Sökning: onr:"swepub:oai:DiVA.org:uu-23035" > On the selection of...
Fältnamn | Indikatorer | Metadata |
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000 | 03626naa a2200601 4500 | |
001 | oai:DiVA.org:uu-23035 | |
003 | SwePub | |
008 | 070124s2006 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:lnu-1570 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-230352 URI |
024 | 7 | a https://doi.org/10.1016/j.astropartphys.2006.06.0122 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-15702 URI |
040 | a (SwePub)uud (SwePub)lnu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Achterberg, A.4 aut |
245 | 1 0 | a On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes |
264 | 1 | b Elsevier BV,c 2006 |
338 | a print2 rdacarrier | |
520 | a 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 highenergy neutrino detector during the year 2000. No significant excess for any of the suggested groups was found. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
653 | a neutrinos | |
653 | a AGN | |
653 | a source stacking | |
653 | a point sources | |
653 | a AMANDA | |
653 | a IceCube | |
653 | a Physics | |
653 | a Fysik | |
653 | a Astroparticle physics | |
653 | a Astroparticle Physics | |
700 | 1 | a Botner, Olgau Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Bouchta, Adamu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Conrad, Janu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Davour, Annau Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Hallgren, Allanu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Lundberg, Johanu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Marciniewski, Pawelu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Pérez de los Heros, Carlosu Uppsala universitet,Högenergifysik4 aut0 (Swepub:uu)capedlhe |
700 | 1 | a Biermann, P.L.4 aut |
700 | 1 | a IceCube Collaboration, -4 aut |
700 | 1 | a Pohl, Arvidu Högskolan i Kalmar,Naturvetenskapliga institutionen4 aut0 (Swepub:lnu)tpoar |
710 | 2 | a Uppsala universitetb Högenergifysik4 org |
773 | 0 | t Astroparticle physicsd : Elsevier BVg 26:4-5, s. 282-300q 26:4-5<282-300x 0927-6505x 1873-2852 |
856 | 4 | u http://arxiv.org/pdf/astro-ph/0609534 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-23035 |
856 | 4 8 | u https://doi.org/10.1016/j.astropartphys.2006.06.012 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-1570 |
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