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863 results on '"Bahcall, J. N."'

1. Is Large Mixing Angle MSW the Solution of the Solar Neutrino Problems?

Author

Bahcall, J. N., Krastev, P. I., and Smirnov, A. Yu.

Subjects
High Energy Physics - Phenomenology, Astrophysics, High Energy Physics - Experiment, Nuclear Theory
Abstract

Recent results on solar neutrinos provide hints that the LMA MSW solution could be correct. We perform accurate calculations for potential `smoking-gun' effects of the LMA solution in the SuperKamiokande solar neutrino experiment, including: (1) an almost constant reduction of the standard recoil electron energy spectrum (with a weak, < 10%, relative increase below 6.5 MeV); (2) an integrated difference in day-night rates (2% to 14%); (3) an approximately constant zenith-angle dependence of the nighttime event rate; (4) a new test for the difference in the shape of the equally-normalized day-night energy spectra (~ 1%); and (5) annual variations of the signal due to the regeneration effect (~ 6 times smaller than the integrated day-night effect). We also establish a relation between the integrated day-night asymmetry and the seasonal asymmetry due to LMA regeneration. As a cautionary example, we simulate the effect of an absolute energy calibration error on the shape (distortion) of the recoil energy spectrum. We compare LMA predictions with SuperKamiokande data and discuss the possibilities for distinguishing experimentally between LMA and vacuum oscillations., Comment: Added Fig. 1 showing LMA allowed region. Editorial changes. Accepted Phys Rev D. Related information: http://www.sns.ias.edu/~jnb

Published
1999
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2. Where do we stand with solar neutrino oscillations?

Author

Bahcall, J. N., Krastev, P. I., and Smirnov, A. Yu.

Subjects
High Energy Physics - Phenomenology, Astrophysics, High Energy Physics - Experiment, Nuclear Experiment
Abstract

We determine the neutrino parameters for MSW and vacuum oscillations (active and sterile neutrinos) that are allowed by the separate, and collective, imposition of the constraints from total event rates in the chlorine, GALLEX, SAGE, and SuperKamiokande experiments (504 days), the SuperKamiokande electron energy spectrum, and the SuperKamiokande zenith-angle dependence. The small mixing angle MSW solution is acceptable at the 7% C.L. (8% for sterile nu's) and the vacuum solution is acceptable at the 6% C.L. . The best-fit global MSW solution for active neutrinos is: Delta m^2 = 5 x 10^-6 eV^2, sin^2 (2 theta) = 5.5 x 10^{-3} (and for sterile neutrinos: Delta m^2 = 4 x 10^-6 eV^2, sin^2 (2 theta) = 7 x 10^-3). For vacuum oscillations, the best-fit solution is: Delta m^2 = 6.5 x 10^-11 eV^2, sin^2 (2 theta) = 0.75 . An arbitrary combination of undistorted (no oscillations) pp, 7Be, 8B, and CNO neutrino fluxes is inconsistent with the combined data sets at the 3.5 sigma C.L., independent of astrophysical considerations. We use improved calculations of solar model fluxes, neutrino absorption cross sections and energy spectra, and a detailed evaluation of regeneration effects., Comment: LaTeX file. Added Figure comparing with SuperK spectrum. Predictions for LENS experiment. Viewgraphs and related information at http://www.sns.ias.edu/~jnb

Published
1998
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3. Does the Sun Appear Brighter at Night in Neutrinos?

Author

Bahcall, J. N. and Krastev, P. I.

Subjects
High Energy Physics - Phenomenology, Astrophysics, Nuclear Theory
Abstract

We calculate accurately the number of solar neutrino events expected as a function of solar zenith angle, with and without neutrino oscillations, for detectors at the locations of Super-Kamiokande, SNO, and the Gran Sasso National Laboratory. Using different earth models to estimate geophysical uncertainties, and different solar models to estimate solar uncertainties, we evaluate distortions predicted by the MSW effect in the zenith angle distributions of solar neutrino events. The distortions are caused by oscillations and by $\nu-e$ interactions in the earth that regenerate $\nu_e$ from $\nu_\mu$ or $\nu_\tau$. We show that the first two moments of the zenith-angle distribution are more sensitive to the small mixing angle MSW solution than the conventionally studied day-night asymmetry. We present iso-sigma contours that illustrate the potential of Super-Kamiokande, SNO, BOREXINO, ICARUS and HERON/HELLAZ for detecting the earth regeneration effect at their actual locations (and at the equator). MSW solutions favored by the four pioneering solar neutrino experiments predict characteristic distortions for Super-Kamiokande, SNO, BOREXINO, and ICARUS that range from being unmeasurably small to $> 5\sigma$ (stat) after only a few years of observations., Comment: 49 pages, 16 figures, uses REVTEX, Seven exportable viewgraphs based upon paper are available at this http URL, where the table of solar zenith-angle distributions can also be found

Published
1997
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4. FCNC Solutions to the Solar Neutrino Problem

Author

Krastev, P. I. and Bahcall, J. N.

