We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory / Abreu, P; Aglietta, M; Ahlers, M; Ahn, Ej; Albuquerque, Ifm; Allekotte, I; Allen, J; Allison, P; Almela, A; Castillo, Ja; Alvarcz-Muniz, J; Batista, Ra; Ambrosio, M; Aminaei, A; Anchordoqui, L; Andringa, S; Antici'C, T; Aramo, C; Arqueros, F; Asorey, H; Assis, P; Aublin, J; Ave, M; Avenier, M; Avila, G; Badescu, Am; Barber, Kb; Barbosa, Af; Bardenet, R; Baughman, B; Bauml, J; Baus, C; Beatty, Jj; Becker, Kh; Belletoile, A; Bellido, Ja; Benzvi, S; Berat, C; Bertou, X; Biermann, Pl; Billoir, P; Blanco, F; Blanco, M; Bleve, C; Blumer, H; Bohacova, M; Boncioli, D; Bonifazi, C; Bonino, R; Borodai, N; Brack, J; Brancus, I; Brogueira, P; Brown, Vc; Buchholz, P; Bueno, A; Buroker, L; Burton, Re; Buscemi, M; Caballero-Mora, Ks; Caccianiga, B; Caramete, F; Caruso, R; Castellina, A; Cataldi, G; Cazon, L; Cester, R; Chauvin, J; Cheng, Sh; Chiavassa, A; Chinellato, Ja; Diaz, Jc; Chudoba, J; Cilmo, M; Clay, Rw; Cocciolo, G; Colalillo, R; Collica, L; Coluccia, Mr; Conceicao, R; Contreras, F; Cook, H; Cooper, Mj; Coppens, J; 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 Donato, C; de Jong, Sj; De la Vegas, G; de Mello, Wjm; Neto, Jrtd; De Mitri, I; De Souza, V; de Vries, Kd; del Peral, L; Deligny, O; Dembinski, H; Dhital, N; Di Giulio, C; Castro, Mld; Diep, Pn; Diogo, F; Dobrigkeit, C; Docters, W; D'Olivo, Jc; Dong, Pn; Dorofeev, A; dos Anjos, Jc; Dova, Mt; D'Urso, D; Ebr, J; Engel, R; Erdmann, M; Escobar, Co; Espadartal, J; Etchegoyen, A; San Luis, Pf; Falcke, H; Fang, K; Farrar, G; Fauth, Ac; Fazzini, N; Ferguson, Ap; Fick, B; Figueira, Jm; Filevich, A; Filipcic, A; Fliescher, S; Fox, B; Fracchiolla, Ce; Fraenkel, Fd; Fratu, O; Frohlich, U; Fuchs, B; Gaior, R; Gamarra, Rf; Gambetta, S; Garcia, B; Roca, Stg; Garcia-Gamez, D; Garcia-Pinto, D; Garilli, G; Bravo, Ag; Gemmeke, H; Ghia, Pl; Giller, M; Gitto, J; Glass, H; Gold, Ms; Golup, G; Albarracin, Fg; Berisso, Mg; Vitale, Pfg; Goncalves, P; Gonzalez, Jg; Gookin, B; Gorgi, A; Gorham, P; Gouffon, P; Grashorn, E; Grebe, S; Griffith, N; Grillo, Af; Guardincerri, Y; Guarino, F; Guedes, Gp; Hansen, P; Harari, D; Harrison, Ta; Harton, Jl; Haungs, A; Hebbeker, T; Heck, D; Herve, Ae; Hill, Gc; Hojvat, C; Hollon, N; Holmes, Vc; Homola, P; Horandel, Jr; Horvath, P; Hrabovsky, M; Huber, D; Huege, T; Insolia, A; Ionita, F; Jansen, S; Jarne, C; Jirtskova, S; Josebachuili, M; Kadija, K; Kampert, Kh; Karhan, P; Kasper, P; Katkov, I; Kegl, B; Keilkauer, B; Keivani, A; Kelley, Jl; Kemp, E; Kieckhafer, Rm; Klages, Ho; Kleifges, M; Kleinfeller, J; Knapp, J; Koang, Dh; Kotera, K; Krohm, N; Kroemer, O; Kruppke-Hansen, D; Kuempel, D; Kulbartz, Jk; Kunka, N; La Rosa, G; Lahurd, D; Latronico, L; Lauer, R; Lauscher, M; Lautridon, 