On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

A. Achterberg; M. Ackermann; J. Adams; J. Ahrens; D. W. Atlee; J. N. Bahcall; X. Bai; B. Baret; M. Bartelt; S. W. Barwick; R. Bay; K. Beattie; T. Becka; J. K. Becker; K. H. Becker; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; E. Blaufuss; D. J. Boersma; C. Bohm; S. Böser; O. Botner; A. Bouchta; J. Braun; C. Burgess; T. Burgess; T. Castermans; D. Chirkin; J. Clem; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; M. V. D'Agostino; A. Davour; C. T. Day; C. De Clercq; P. Desiati; T. DeYoung; J. Dreyer; M. R. Duvoort; W. R. Edwards; R. Ehrlich; R. W. Ellsworth; P. A. Evenson; A. R. Fazely; T. Feser; K. Filimonov; T. K. Gaisser; J. Gallagher; R. Ganugapati; H. Geenen; L. Gerhardt; A. Goldschmidt; J. A. Goodman; M. G. Greene; S. Grullon; A. Groß; R. M. Gunasingha; A. Hallgren; F. Halzen; K. Han; K. Hanson; D. Hardtke; R. Hardtke; T. Harenberg; J. E. Hart; T. Hauschildt; D. Hays; J. Heise; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; J. Hodges; K. D. Hoffman; K. Hoshina; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; S. Hundertmark; A. Ishihara; J. Jacobsen; G. S. Japaridze; A. Jones; J. M. Joseph; K. H. Kampert; A. Karle; H. Kawai; J. L. Kelley; M. Kestel; N. Kitamura; S. R. Klein; S. Klepser; G. Kohnen; H. Kolanoski; L. Köpke; M. Krasberg; K. Kuehn; H. Landsman; R. Lang; H. Leich; M. Leuthold; I. Liubarsky; J. Lundberg; J. Madsen; K. Mase; H. S. Matis; T. McCauley; C. P. McParland; A. Meli; T. Messarius; P. Mészáros; R. H. Minor; P. Miočinović; H. Miyamoto; A. Mokhtarani; T. Montaruli; A. Morey; R. Morse; S. M. Movit; K. Münich; R. Nahnhauer; J. W. Nam; P. Nießen; D. R. Nygren; H. Ögelman; Ph Olbrechts; A. Olivas; S. Patton; C. Peña-Garay; C. Pérez de los Heros; D. Pieloth; A. C. Pohl; R. Porrata; J. Pretz; P. B. Price; G. T. Przybylski; K. Rawlins; S. Razzaque; F. Refflinghaus; E. Resconi; W. Rhode; M. Ribordy; S. Richter; A. Rizzo; S. Robbins; C. Rott; D. Rutledge; H. G. Sander; S. Schlenstedt; D. Schneider; D. Seckel; S. H. Seo; S. Seunarine; A. Silvestri; A. J. Smith; M. Solarz; C. Song; J. E. Sopher; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; P. Steffen; D. Steele; T. Stezelberger; R. G. Stokstad; M. C. Stoufer; S. Stoyanov; K. H. Sulanke; G. W. Sullivan; T. J. Sumner; I. Taboada; O. Tarasova; A. Tepe; L. Thollander; S. Tilav; P. A. Toale; D. Turčan; N. van Eijndhoven; J. Vandenbroucke; B. Voigt; W. Wagner; C. Walck; H. Waldmann; M. Walter; Y. R. Wang; C. Wendt; C. H. Wiebusch; G. Wikström; D. R. Williams; R. Wischnewski; H. Wissing; K. Woschnagg; X. W. Xu; G. Yodh; S. Yoshida; J. D. Zornoza; P. L. Biermann