Subjects
High Energy Physics - Phenomenology
Abstract

We present the status of FCNC solutions to the solar neutrino problem. Our analysis shows that the FCNC solutions with massless neutrinos provide a good fit to the latest solar neutrino data. Predictions for future experiments are formulated which will permit further tests of these solutions., Comment: 5 pages, talk given by P. Krastev at the first symposium of FCNC, February 19-21, 1997, Santa Monica, organized by UCLA

Published
1997

5. The HST Quasar Absorption Line Key Project XII. The Unusual Absorption Line System in the Spectrum of PG 2302+029 ---Ejected or Intervening?

Author

Jannuzi, B. T., Hartig, G. F., Kirhakos, S., Sargent, W. L. W., Turnshek, D. A., Weymann, R. J., Bahcall, J. N., Bergeron, J., Boksenberg, A., Savage, B. D., Schneider, D. P., and Wolfe, A. M.

Subjects
Astrophysics
Abstract

We report the discovery of a high-ionization broad absorption line system at a redshift of z_abs=0.695 in the spectrum of the z_em=1.052 radio-quiet quasar PG 2302+039. Broad absorption with FWHM from 3,000 to 5,000 km/s is detected from C IV, N V, and O VI in HST Faint Object Spectrograph spectra of the quasar. A narrow line system (FWHM approximately 250 km/s) at z_abs=0.7016 is resolved from the broad blend and includes absorption by Ly-alpha and the C IV, N V, and O VI doublets. No absorption by low-ionization metal species (e.g. Si II and Mg II) is detected in the HST or ground-based spectra for either the broad or the narrow system. The centroids of the broad system lines are displaced by approximately 56,000 km/s to the blue of the quasar's broad emission lines. The reddest extent of the broad line absorption is more than 50,000 km/s from the quasar. The properties of this system are unprecedented whether it is an intervening or an ejected system., Comment: 9 pages, LaTeX file, two postscript figures. Accepted for publication in The Astrophysical Journal Letters. Changes include removing TeX macros from abstract

Published
1996
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6. What Can Be Learned by Measuring the Fluxes of the 7-Be and the pep Solar Neutrino Lines?

Author

Bahcall, J. N. and Krastev, P. I.

Subjects
Astrophysics, High Energy Physics - Phenomenology, Nuclear Experiment, Nuclear Theory
Abstract

Measurements of the interaction rates of the solar neutrino lines of $^7$Be and $pep$ can be used, independent of solar models, to test whether electron flavor is conserved, to determine survival probabilities of electron-type neutrinos at specific energies, and to test for the existence of sterile neutrinos. We present analytic descriptions of these tests. We also illustrate by numerical simulations, assuming matter-enhanced and vacuum neutrino oscillations, what measurements of solar neutrino lines can teach us about neutrino masses and mixing angles., Comment: 34 pages, RevTeX file. New and better quality figures. Submitted to Physical Review D

Published
1996
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7. How Does the Sun Shine?

Author

Bahcall, J. N., Fukugita, M., and Krastev, P. I.

Subjects
Astrophysics, High Energy Physics - Phenomenology, Nuclear Experiment, Nuclear Theory
Abstract

Assuming that MSW neutrino oscillations occur and ignoring all solar physics except for the constraint that nuclear fusion produces the solar luminosity, we show that new solar neutrino experiments are required to rule out empirically the hypothesis that the sun shines via the CNO cycle., Comment: 15 pages (RevTeX) + 2 figures (postscript), uuencoded gz-compressed tar file including text+figures. Postscript file also available at http://www.sns.ias.edu/~jnb/preprints.html Accepted for publication in Physics Letters B

Published
1996
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8. How Well Do We (and Will We) Know Solar Neutrino Fluxes and Oscillation Parameters?