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; Macolino, C; Malacari, M; Maldera, S; Maller, J; Mandat, D; Mantsch, P; Mariazzi, Ag; Marin, J; Marin, V; Maris, Ic; Falcon, Hrm; Marsella, G; Martello, D; Martin, L; Martinez, H; Bravo, Om; Martraire, D; Meza, Jjm; Mathes, Hj; Matthews, J; Matthews, Jaj; Matthiae, G; Maurel, D; Maurizio, D; Mayotte, E; Mazur, Po; Medina-Tanco, G; Melissas, M; Melo, D; Menichetti, E; Menshikov, A; Mertsch, P; Messina, S; Meurer, C; Meyhandan, R; Mi'Canovi'C, S; Micheletti, Mi; Minaya, Ia; Miramonti, L; Mitrica, B; Molina-Bueno, L; Mollerach, S; Monasor, M; Ragaigne, Dm; Montanet, F; Morales, B; Morello, C; Moreno, Jc; Mostafa, M; Moura, Ca; Muller, Ma; Muller, G; Munchmeyer, M; Mussa, R; Navarra, G; Navarro, Jl; Navas, S; Necesal, P; Nellen, L; Nelles, A; Neuser, J; Nhung, Pt; Niechciol, M; Niemietz, L; Nierstenhoefer, N; Niggemann, T; Nitz, D; Nosek, D; Nozka, L; Oehlschlager, J; Olinto, A; Oliveira, M; Ortiz, M; Pacheco, N; Selmi-Dei, Dp; Palatka, M; Pallotta, J; Palmieri, N; Parente, G; Parra, A; Pastor, S; Paul, T; Pech, M; Pekala, J; Pelayo, R; Pepe, Im; Perrone, L; Pesce, R; Petermann, E; Petrera, S; Petrolini, A; Petrov, Y; Pfendner, C; Piegaia, R; Pierog, T; Pieroni, P; Pimenta, M; Pirronello, V; Platino, M; Plum, M; Ponce, Vh; Pontz, M; Porcelli, A; Privitera, P; Prouza, M; Quel, Ej; Querchfeld, S; Rautenberg, J; Ravel, O; Ravignani, D; Revenu, B; Ridky, J; Riggi, S; Risse, M; Ristori, P; Rivera, H; Rizi, V; Roberts, J; de Carvalho, Wr; Cabo, Ir; Fernandez, Gr; Martino, Jr; Rojo, Jr; Rodriguez-Frias, Md; Ros, G; Rosado, J; Rossler, T; Roth, M; Rouille-d'Orfeuil, B; Roulet, E; Rovero, Ac; Ruhle, C; Saffi, Sj; Saftoiu, A; Salamida, F; Salazar, H; Greus, Fs; Salina, G; Sanchez, F; Santo, Ce; Santos, E; Santos, Em; Sarazin, F; Sarkar, B; Sarkar, S; Sato, R; Scharf, N; Scherini, V; Schieler, H; Schiffer, P; Schmidt, A; Scholten, O; Schoorlemmer, H; Schovancova, J; Schovanek, P; Schroder, F; Schulz, J; Schuster, D; Sciutto, Sj; Scuderi, M; Segreto, A; Settimo, M; Shadkam, A; Shellard, Rc; Sidelnik, I; Sigl, G; Lopez, Hhs; Sima, O; 'Smialkowski, A; Smida, R; Snow, Gr; Sommers, P; Sorokin, J; Spinka, H; Squartini, R; Srivastava, Yn; Stanic, S; Stapleton, J; Stasielak, J; Stephan, M; Straub, M; Stutz, A; Suarez, F; Suomijaevi, T; Supanitsky, Ad; Susa, T; Sutherland, Ms; Swain, J; Szadkowski, Z; Szuba, M; Tapia, A; Tartare, M; Tascau, O; Tcaciuc, R; Thao, Nt; Thomas, D; Tiffenberg, J; Timmermans, C; Tkaczyk, V; Peixoto, Cjt; Toma, G; Tomankova, L; Tome, B; Tonachini, A; Elippe, Gt; Machado, Dt; Travnicek, P; Tridapalli, Db; Trovato, E; Tueros, M; Ulrich, R; Unger, M; Urban, M; Galicia, Jfv; Vallno, I; Valore, L; van Aar, G; van den Berg, Am; van Velzen, S; van Vliet, A; Varela, E; Cardenas, Bv; Varner, C; Vazquez, Jr; Vazquez, Ra; Veberie, D; Verzi, V; Vicha, J; Videla, M; Villasenor, L; Wahlberg, H; Wahrlich, P; Wainberg, O; Walz, D; Watson, Aa; Weber, M; Weidenhaupt, K; Weindl, A; Werner, F; Westerhoff, S; Whelan, Bj; Widom, A; Wieczorek, G; Wiencke, L; Wilczynska, B; Wilczyriski, H; Will, M; Williams, C; Winchen, T; Wommer, M; Wundheiler, B; Yamamoto, T; Yapici, T; Younki, P; Yuan, G; Yushkov, A; Garcia, Bz; Zas, E; Zavrtanik, D; Zavrtanik, M; Zaw, I; Zepeda, A; Zhou, J; Zhu, Y; Silva, Mz; Ziolkowski, M. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 5(2013). [10.1088/1475-7516/2013/05/009]