doi:10.1016/j.astropartphys.2006.06.012

On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

A. Achterberg, M. Ackermann, J. Adams, J. Ahrens, D. W. Atlee, J. N. Bahcall, X. Bai, B. Baret, M. Bartelt, S. W. Barwick, R. Bay, K. Beattie, T. Becka, J. K. Becker, K. H. Becker, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. BessonE. Blaufuss, D. J. Boersma, C. Bohm, S. Böser, O. Botner, A. Bouchta, J. Braun, C. Burgess, T. Burgess, T. Castermans, D. Chirkin, J. Clem, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, M. V. D'Agostino, A. Davour, C. T. Day, C. De Clercq, P. Desiati, T. DeYoung, J. Dreyer, M. R. Duvoort, W. R. Edwards, R. Ehrlich, R. W. Ellsworth, P. A. Evenson, A. R. Fazely, T. Feser, K. Filimonov, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, J. A. Goodman, M. G. Greene, S. Grullon, A. Groß, R. M. Gunasingha, A. Hallgren, F. Halzen, K. Han, K. Hanson, D. Hardtke, R. Hardtke, T. Harenberg, J. E. Hart, T. Hauschildt, D. Hays, J. Heise, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, K. D. Hoffman, K. Hoshina, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, A. Ishihara, J. Jacobsen, G. S. Japaridze, A. Jones, J. M. Joseph, K. H. Kampert, A. Karle, H. Kawai, J. L. Kelley, M. Kestel, N. Kitamura, S. R. Klein, S. Klepser, G. Kohnen, H. Kolanoski, L. Köpke, M. Krasberg, K. Kuehn, H. Landsman, R. Lang, H. Leich, M. Leuthold, I. Liubarsky, J. Lundberg, J. Madsen, K. Mase, H. S. Matis, T. McCauley, C. P. McParland, A. Meli, T. Messarius, P. Mészáros, R. H. Minor, P. Miočinović, H. Miyamoto, A. Mokhtarani, T. Montaruli, A. Morey, R. Morse, S. M. Movit, K. Münich, R. Nahnhauer, J. W. Nam, P. Nießen, D. R. Nygren, H. Ögelman, Ph Olbrechts, A. Olivas, S. Patton, C. Peña-Garay, C. Pérez de los Heros, D. Pieloth, A. C. Pohl, R. Porrata, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, F. Refflinghaus, E. Resconi, W. Rhode, M. Ribordy, S. Richter, A. Rizzo, S. Robbins, C. Rott, D. Rutledge, H. G. Sander, S. Schlenstedt, D. Schneider, D. Seckel, S. H. Seo, S. Seunarine, A. Silvestri, A. J. Smith, M. Solarz, C. Song, J. E. Sopher, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, P. Steffen, D. Steele, T. Stezelberger, R. G. Stokstad, M. C. Stoufer, S. Stoyanov, K. H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, O. Tarasova, A. Tepe, L. Thollander, S. Tilav, P. A. Toale, D. Turčan, N. van Eijndhoven, J. Vandenbroucke, B. Voigt, W. Wagner, C. Walck, H. Waldmann, M. Walter, Y. R. Wang, C. Wendt, C. H. Wiebusch, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, X. W. Xu, G. Yodh, S. Yoshida, J. D. Zornoza, P. L. Biermann

Research output: Contribution to journal › Article › peer-review

40 Scopus citations

Abstract

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN models, as briefly reviewed in this paper. The source stacking search for neutrinos from generic AGN classes is illustrated using the data collected by the AMANDA-II high-energy neutrino detector during the year 2000. No significant excess for any of the suggested groups was found.

Original language	English (US)
Pages (from-to)	282-300
Number of pages	19
Journal	Astroparticle Physics
Volume	26
Issue number	4-5
DOIs	https://doi.org/10.1016/j.astropartphys.2006.06.012
State	Published - Nov 2006

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics

Access to Document

10.1016/j.astropartphys.2006.06.012

Cite this

Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Atlee, D. W., Bahcall, J. N., Bai, X., Baret, B., Bartelt, M., Barwick, S. W., Bay, R., Beattie, K., Becka, T., Becker, J. K., Becker, K. H., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., ... Biermann, P. L. (2006). On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes. Astroparticle Physics, 26(4-5), 282-300. https://doi.org/10.1016/j.astropartphys.2006.06.012