Author

Bahcall, J. N. and Krastev, P. I.

Subjects
High Energy Physics - Phenomenology
Abstract

Assuming neutrino oscillations occur, the pp electron neutrino flux is uncertain by at least a factor of two, the ${\rm ^8B}$ flux by a factor of five, and the ${\rm ^7Be}$ flux by a factor of forty-five. Calculations of the expected results of future solar neutrino experiments (SuperKamiokande, SNO, BOREXINO, ICARUS, HELLAZ, and HERON) are used to illustrate the extent to which these experiments will restrict the range of the allowed neutrino mixing parameters. We present an improved formulation of the ``luminosity constraint'' and show that at 95\% confidence limit this constraint establishes the best available limits on the rate of creation of pp neutrinos in the solar interior and provides the best upper limit to the ${\rm ^7Be}$ neutrino flux., Comment: 37 pages, uuencoded Z-compressed postscript file (with figures); Submitted to Physical Review D

Published
1995
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9. HST and MERLIN Observations of the Jet in 3C273

Author

Bahcall, J. N., Kirhakos, S., Schneider, D. P., Davis, R. J., Muxlow, T. W. B., Garrington, S. T., Conway, R. G., and Unwin, S. C.

Subjects
Astrophysics
Abstract

We present red and blue images of the jet of the quasar 3C273 obtained with the WFPC2 on the Hubble Space Telescope as well as a new radio map made with the MERLIN array. The images are of significantly better quality than that of previous data. The two maps are aligned to an accuracy of 0.020$''$; this accuracy is achieved because both the quasar and the jet are contained in both the radio and optical images. The start of the optical jet is marked by an elongated knot which appears identical at radio and optical wavelengths. Other knots in the optical jet correspond to narrow oblique features within the radio outline. The total width of the smooth emission in the optical jet is~$0.7''$; the FWHM of the optical knots is~$0.3''$. The knots may trace the current location of a narrow, perhaps helical jet lying within the outlines of the older radio cocoon., Comment: 9 pages, uuencoded postscript file, three postscript figures are available by anonymous ftp to ftp://eku.sns.ias.edu/pub/best/ as 3c273fig1.ps, 3c273fig2.ps, 3c273fig3.ps. To appear in ApJ Letters, October 1995

Published
1995
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10. PKS 2349$-$014: A LUMINOUS QUASAR WITH THIN WISPS, A LARGE OFF-CENTER NEBULOSITY, AND A CLOSE COMPANION GALAXY

Author

Bahcall, J. N., Kirhakos, Sofia, and Schneider, D. P.

Subjects
Astrophysics
Abstract

HST images (WFC2) of \pks show that this luminous nearby quasar is interacting with diffuse (presumably galactic) material. Two thin wisps that have a total extent of about 20 kpc (for $H_0 = 100$ \kms ${\rm Mpc}^{-1}$ and $\Omega_0 = 1.0$) are observed to approximately surround the quasar. One of the wisps appears to pass through a companion galaxy that is located at a projected distance of three~kpc from the center of the quasar light. The companion galaxy, if located at the distance of \pks, has an intrinsic size and luminosity similar to the Large Magellanic Cloud. A faint extended nebulosity, which is detected over a region of 35 kpc by 50 kpc and is centered about 5 kpc from the quasar nucleus, overlaps the wisps. The immediate environment of \pks is different from the enivronments of the other eight luminous quasars that we have studied previously with HST. If the multiple light components of the HST images are fit to a single de~Vaucouleurs profile, as was done in previous analyses of ground--based data, then the result obtained for the total luminosity of the model galaxy is in agreement with the earlier ground-based studies., Comment: Submitted to ApJ Letters, uuencoded postscript file, three postscript figures are available anonymous ftp at ftp://eku.ias.edu/pub/best/ as pks2349fig1.ps, pks2349fig2.ps, and pks2349fig3.ps

Published
1995
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11. Limits on Electron-Neutrino Oscillations from the GALLEX $^{51}$Cr Source Experiment

Author

Bahcall, J. N., Krastev, P. I., and Lisi, E.