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
Abreu P; Aglietta M; Ahlers M; Ahn EJ; Albuquerque IFM; Allekotte I; Allen J; Allison P; Almela A; Castillo JA; Alvarcz-Muniz J; Batista RA; Ambrosio M; Aminaei A; Anchordoqui L; Andringa S; Antici'c T; Aramo C; Arqueros F; Asorey H; Assis P; Aublin J; Ave M; Avenier M; Avila G; Badescu AM; Barber KB; Barbosa AF; Bardenet R; Baughman B; Bauml J; Baus C; Beatty JJ; Becker KH; Belletoile A; Bellido JA; BenZvi S; Berat C; Bertou X; Biermann PL; Billoir P; Blanco F; Blanco M; Bleve C; Blumer H; Bohacova M; Boncioli D; Bonifazi C; Bonino R; Borodai N; Brack J; Brancus I; Brogueira P; Brown VC; Buchholz P; Bueno A; Buroker L; Burton RE; Buscemi M; Caballero-Mora KS; Caccianiga B; Caramete F; Caruso R; Castellina A; Cataldi G; Cazon L; Cester R; Chauvin J; Cheng SH; Chiavassa A; Chinellato JA; Diaz JC; Chudoba J; Cilmo M; Clay RW; Cocciolo G; Colalillo R; Collica L; Coluccia MR; Conceicao R; Contreras F; Cook H; Cooper MJ; Coppens J; 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 Donato C; de Jong SJ; De la Vegas G; de Mello WJM; Neto JRTD; De Mitri I; De Souza V; de Vries KD; del Peral L; Deligny O; Dembinski H; Dhital N; Di Giulio C; Castro MLD; Diep PN; Diogo F; Dobrigkeit C; Docters W; D'Olivo JC; Dong PN; Dorofeev A; dos Anjos JC; Dova MT; D'Urso D ;Ebr J; Engel R; Erdmann M; Escobar CO; Espadartal J; Etchegoyen A; San Luis PF; Falcke H; Fang K; Farrar G; Fauth AC; Fazzini N; Ferguson AP; Fick B; Figueira JM; Filevich A; Filipcic A; Fliescher S; Fox B; Fracchiolla CE; Fraenkel FD; Fratu O; Frohlich U; Fuchs B; Gaior R; Gamarra RF; Gambetta S; Garcia B; Roca STG; Garcia-Gamez D; Garcia-Pinto D; Garilli G; Bravo AG; Gemmeke H; Ghia PL; Giller M; Gitto J; Glass H; Gold MS; Golup G; Albarracin FG; Berisso MG; Vitale PFG; Goncalves P; Gonzalez JG; Gookin B; Gorgi A; Gorham P; Gouffon P; Grashorn E; Grebe S; Griffith N; Grillo AF; Guardincerri Y; Guarino F; Guedes GP; Hansen P; Harari D; Harrison TA; Harton JL; Haungs A; Hebbeker T; Heck D; Herve AE; Hill GC; Hojvat C; Hollon N; Holmes VC; Homola P; Horandel JR; Horvath P; Hrabovsky M; Huber D; Huege T; Insolia A; Ionita F; Jansen S; Jarne C; Jirtskova S; Josebachuili M; Kadija K; Kampert KH; Karhan P; Kasper P; Katkov I; Kegl B; Keilkauer B; Keivani A; Kelley JL; Kemp E; Kieckhafer RM; Klages HO; Kleifges M; Kleinfeller J; Knapp J; Koang DH; Kotera K; Krohm N; Kroemer O; Kruppke-Hansen D; Kuempel D; Kulbartz JK; Kunka N; La Rosa G; LaHurd D; Latronico L; Lauer R; Lauscher M; Lautridon 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; Macolino C; Malacari M; Maldera S; Maller J; Mandat D; Mantsch P; Mariazzi AG; Marin J; Marin V; Maris