@article{6c8519617c6b402dac4698ce8b4ec844,

title = "On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes",

abstract = "The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN models, as briefly reviewed in this paper. The source stacking search for neutrinos from generic AGN classes is illustrated using the data collected by the AMANDA-II high-energy neutrino detector during the year 2000. No significant excess for any of the suggested groups was found.",

author = "A. Achterberg and M. Ackermann and J. Adams and J. Ahrens and Atlee, {D. W.} and Bahcall, {J. N.} and X. Bai and B. Baret and M. Bartelt and Barwick, {S. W.} and R. Bay and K. Beattie and T. Becka and Becker, {J. K.} and Becker, {K. H.} and P. Berghaus and D. Berley and E. Bernardini and D. Bertrand and Besson, {D. Z.} and E. Blaufuss and Boersma, {D. J.} and C. Bohm and S. B{\"o}ser and O. Botner and A. Bouchta and J. Braun and C. Burgess and T. Burgess and T. Castermans and D. Chirkin and J. Clem and B. Collin and J. Conrad and J. Cooley and Cowen, {D. F.} and D'Agostino, {M. V.} and A. Davour and Day, {C. T.} and {De Clercq}, C. and P. Desiati and T. DeYoung and J. Dreyer and Duvoort, {M. R.} and Edwards, {W. R.} and R. Ehrlich and Ellsworth, {R. W.} and Evenson, {P. A.} and Fazely, {A. R.} and T. Feser and K. Filimonov and Gaisser, {T. K.} and J. Gallagher and R. Ganugapati and H. Geenen and L. Gerhardt and A. Goldschmidt and Goodman, {J. A.} and Greene, {M. G.} and S. Grullon and A. Gro{\ss} and Gunasingha, {R. M.} and A. Hallgren and F. Halzen and K. Han and K. Hanson and D. Hardtke and R. Hardtke and T. Harenberg and Hart, {J. E.} and T. Hauschildt and D. Hays and J. Heise and K. Helbing and M. Hellwig and P. Herquet and Hill, {G. C.} and J. Hodges and Hoffman, {K. D.} and K. Hoshina and D. Hubert and B. Hughey and Hulth, {P. O.} and K. Hultqvist and S. Hundertmark and A. Ishihara and J. Jacobsen and Japaridze, {G. S.} and A. Jones and Joseph, {J. M.} and Kampert, {K. H.} and A. Karle and H. Kawai and Kelley, {J. L.} and M. Kestel and N. Kitamura and Klein, {S. R.} and S. Klepser and G. Kohnen and H. Kolanoski and L. K{\"o}pke and M. Krasberg and K. Kuehn and H. Landsman and R. Lang and H. Leich and M. Leuthold and I. Liubarsky and J. Lundberg and J. Madsen and K. Mase and Matis, {H. S.} and T. McCauley and McParland, {C. P.} and A. Meli and T. Messarius and P. M{\'e}sz{\'a}ros and Minor, {R. H.} and P. Mio{\v c}inovi{\'c} and H. Miyamoto and A. Mokhtarani and T. Montaruli and A. Morey and R. Morse and Movit, {S. M.} and K. M{\"u}nich and R. Nahnhauer and Nam, {J. W.} and P. Nie{\ss}en and Nygren, {D. R.} and H. {\"O}gelman and Ph Olbrechts and A. Olivas and S. Patton and C. Pe{\~n}a-Garay and {P{\'e}rez de los Heros}, C. and D. Pieloth and Pohl, {A. C.} and R. Porrata and J. Pretz and Price, {P. B.} and Przybylski, {G. T.} and K. Rawlins and S. Razzaque and F. Refflinghaus and E. Resconi and W. Rhode and M. Ribordy and S. Richter and A. Rizzo and S. Robbins and C. Rott and D. Rutledge and Sander, {H. G.} and S. Schlenstedt and D. Schneider and D. Seckel and Seo, {S. H.} and S. Seunarine and A. Silvestri and Smith, {A. J.} and M. Solarz and C. Song and Sopher, {J. E.} and Spiczak, {G. M.} and C. Spiering and M. Stamatikos and T. Stanev and P. Steffen and D. Steele and T. Stezelberger and Stokstad, {R. G.} and Stoufer, {M. C.} and S. Stoyanov and Sulanke, {K. H.} and Sullivan, {G. W.} and Sumner, {T. J.} and I. Taboada and O. Tarasova and A. Tepe and L. Thollander and S. Tilav and Toale, {P. A.} and D. Tur{\v c}an and {van Eijndhoven}, N. and J. Vandenbroucke and B. Voigt and W. Wagner and C. Walck and H. Waldmann and M. Walter and Wang, {Y. R.} and C. Wendt and Wiebusch, {C. H.} and G. Wikstr{\"o}m and Williams, {D. R.} and R. Wischnewski and H. Wissing and K. Woschnagg and Xu, {X. W.} and G. Yodh and S. Yoshida and Zornoza, {J. D.} and Biermann, {P. L.}",

