Title
Searches for periodic neutrino emission from binary systems with 22 and 40 strings of IceCube
Date Issued
01 April 2012
Access level
open access
Resource Type
journal article
Author(s)
Abbasi R.
Abdou Y.
Abu-Zayyad T.
Ackermann M.
Adams J.
Aguilar J.A.
Ahlers M.
Allen M.M.
Altmann D.
Andeen K.
Auffenberg J.
Bai X.
Baker M.
Barwick S.W.
Bay R.
Beattie K.
Beatty J.J.
Bechet S.
Becker J.K.
Becker K.H.
Benabderrahmane M.L.
Benzvi S.
Berdermann J.
Berghaus P.
Berley D.
Bernardini E.
Bertrand D.
Besson D.Z.
Bindig D.
Bissok M.
Blaufuss E.
Blumenthal J.
Boersma D.J.
Bohm C.
Bose D.
Böser S.
Botner O.
Brown A.M.
Buitink S.
Caballero-Mora K.S.
Carson M.
Chirkin D.
Christy B.
Clevermann F.
Cohen S.
Colnard C.
Cowen D.F.
Cruz Silva A.H.
D'Agostino M.V.
Danninger M.
Daughhetee J.
Davis J.C.
De Clercq C.
Degner T.
Demirörs L.
Descamps F.
Desiati P.
De Vries-Uiterweerd G.
Deyoung T.
Díaz-Vélez J.C.
Dierckxsens M.
Dreyer J.
Dumm J.P.
Dunkman M.
Eisch J.
Ellsworth R.W.
Engdegrd O.
Euler S.
Evenson P.A.
Fadiran O.
Fazely A.R.
Fedynitch A.
Feintzeig J.
Feusels T.
Filimonov K.
Finley C.
Fischer-Wasels T.
Fox B.D.
Franckowiak A.
Franke R.
Gaisser T.K.
Gallagher J.
Gerhardt L.
Gladstone L.
Glüsenkamp T.
Goldschmidt A.
Goodman J.A.
Góra D.
Grant D.
Griesel T.
Gro A.
Grullon S.
Gurtner M.
Ha C.
Haj Ismail A.
Hallgren A.
Halzen F.
Han K.
Hanson K.
Deutsches Elektronen Synchrotron
Publisher(s)
Institute of Physics Publishing
Abstract
In this paper, we present the results of searches for periodic neutrino emission from a catalog of binary systems. Such modulation, observed in the photon flux, would be caused by the geometry of these systems. In the analysis, the period is fixed by these photon observations, while the phase and duration of the neutrino emission are treated as free parameters to be fit with the data. If the emission occurs during 20% or less of the total period, this analysis achieves better sensitivity than a time-integrated analysis. We use the IceCube data taken from 2007 May 31 to 2008 April 5 with its 22 string configuration and from 2008 April 5 to 2009 May 20 with its 40 string configuration. No evidence for neutrino emission is found, with the strongest excess occurring for CygnusX-3 at 2.1σ significance after accounting for trials. Neutrino flux upper limits for both periodic and time-integrated emission are provided. © 2012. The American Astronomical Society. All rights reserved.
Volume
748
Issue
2
Language
English
OCDE Knowledge area
Física de partículas, Campos de la Física Astronomía
Scopus EID
2-s2.0-84863351703
Source
Astrophysical Journal
ISSN of the container
0004637X
Sponsor(s)
National Science Foundation - 0969661 Science and Technology Facilities Council - ST/J000507/1 Japan Society for the Promotion of Science - 10J40081 Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung - 133630
Sources of information: Directorio de Producción Científica Scopus