IC; Falcon HRM; Marsella G; Martello D; Martin L; Martinez H; Bravo OM; Martraire D; Meza JJM; Mathes HJ; Matthews J; Matthews JAJ; Matthiae G; Maurel D; Maurizio D; Mayotte E; Mazur PO; Medina-Tanco G; Melissas M; Melo D; Menichetti E; Menshikov A; Mertsch P; Messina S; Meurer C; Meyhandan R; Mi'canovi'c S; Micheletti MI; Minaya IA; Miramonti L; Mitrica B; Molina-Bueno L; Mollerach S; Monasor M; Ragaigne DM; Montanet F; Morales B; Morello C; Moreno JC; Mostafa M; Moura CA; Muller MA; Muller G; Munchmeyer M; Mussa R; Navarra G; Navarro JL; Navas S; Necesal P; Nellen L; Nelles A; Neuser J; Nhung PT; Niechciol M; Niemietz L; Nierstenhoefer N; Niggemann T; Nitz D; Nosek D; Nozka L; Oehlschlager J; Olinto A; Oliveira M; Ortiz M; Pacheco N; Selmi-Dei DP; Palatka M; Pallotta J; Palmieri N; Parente G; Parra A; Pastor S; Paul T; Pech M; Pekala J; Pelayo R; Pepe IM; Perrone L; Pesce R; Petermann E; Petrera S; Petrolini A; Petrov Y; Pfendner C; Piegaia R; Pierog T; Pieroni P; Pimenta M; Pirronello V; Platino M; Plum M; Ponce VH; Pontz M; Porcelli A; Privitera P; Prouza M; Quel EJ; Querchfeld S; Rautenberg J; Ravel O; Ravignani D; Revenu B; Ridky J; Riggi S; Risse M; Ristori P; Rivera H; Rizi V; Roberts J; de Carvalho WR; Cabo IR; Fernandez GR; Martino JR; Rojo JR; Rodriguez-Frias MD; Ros G; Rosado J; Rossler T; Roth M; Rouille-d'Orfeuil B; Roulet E; Rovero AC; Ruhle C; Saffi SJ; Saftoiu A; Salamida F; Salazar H; Greus FS; Salina G; Sanchez F; Santo CE; Santos E; Santos EM; Sarazin F; Sarkar B; Sarkar S; Sato R; Scharf N; Scherini V ;Schieler H; Schiffer P; Schmidt A; Scholten O; Schoorlemmer H; Schovancova J; Schovanek P; Schroder F; Schulz J; Schuster D; Sciutto SJ; Scuderi M; Segreto A; Settimo M; Shadkam A; Shellard RC; Sidelnik I; Sigl G; Lopez HHS; Sima O; 'Smialkowski A; Smida R; Snow GR; Sommers P; Sorokin J; Spinka H; Squartini R; Srivastava YN; Stanic S; Stapleton J; Stasielak J; Stephan M; Straub M; Stutz A; Suarez F; Suomijaevi T; Supanitsky AD; Susa T; Sutherland MS; Swain J; Szadkowski Z; Szuba M; Tapia A; Tartare M; Tascau O; Tcaciuc R; Thao NT; Thomas D; Tiffenberg J; Timmermans C; Tkaczyk V; Peixoto CJT; Toma G; Tomankova L; Tome B; Tonachini A; Elippe GT; Machado DT; Travnicek P; Tridapalli DB; Trovato E; Tueros M; Ulrich R; Unger M; Urban M; Galicia JFV; Vallno I; Valore L; van Aar G; van den Berg AM; van Velzen S; van Vliet A; Varela E; Cardenas BV; Varner C; Vazquez JR; Vazquez RA; Veberie D; Verzi V; Vicha J; Videla M; Villasenor L; Wahlberg H; Wahrlich P; Wainberg O; Walz D; Watson AA; Weber M; Weidenhaupt K; Weindl A; Werner F; Westerhoff S; Whelan BJ; Widom A; Wieczorek G; Wiencke L; Wilczynska B; Wilczyriski H; Will M; Williams C; Winchen T; Wommer M; Wundheiler B; Yamamoto T; Yapici T; Younki P; Yuan G; Yushkov A; Garcia BZ; Zas E; Zavrtanik D; Zavrtanik M; Zaw I; Zepeda A; Zhou J; Zhu Y; Silva MZ; Ziolkowski M
2013-01-01
Abstract
We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.