note = "Funding Information: We acknowledge the support from the following agencies: National Science Foundation-Office of Polar Program, National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, Department of Energy, and National Energy Research Scientific Computing Center (supported by the Office of Energy Research of the Department of Energy), the NSF-supported TeraGrid system at the San Diego Supercomputer Center (SDSC), and the National Center for Supercomputing Applications (NCSA); Swedish Research Council, Swedish Polar Research Secretariat, and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research, Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Office for Scientific, Technical and Cultural affairs (OSTC); the Netherlands Organisation for Scientific Research (NWO); M. Ribordy acknowledges the support of the SNF (Switzerland); J.D. Zornoza acknowledges the Marie Curie OIF Program (contract 007921). ",

year = "2006",

month = nov,

doi = "10.1016/j.astropartphys.2006.06.012",

language = "English (US)",

volume = "26",

pages = "282--300",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "4-5",

}

Achterberg, A, Ackermann, M, Adams, J, Ahrens, J, Atlee, DW, Bahcall, JN, Bai, X, Baret, B, Bartelt, M, Barwick, SW, Bay, R, Beattie, K, Becka, T, Becker, JK, Becker, KH, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, DZ, Blaufuss, E, Boersma, DJ, Bohm, C, Böser, S, Botner, O, Bouchta, A, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Clem, J, Collin, B, Conrad, J, Cooley, J, Cowen, DF, D'Agostino, MV, Davour, A, Day, CT, De Clercq, C, Desiati, P, DeYoung, T, Dreyer, J, Duvoort, MR, Edwards, WR, Ehrlich, R, Ellsworth, RW, Evenson, PA, Fazely, AR, Feser, T, Filimonov, K, Gaisser, TK, Gallagher, J, Ganugapati, R, Geenen, H, Gerhardt, L, Goldschmidt, A, Goodman, JA, Greene, MG, Grullon, S, Groß, A, Gunasingha, RM, Hallgren, A, Halzen, F, Han, K, Hanson, K, Hardtke, D, Hardtke, R, Harenberg, T, Hart, JE, Hauschildt, T, Hays, D, Heise, J, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hodges, J, Hoffman, KD, Hoshina, K, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Ishihara, A, Jacobsen, J, Japaridze, GS, Jones, A, Joseph, JM, Kampert, KH, Karle, A, Kawai, H, Kelley, JL, Kestel, M, Kitamura, N, Klein, SR, Klepser, S, Kohnen, G, Kolanoski, H, Köpke, L, Krasberg, M, Kuehn, K, Landsman, H, Lang, R, Leich, H, Leuthold, M, Liubarsky, I, Lundberg, J, Madsen, J, Mase, K, Matis, HS, McCauley, T, McParland, CP, Meli, A, Messarius, T, Mészáros, P, Minor, RH, Miočinović, P, Miyamoto, H, Mokhtarani, A, Montaruli, T, Morey, A, Morse, R, Movit, SM, Münich, K, Nahnhauer, R, Nam, JW, Nießen, P, Nygren, DR, Ögelman, H, Olbrechts, P, Olivas, A, Patton, S, Peña-Garay, C, Pérez de los Heros, C, Pieloth, D, Pohl, AC, Porrata, R, Pretz, J, Price, PB, Przybylski, GT, Rawlins, K, Razzaque, S, Refflinghaus, F, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Rizzo, A, Robbins, S, Rott, C, Rutledge, D, Sander, HG, Schlenstedt, S, Schneider, D, Seckel, D, Seo, SH, Seunarine, S, Silvestri, A, Smith, AJ, Solarz, M, Song, C, Sopher, JE, Spiczak, GM, Spiering, C, Stamatikos, M, Stanev, T, Steffen, P, Steele, D, Stezelberger, T, Stokstad, RG, Stoufer, MC, Stoyanov, S, Sulanke, KH, Sullivan, GW, Sumner, TJ, Taboada, I, Tarasova, O, Tepe, A, Thollander, L, Tilav, S, Toale, PA, Turčan, D, van Eijndhoven, N, Vandenbroucke, J, Voigt, B, Wagner, W, Walck, C, Waldmann, H, Walter, M, Wang, YR, Wendt, C, Wiebusch, CH, Wikström, G, Williams, DR, Wischnewski, R, Wissing, H, Woschnagg, K, Xu, XW, Yodh, G, Yoshida, S, Zornoza, JD & Biermann, PL 2006, 'On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes', Astroparticle Physics, vol. 26, no. 4-5, pp. 282-300. https://doi.org/10.1016/j.astropartphys.2006.06.012