Subjects
High Energy Physics - Phenomenology
Abstract

The recent result from the chromium source experiment carried out by the GALLEX collaboration implies interesting limits on the parameters $\Delta m^2$ and $\sin^22\theta$ describing neutrino oscillations. Values of $\Delta m^2~>~0.17$ eV$^2$ for maximal mixing and of $\sin^22\theta > 0.38$ for $\Delta m^2 > 1$~eV$^2$ are ruled out at 90\% C.L. This result improves by more than an order of magnitude previous limits on $\Delta m^2$ derived from electron-neutrino oscillation experiments at accelerators., Comment: 6 pages (REVTEX) + one figure (postscript), all in uuencoded format

Published
1994
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12. Solar Neutrinos and the Principle of Equivalence

Author

Bahcall, J. N, Krastev, P. I., and Leung, C. N.

Subjects
High Energy Physics - Phenomenology, Astrophysics, General Relativity and Quantum Cosmology
Abstract

We study the proposed solution of the solar neutrino problem which requires a flavor nondiagonal coupling of neutrinos to gravity. We adopt a phenomenological point of view and investigate the consequences of the hypothesis that the neutrino weak interaction eigenstates are linear combinations of the gravitational eigenstates which have slightly different couplings to gravity, $f_1G$ and $f_2G$, $|f_1-f_2| << 1$, corresponding to a difference in red-shift between electron and muon neutrinos, $\Delta z/(1+z) \sim |f_1 - f_2|$. We perform a $\chi^2$ analysis of the latest available solar neutrino data and obtain the allowed regions in the space of the relevant parameters. The existing data rule out most of the parameter space which can be probed in solar neutrino experiments, allowing only $|f_1 - f_2| \sim 3 \times 10^{-14}$ for small values of the mixing angle ($2 \times 10^{-3} \le \sin^2(2\theta_G) \le 10^{-2}$) and $10^{-16} \stackrel{<}{\sim} |f_1 - f_2| \stackrel{<}{\sim}10^{-15}$ for large mixing ($0.6 \le \sin^2(2\theta_G) \le 0.9$). Measurements of the $^8{\rm B}$-neutrino energy spectrum in the SNO and Super-Kamiokande experiments will provide stronger constraints independent of all considerations related to solar models. We show that these measurements will be able to exclude part of the allowed region as well as to distinguish between conventional oscillations and oscillations due to the violation of the equivalence principle., Comment: 20 pages + 4 figures, IASSNS-AST 94/54

Published
1994
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13. Proposed Solar-Neutrino Experiment Using 7lGa

Author

Bahcall, J. N., primary, Cleveland, B. T., additional, Davis, R., additional, Dostrovsky, L., additional, Evans, J. C., additional, Frati, W., additional, Friedlander, G., additional, Lande, K., additional, Rowley, J. K., additional, Stoenner, R. W., additional, and Weneser, J., additional

Published
2018
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25. A Very Large Array search for emission from HI associated with nearby Lyman alpha absorbers

Author

Van Gorkom, J. H, Bahcall, J. N, Jannuzi, B. T, and Schneider, D. P

Subjects
Astronomy
Abstract

We present a sensitive Very Large Array (VLA) search for H I emission from the vicinity of the Lyman alpha clouds in the Virgo Cluster, which were recently discovered with Hubble Space Telescope (HST) in absorption toward the nearest quasar 3C273. We searched an area of 40 by 40 arcmin centered on 3C273, covering a velocity range from 840 to 1840 km/s. The bandpass was self-calibrated on 3C273 leading to a spectral dynamic range of better than 10(exp 5) to 1. No H I was detected. The rms noise in the final images corresponds to a 3 sigma column density sensitivity of 2.8 x 10(exp 19) sq cm on scales of a few kpc. Small H I clouds could have been detected down to a few times 10(exp 6) solar mass. Our failure to detect H I emission at the higher column densities sets a lower limit to the radius of the Lyman alpha clouds of 3.9 kpc, assuming a spherical geometry.

Published
1993
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26. Star counts from the Hubble Space Telescope Snapshot Survey. I - Galactic models