Citazione
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory / Abreu, P; Aglietta, M; Ahlers, M; Ahn, Ej; Albuquerque, Ifm; Allekotte, I; Allen, J; Allison, P; Almela, A; Castillo, Ja; Alvarcz-Muniz, J; Batista, Ra; Ambrosio, M; Aminaei, A; Anchordoqui, L; Andringa, S; Antici'C, T; Aramo, C; Arqueros, F; Asorey, H; Assis, P; Aublin, J; Ave, M; Avenier, M; Avila, G; Badescu, Am; Barber, Kb; Barbosa, Af; Bardenet, R; Baughman, B; Bauml, J; Baus, C; Beatty, Jj; Becker, Kh; Belletoile, A; Bellido, Ja; Benzvi, S; Berat, C; Bertou, X; Biermann, Pl; Billoir, P; Blanco, F; Blanco, M; Bleve, C; Blumer, H; Bohacova, M; Boncioli, D; Bonifazi, C; Bonino, R; Borodai, N; Brack, J; Brancus, I; Brogueira, P; Brown, Vc; Buchholz, P; Bueno, A; Buroker, L; Burton, Re; Buscemi, M; Caballero-Mora, Ks; Caccianiga, B; Caramete, F; Caruso, R; Castellina, A; Cataldi, G; Cazon, L; Cester, R; Chauvin, J; Cheng, Sh; Chiavassa, A; Chinellato, Ja; Diaz, Jc; Chudoba, J; Cilmo, M; Clay, Rw; Cocciolo, G; Colalillo, R; Collica, L; Coluccia, Mr; Conceicao, R; Contreras, F; Cook, H; Cooper, Mj; Coppens, J; 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 Donato, C; de Jong, Sj; De la Vegas, G; de Mello, Wjm; Neto, Jrtd; De Mitri, I; De Souza, V; de Vries, Kd; del Peral, L; Deligny, O; Dembinski, H; Dhital, N; Di Giulio, C; Castro, Mld; Diep, Pn; Diogo, F; Dobrigkeit, C; Docters, W; D'Olivo, Jc; Dong, Pn; Dorofeev, A; dos Anjos, Jc; Dova, Mt; D'Urso, D; Ebr, J; Engel, R; Erdmann, M; Escobar, Co; Espadartal, J; Etchegoyen, A; San Luis, Pf; Falcke, H; Fang, K; Farrar, G; Fauth, Ac; Fazzini, N; Ferguson, Ap; Fick, B; Figueira, Jm; Filevich, A; Filipcic, A; Fliescher, S; Fox, B; Fracchiolla, Ce; Fraenkel, Fd; Fratu, O; Frohlich, U; Fuchs, B; Gaior, R; Gamarra, Rf; Gambetta, S; Garcia, B; Roca, Stg; Garcia-Gamez, D; Garcia-Pinto, D; Garilli, G; Bravo, Ag; Gemmeke, H; Ghia, Pl; Giller, M; Gitto, J; Glass, H; Gold, Ms; Golup, G; Albarracin, Fg; Berisso, Mg; Vitale, Pfg; Goncalves, P; Gonzalez, Jg; Gookin, B; Gorgi, A; Gorham, P; Gouffon, P; Grashorn, E; Grebe, S; Griffith, N; Grillo, Af; Guardincerri, Y; Guarino, F; Guedes, Gp; Hansen, P; Harari, D; Harrison, Ta; Harton, Jl; Haungs, A; Hebbeker, T; Heck, D; Herve, Ae; Hill, Gc; Hojvat, C; Hollon, N; Holmes, Vc; Homola, P; Horandel, Jr; Horvath, P; Hrabovsky, M; Huber, D; Huege, T; Insolia, A; Ionita, F; Jansen, S; Jarne, C; Jirtskova, S; Josebachuili, M; Kadija, K; Kampert, Kh; Karhan, P; Kasper, P; Katkov, I; Kegl, B; Keilkauer, B; Keivani, A; Kelley, Jl; Kemp, E; Kieckhafer, Rm; Klages, Ho; Kleifges, M; Kleinfeller, J; Knapp, J; Koang, Dh; Kotera, K; Krohm, N; Kroemer, O; Kruppke-Hansen, D; Kuempel, D; Kulbartz, Jk; Kunka, N; La