TY - JOUR

T1 - On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

AU - Achterberg, A.

AU - Ackermann, M.

AU - Adams, J.

AU - Ahrens, J.

AU - Atlee, D. W.

AU - Bahcall, J. N.

AU - Bai, X.

AU - Baret, B.

AU - Bartelt, M.

AU - Barwick, S. W.

AU - Bay, R.

AU - Beattie, K.

AU - Becka, T.

AU - Becker, J. K.

AU - Becker, K. H.

AU - Berghaus, P.

AU - Berley, D.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Besson, D. Z.

AU - Blaufuss, E.

AU - Boersma, D. J.

AU - Bohm, C.

AU - Böser, S.

AU - Botner, O.

AU - Bouchta, A.

AU - Braun, J.

AU - Burgess, C.

AU - Burgess, T.

AU - Castermans, T.

AU - Chirkin, D.

AU - Clem, J.

AU - Collin, B.

AU - Conrad, J.

AU - Cooley, J.

AU - Cowen, D. F.

AU - D'Agostino, M. V.

AU - Davour, A.

AU - Day, C. T.

AU - De Clercq, C.

AU - Desiati, P.

AU - DeYoung, T.

AU - Dreyer, J.

AU - Duvoort, M. R.

AU - Edwards, W. R.

AU - Ehrlich, R.

AU - Ellsworth, R. W.

AU - Evenson, P. A.

AU - Fazely, A. R.

AU - Feser, T.

AU - Filimonov, K.

AU - Gaisser, T. K.

AU - Gallagher, J.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Gerhardt, L.

AU - Goldschmidt, A.

AU - Goodman, J. A.

AU - Greene, M. G.

AU - Grullon, S.

AU - Groß, A.

AU - Gunasingha, R. M.

AU - Hallgren, A.

AU - Halzen, F.

AU - Han, K.

AU - Hanson, K.

AU - Hardtke, D.

AU - Hardtke, R.

AU - Harenberg, T.

AU - Hart, J. E.

AU - Hauschildt, T.

AU - Hays, D.

AU - Heise, J.

AU - Helbing, K.

AU - Hellwig, M.

AU - Herquet, P.

AU - Hill, G. C.

AU - Hodges, J.

AU - Hoffman, K. D.

AU - Hoshina, K.

AU - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, S.

AU - Ishihara, A.

AU - Jacobsen, J.

AU - Japaridze, G. S.

AU - Jones, A.

AU - Joseph, J. M.

AU - Kampert, K. H.

AU - Karle, A.

AU - Kawai, H.

AU - Kelley, J. L.

AU - Kestel, M.

AU - Kitamura, N.

AU - Klein, S. R.

AU - Klepser, S.

AU - Kohnen, G.

AU - Kolanoski, H.

AU - Köpke, L.

AU - Krasberg, M.

AU - Kuehn, K.

AU - Landsman, H.

AU - Lang, R.

AU - Leich, H.

AU - Leuthold, M.

AU - Liubarsky, I.

AU - Lundberg, J.

AU - Madsen, J.

AU - Mase, K.

AU - Matis, H. S.

AU - McCauley, T.

AU - McParland, C. P.

AU - Meli, A.