Author

Gould, A, Bahcall, J. N, and Maoz, D

Subjects
Astronomy
Abstract

We report a photometric study of stars from 450 fields at high Galactic latitudes that were observed in the Hubble Space Telescope Snapshot Survey to an average limiting apparent magnitude of V = 21.4. There are 166 fields that contain quasars selected in radio, X-ray, and color-excess surveys. This sample of 273 stars is free of selection bias with respect to the density of stars. To within the Poisson errors, the total counts and magnitude distribution of this unbiased sample are in agreement with the Bahcall-Soneira model (Bahcall, 1986). The angular distribution of the faint stars favors, at the 2 sigma level, a somewhat steeper disk luminosity function and a smaller spheroid main-sequence normalization than given by the model. The sample does not have enough statistical power to distinguish between the two-component Bahcall-Soneira model and the three-component model first proposed by Gilmore and Reid (1983), which contains a thick disk. The statistical power of the survey would increase about 15-fold if colors were obtained for the stars: the data probe the main sequences of the disk, thick disk, and spheroid. Models with and without a thick disk could then be distinguished at the 6 sigma level. The HST Snapshot Survey includes an additional 284 fields, 279 of which are centered on quasars that were selected by objective-prism surveys. These 279 fields are expected to show and do exhibit bias against bright stars, making them unsuitable for testing Galactic models.

Published
1993
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27. The Hubble Space Telescope Snapshot Survey. IV - A summary of the search for gravitationally lensed quasars

Author

Maoz, D, Bahcall, J. N, Schneider, D. P, Bahcall, N. A, Djorgovski, S, Doxsey, R, Gould, A, Kirhakos, S, Meylan, G, and Yanny, B

Subjects
Astrophysics
Abstract

We report the concluding results of the HST Snapshot Survey for gravitationally lensed quasars. New observations of 153 high-luminosity z above 1 quasars are presented, bringing to 498 the total number of quasars observed in the survey. The new observations do not reveal new candidates for gravitational lensing. We present tables summarizing all of the snapshot observations, with measured V-magnitudes, accurate to 0.1 mag, for each of the quasars successfully observed. The observed frequency of lensing of quasars into multiple images is 3-6 out of 502, depending on whether one counts candidates that are not yet securely confirmed and cases in which clusters play a role. This frequency is in the range predicted by calculations with a vanishing cosmological constant, assuming galaxies can be modeled by unevolving isothermal spheres dominated in their centers by dark matter. The observed frequency is an order of magnitude lower than expected in such models when the universe is strongly dominated by a cosmological constant. This conclusion is, however, sensitive to the model assumptions and to the precise number of actual lensed quasars.

Published
1993
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28. The Hubble Space Telescope Snapshot Survey. III - Further observations in search of gravitationally lensed quasars

Author

Maoz, D, Bahcall, J. N, Doxsey, R, Schneider, D. P, Bahcall, N. A, Lahav, O, and Yanny, B

Subjects
Astrophysics
Abstract

We present new HST Snapshot Survey observations of 163 high-luminosity z greater than 1 quasars, bringing the total number observed to date in the survey to 347 quasars. Each exposure was searched for evidence on gravitational lensing. Among the newly observed quasars, six have additional point sources at separations of 2-6 arcsec, but in all six cases ground-based data indicate that gravitational lensing is not involved. No point sources were found at smaller separations. Counting the one new lens candidate the survey has uncovered and the known lenses excluded from the sample, the observed frequency of lensing of quasars by galaxies is 5/351. This frequency is in the range predicted by models with a vanishing cosmological constant, but an order of magnitude lower than expected in models strongly dominated by a cosmological constant.

Published
1993
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29. Helium diffusion in the sun

Author

Bahcall, J. N and Pinsonneault, M. H

Subjects
Solar Physics
Abstract

We calculate improved standard solar models using the new Livermore (OPAL) opacity tables, an accurate (exportable) nuclear energy generation routine which takes account of recent measurements and analyses, and the recent Anders-Grevesse determination of heavy element abundances. We also evaluate directly the effect of the diffusion of helium with respect to hydrogen on the calculated neutrino fluxes, on the primordial solar helium abundance, and on the depth of the convective zone. Helium diffusion increases the predicted event rates by about 0.8 SNU, or 11 percent of the total rate, in the chlorine solar neutrino experiment, by about 3.5 SNU, or 3 percent, in the gallium solar neutrino experiments, and by about 12 percent in the Kamiokande and SNO solar neutrino experiments. The best standard solar model including helium diffusion and the most accurate nuclear parameters, element abundances, and radiative opacity predicts a value of 8.0 SNU +/- 3.0 SNU for the C1-37 experiment and 132 +21/-17 SNU for the Ga - 71 experiment, where the uncertainties include 3 sigma errors for all measured input parameters.