Rosa, G; Lahurd, D; Latronico, L; Lauer, R; Lauscher, M; Lautridon, 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; Macolino, C; Malacari, M; Maldera, S; Maller, J; Mandat, D; Mantsch, P; Mariazzi, Ag; Marin, J; Marin, V; Maris, Ic; Falcon, Hrm; Marsella, G; Martello, D; Martin, L; Martinez, H; Bravo, Om; Martraire, D; Meza, Jjm; Mathes, Hj; Matthews, J; Matthews, Jaj; Matthiae, G; Maurel, D; Maurizio, D; Mayotte, E; Mazur, Po; Medina-Tanco, G; Melissas, M; Melo, D; Menichetti, E; Menshikov, A; Mertsch, P; Messina, S; Meurer, C; Meyhandan, R; Mi'Canovi'C, S; Micheletti, Mi; Minaya, Ia; Miramonti, L; Mitrica, B; Molina-Bueno, L; Mollerach, S; Monasor, M; Ragaigne, Dm; Montanet, F; Morales, B; Morello, C; Moreno, Jc; Mostafa, M; Moura, Ca; Muller, Ma; Muller, G; Munchmeyer, M; Mussa, R; Navarra, G; Navarro, Jl; Navas, S; Necesal, P; Nellen, L; Nelles, A; Neuser, J; Nhung, Pt; Niechciol, M; Niemietz, L; Nierstenhoefer, N; Niggemann, T; Nitz, D; Nosek, D; Nozka, L; Oehlschlager, J; Olinto, A; Oliveira, M; Ortiz, M; Pacheco, N; Selmi-Dei, Dp; Palatka, M; Pallotta, J; Palmieri, N; Parente, G; Parra, A; Pastor, S; Paul, T; Pech, M; Pekala, J; Pelayo, R; Pepe, Im; Perrone, L; Pesce, R; Petermann, E; Petrera, S; Petrolini, A; Petrov, Y; Pfendner, C; Piegaia, R; Pierog, T; Pieroni, P; Pimenta, M; Pirronello, V; Platino, M; Plum, M; Ponce, Vh; Pontz, M; Porcelli, A; Privitera, P; Prouza, M; Quel, Ej; Querchfeld, S; Rautenberg, J; Ravel, O; Ravignani, D; Revenu, B; Ridky, J; Riggi, S; Risse, M; Ristori, P; Rivera, H; Rizi, V; Roberts, J; de Carvalho, Wr; Cabo, Ir; Fernandez, Gr; Martino, Jr; Rojo, Jr; Rodriguez-Frias, Md; Ros, G; Rosado, J; Rossler, T; Roth, M; Rouille-d'Orfeuil, B; Roulet, E; Rovero, Ac; Ruhle, C; Saffi, Sj; Saftoiu, A; Salamida, F; Salazar, H; Greus, Fs; Salina, G; Sanchez, F; Santo, Ce; Santos, E; Santos, Em; Sarazin, F; Sarkar, B; Sarkar, S; Sato, R; Scharf, N; Scherini, V; Schieler, H; Schiffer, P; Schmidt, A; Scholten, O; Schoorlemmer, H; Schovancova, J; Schovanek, P; Schroder, F; 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[10.1088/1475-7516/2013/05/009]
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande. La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.