AU - Messarius, T.

AU - Mészáros, P.

AU - Minor, R. H.

AU - Miočinović, P.

AU - Miyamoto, H.

AU - Mokhtarani, A.

AU - Montaruli, T.

AU - Morey, A.

AU - Morse, R.

AU - Movit, S. M.

AU - Münich, K.

AU - Nahnhauer, R.

AU - Nam, J. W.

AU - Nießen, P.

AU - Nygren, D. R.

AU - Ögelman, H.

AU - Olbrechts, Ph

AU - Olivas, A.

AU - Patton, S.

AU - Peña-Garay, C.

AU - Pérez de los Heros, C.

AU - Pieloth, D.

AU - Pohl, A. C.

AU - Porrata, R.

AU - Pretz, J.

AU - Price, P. B.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Razzaque, S.

AU - Refflinghaus, F.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Richter, S.

AU - Rizzo, A.

AU - Robbins, S.

AU - Rott, C.

AU - Rutledge, D.

AU - Sander, H. G.

AU - Schlenstedt, S.

AU - Schneider, D.

AU - Seckel, D.

AU - Seo, S. H.

AU - Seunarine, S.

AU - Silvestri, A.

AU - Smith, A. J.

AU - Solarz, M.

AU - Song, C.

AU - Sopher, J. E.

AU - Spiczak, G. M.

AU - Spiering, C.

AU - Stamatikos, M.

AU - Stanev, T.

AU - Steffen, P.

AU - Steele, D.

AU - Stezelberger, T.

AU - Stokstad, R. G.

AU - Stoufer, M. C.

AU - Stoyanov, S.

AU - Sulanke, K. H.

AU - Sullivan, G. W.

AU - Sumner, T. J.

AU - Taboada, I.

AU - Tarasova, O.

AU - Tepe, A.

AU - Thollander, L.

AU - Tilav, S.

AU - Toale, P. A.

AU - Turčan, D.

AU - van Eijndhoven, N.

AU - Vandenbroucke, J.

AU - Voigt, B.

AU - Wagner, W.

AU - Walck, C.

AU - Waldmann, H.

AU - Walter, M.

AU - Wang, Y. R.

AU - Wendt, C.

AU - Wiebusch, C. H.

AU - Wikström, G.

AU - Williams, D. R.

AU - Wischnewski, R.

AU - Wissing, H.

AU - Woschnagg, K.

AU - Xu, X. W.

AU - Yodh, G.

AU - Yoshida, S.

AU - Zornoza, J. D.

AU - Biermann, P. L.

N1 - Funding Information: We acknowledge the support from the following agencies: National Science Foundation-Office of Polar Program, National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, Department of Energy, and National Energy Research Scientific Computing Center (supported by the Office of Energy Research of the Department of Energy), the NSF-supported TeraGrid system at the San Diego Supercomputer Center (SDSC), and the National Center for Supercomputing Applications (NCSA); Swedish Research Council, Swedish Polar Research Secretariat, and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research, Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Office for Scientific, Technical and Cultural affairs (OSTC); the Netherlands Organisation for Scientific Research (NWO); M. Ribordy acknowledges the support of the SNF (Switzerland); J.D. Zornoza acknowledges the Marie Curie OIF Program (contract 007921).

PY - 2006/11

Y1 - 2006/11

N2 - The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN models, as briefly reviewed in this paper. The source stacking search for neutrinos from generic AGN classes is illustrated using the data collected by the AMANDA-II high-energy neutrino detector during the year 2000. No significant excess for any of the suggested groups was found.

AB - The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN models, as briefly reviewed in this paper. The source stacking search for neutrinos from generic AGN classes is illustrated using the data collected by the AMANDA-II high-energy neutrino detector during the year 2000. No significant excess for any of the suggested groups was found.

UR - http://www.scopus.com/inward/record.url?scp=33750466183&partnerID=8YFLogxK

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U2 - 10.1016/j.astropartphys.2006.06.012

DO - 10.1016/j.astropartphys.2006.06.012

M3 - Article

AN - SCOPUS:33750466183

SN - 0927-6505

VL - 26

SP - 282

EP - 300

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 4-5

ER -

On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

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