Published
1992

30. Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem

Author

Shi, X, Schramm, D. N, and Bahcall, J. N

Subjects
Solar Physics
Abstract

The paper explores the impact of astrophysical uncertainties on the Mikheyev-Smirnov-Wolfenstein (MSW) solution by calculating the allowed MSW solutions for 1000 different solar models with a Monte Carlo selection of solar model input parameters, assuming a full three-family MSW mixing. Applications are made to the chlorine, gallium, Kamiokande, and Borexino experiments. The initial GALLEX result limits the mixing parameters to the upper diagonal and the vertical regions of the MSW triangle. The expected event rates in the Borexino experiment are also calculated, assuming the MSW solutions implied by GALLEX.

Published
1992
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31. Gravitational lensing of quasars as seen by the Hubble Space Telescope Snapshot Survey

Author

Maoz, D, Bahcall, J. N, Doxsey, R, Schneider, D. P, Bahcall, N. A, Lahav, O, and Yanny, B

Subjects
Astrophysics
Abstract

Results from the ongoing HST Snapshot Survey are presented, with emphasis on 152 high-luminosity, z greater than 1 quasars. One quasar among those observed, 1208 + 1011, is a candidate lens system with subarcsecond image separation. Six other quasars have point sources within 6 arcsec. Ground-based observations of five of these cases show that the companion point sources are foreground Galactic stars. The predicted lensing frequency of the sample is calculated for a variety of cosmological models. The effect of uncertainties in some of the observational parameters upon the predictions is discussed. No correlation of the drift rate with time, right ascension, declination, or point error is found.

Published
1992
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32. The snapshot survey - A search for gravitationally lensed quasars with the Hubble Space Telescope

Author

Bahcall, J. N, Maoz, D, Doxsey, R, Schneider, D. P, Bahcall, N. A, Lahav, O, and Yanny, B

Subjects
Astronomy
Abstract

The first results from the HST Non-Proprietary Snapshot Survey are presented in order to investigate new examples of multiply imaged quasars that are the result of gravitational lensing. None of the approximately 30 quasars observed at high spatial resolution show evidence of multiple imaging by gravitational lensing. These results are compared with lower resolution ground-based surveys and current theoretical predictions. Several engineering problems in the observatory's performance are addressed. It particular, the large telescope pointing errors and drift rates are found to be primarily the result of the lack of correction for stellar aberration when pointing and tracking are performed solely with gyroscopes. The implications for the possibly low intrinsic gyro drift rate on future observations are discussed.

Published
1992
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34. Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

