, La Rosa G, Lahurd D, Latronico L, Lauer R, Lauscher M, Lautridou P, Le Coz S, Leao MSAB, Lebrun D, Lebrun P, De Oliveira MAL, Letessier-Selvon A, Lhenry-Yvon I, Link K, Lopez R, Aguera AL, Louedec K, Bahilo JL, Lu L, Lucero A, Ludwig M, Lyberis H, Maccarone MC, Malacari M, Maldera S, Maller J, Mandat D, Mantsch P, Mariazzi AG, Marin V, Maris IC, Marsella G, Martello D, Martin L, Martinez H, Bravo OM, Martraire D, Meza JJM, Mathes HJ, Mathys S, Matthews AJ, Matthews J, Matthiae G, Maurel D, Maurizio D, Mayotte E, Mazur PO, Medina C, Medina-Tanco G, Melissas M, Melo D, Menichetti E, Menshikov A, Messina S, Meyhandan R, Micanovic S, Micheletti MI, Middendorf L, Minaya IA, Miramonti L, Mitrica B, Molina-Bueno L, Mollerach S, Monasor M, Ragaigne DM, Montanet F, Morello C, Moreno JC, Mostafa M, Moura CA, Muller MA, Mueller G, Muenchmeyer M, Mussa R, Navarra G, Navas S, Necesal P, Nellen L, Nelles A, Neuser J, Niechciol M, Niemietz L, Niggemann T, Nitz D, Nosek D, Novotny V, Nozka L, Ochilo L, Olinto A, Oliveira M, Ortiz M, Pacheco N, Selmi-Dei DP, Palatka M, Pallotta J, Palmieri N, Papenbreer P, Parente G, Parra A, Pastor S, Paul T, Pech M, Pekala J, Pelayo R, Pepe IM, Perrone L, Pesce R, Petermann E, Peters C, Petrera S, Petrolini A, Petrov Y, Piegaia R, Pierog T, Pieroni P, Pimenta M, Pirronello V, Platino M, Plum M, Porcelli A, Porowski C, Privitera P, Prouza M, Purrello VH, Quel EJ, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Revenu B, Ridky J, Riggi S, Risse M, Ristori P, Rizi V, Roberts J, De Carvalho WR, Cabo IR, Fernandez GR, Rojo JR, Rodriguez-Frias MD, Ros G, Rosado J, Rossler T, Roth M, Roulet E, Rovero AC, Ruehle C, Saffi SJ, Saftoiu A, Salamida F, Salazar H, Greus FS, Salina G, Sanchez F, Sanchez-Lucas P, Santo CE, Santos E, Santos EM, Sarazin F, Sarkar B, Sarmento R, Sato R, Scharf N, Scherini V, Schieler H, Schiffer P, Schmidt A, Scholten O, Schoorlemmer H, Schovanek P, Schulz A, Schulz J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard RC, Sidelnik I, Sigl G, Sima O, Smialkowski A, Smida R, Snow GR, Sommers P, Sorokin J, Squartini R, Srivastava YN, Stanic S, Stapleton J, Stasielak J, Stephan M, Stutz A, Suarez F, Suomijaervi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Szuba M, Taborda OA, Tapia A, Tartare M, Thao NT, Theodoro VM, Tiffenberg J, Timmermans C, Peixoto CJT, Toma G, Tomankova L, Tome B, Tonachini A, Elipe GT, Machado DT, Travnicek P, Trovato E, Tueros M, Ulrich R, Unger M, Urban M, Valdes Galicia JF, Valino I, Valore L, Van Aar G, Van Den Berg AM, Van Velzen S, Van Vliet A, Varela E, Cardenas BV, Varner G, Vazquez JR, Vazquez RA, Veberic D, Verzi V, Vicha J, Videla M, Villasenor L, Vlcek B, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weidenhaupt K, Weindl A, Werner F, Whelan BJ, Widom A, Wiencke L, Wilczynska B, Wilczynski H, Will M, Williams C, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yamamoto T, Yapici T, Younk P, Yuan G, Yushkov A, Zamorano B, Zas E, Zavrtanik D, Zavrtanik M, Zaw I, Zepeda A, Zhou J, Zhu Y, Silva MZ, Ziolkowski M (2014)


Publication Status: Published

Publication Type: Journal article

Publication year: 2014

Journal

Publisher: IOP PUBLISHING LTD

Book Volume: 789

Article Number: ARTN 160

Journal Issue: 2

DOI: 10.1088/0004-637X/789/2/160

Abstract

Measurements of air showers made using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point sources of EeV photons anywhere in the exposed sky. A multivariate analysis reduces the background of hadronic cosmic rays. The search is sensitive to a declination band from -85 degrees to +20 degrees, in an energy range from 10(17.3) eV to 10(18.5) eV. No photon point source has been detected. An upper limit on the photon flux has been derived for every direction. The mean value of the energy flux limit that results from this, assuming a photon spectral index of -2, is 0.06 eV cm(-2) s(-1), and no celestial direction exceeds 0.25 eV cm(-2) s(-1). These upper limits constrain scenarios in which EeV cosmic ray protons are emitted by non-transient sources in the Galaxy.

How to cite

APA:

Aab, A., Abreu, P., Aglietta, M., Ahlers, M., Ahn, E.J., Al Samarai, I.,... Ziolkowski, M. (2014). A SEARCH FOR POINT SOURCES OF EeV PHOTONS. Astrophysical Journal, 789(2). https://dx.doi.org/10.1088/0004-637X/789/2/160

MLA:

Aab, A., et al. "A SEARCH FOR POINT SOURCES OF EeV PHOTONS." Astrophysical Journal 789.2 (2014).

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