Author

Achterberg, A., Ackermann, M., Adams, J., Ahrens, J., Andeen, K., Auffenberg, J., Bahcall, J. N., Bai, X., Baret, B., Barwick, S. W., Bay, R., Beattie, K., Becka, T., Becker, J. K., Becker, K.-H., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Blaufuss, E., Boersma, D. J., Bohm, C., Bolmont, J., Boser, S., Botner, O., Bouchta, A., Braun, J., Burgess, C., Burgess, T., Castermans, T., Chirkin, D., Christy, B., Clem, J., Cowen, D. F., D'Agostino, M. V., Davour, A., Day, C. T., De Clercq, C., Demirors, L., Descamps, F., Desiati, P., DeYoung, T., Diaz-Velez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Edwards, W. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Evenson, P. A., Fadiran, O., Fazely, A. R., Filimonov, K., Foerster, M. M., Fox, B. D., Franckowiak, A., Gaisser, T. K., Gallagher, J., Ganugapati, R., Geenen, H., Gerhardt, L., Goldschmidt, A., Goodman, J. A., Gozzini, R., Griesel, T., Grullon, S., Gross, A., Gunasingha, R. M., Gurtner, M., Hallgren, A., Halzen, F., Han, K., Hanson, K., Hardtke, D., Hardtke, R., Hart, J. E., Hasegawa, Y., Hauschildt, T., Hays, D., Heise, J., Helbing, K., Hellwig, M., Herquet, P., Hill, G. C., Hodges, J., Hoffman, K. D., Hommez, B., Hoshina, K., Hubert, D., Hughey, B., Hulth, P. O., Hultqvist, K., Hulss, J.-P., Hundertmark, S., Inaba, M., Ishihara, A., Jacobsen, J., Japaridze, G. S., Johansson, H., Jones, A., Joseph, J. M., Kampert, K.-H., Karg, T., Karle, A., Kawai, H., Kelley, J. L., Kitamura, N., Klein, S. R., Klepser, S., Kohnen, G., Kolanoski, H., Kopke, L., Kowalski, M., Kowarik, T., Krasberg, M., Kuehn, K., Labare, M., Landsman, H., Leich, H., Leier, D., Liubarsky, I., Lundberg, J., Lunemann, J., Madsen, J., Mase, K., Matis, H. S., McCauley, T., McParland, C. P., Meli, A., Messarius, T., Meszaros, P., Miyamoto, H., Mokhtarani, A., Montaruli, T., Morey, A., Morse, R., Movit, S. M., Muenich, K., Nahnhauer, R., Nam, J. W., Niessen, P., Nygren, D. R., Ogelman, H., Olivas, A., Patton, S., Pena-Garay, C., Perez de los Heros, C., Piegsa, A., Pieloth, D., Pohl, A. C., Porrata, R., Pretz, J., Price, P. B., Przybylski, G. T., Rawlins, K., Razzaque, S., Resconi, E., Rhode, W., Ribordy, M., Rizzo, A., Robbins, S., Roth, P., Rott, C., Rutledge, D., Ryckbosch, D., Sander, H.-G., Sarkar, S., Schlenstedt, S., Schmidt, T., Schneider, D., Seckel, D., Semburg, B., Seo, S. H., Seunarine, S., Silvestri, A., Smith, A. J., Solarz, M., Song, C., Sopher, J. E., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Steffen, P., Stezelberger, T., Stokstad, R. G., Stoufer, M. C., Stoyanov, S., Strahler, E. A., Straszheim, T., Sulanke, K.-H., Sullivan, G. W., Sumner, T. J., Taboada, I., Tarasova, O., Tepe, A., Thollander, L., Tilav, S., Tluczykont, M., Toale, P. A., Turcan, D., van Eijndhoven, N., Vandenbroucke, J., Van Overloop, A., Viscomi, V., Voigt, B., Wagner, W., Walck, C., Waldmann, H., Walter, M., Wang, Y.-R., Wendt, C., Wiebusch, C. H., Wikstrom, G., Williams, D. R., Wischnewski, R., Wissing, H., Woschnagg, K., Xu, X. W., Yodh, G., Yoshida, S., Zornoza, J. D., and IceCube Collaboration

Subjects
Gamma rays: bursts, Normalization (statistics), Physics, Range (particle radiation), Muon, Astrophysics::High Energy Astrophysical Phenomena, Neutrinos, Telescopes, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Coincidence, Space and Planetary Science, Cascade, Astronomia, Diffuse flux, High Energy Physics::Experiment, Neutrino, Gamma-ray burst
Abstract

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the theoretical prediction). For this search 90% of the neutrinos would fall in the energy range 50 TeV to 7 PeV. The second analysis looked for neutrino-induced cascades in coincidence with 73 bursts detected by BATSE in the year 2000. The resulting upper limit on the diffuse flux normalization times E^2, also at 1 PeV, is 1.5 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 110 above the theoretical prediction) for the same energy range. The neutrino-induced cascade channel is complementary to the up-going muon channel. We comment on its advantages for searches of neutrinos from GRBs and its future use with IceCube., Comment: 38 pages. 16 postscript figures. Accepted for publication in the Astrophysical Journal

Published
2007
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37. Multiwavelength comparison of selected neutrino point source candidates

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

38. Search for Diffuse Flux of Extraterrestrial Muon Neutrinos using AMANDA-II Data from 2000 to 2003

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

39. Performance of AMANDA-II using Transient Waveform Recorders

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

40. IceCube : Initial Performance

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

41. Calibration and characterization of photomultiplier tubes of the IceCube neutrino detector

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

42. Search for neutralino dark matter with the AMANDA neutrino detector

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

43. A software trigger for the AMANDA neutrino detector

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

44. Sensitivity of AMANDA-II to UHE Neutrinos

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

45. An investigation of seasonal variations in the atmospheric neutrino rate with the AMANDA-II neutrino telescope

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

46. Air showers with IceCube : First Engineering Data

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

47. Search for high energy neutrino point sources in the northern hemisphere with the AMANDA-II neutrino telescope

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

48. A source stacking analysis of AGN as neutrino point source candidates with AMANDA

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

49. Search for a diffuse flux of non-terrestrial muon neutrinos with the AMANDA detector

Author

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

Subjects
Astrophysics and Astronomy
Published
2005

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