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Amanda W. Harrist, K. Denise Bradley 


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Amanda W. Harrist and K. Denise Bradley are not mentioned in any of the provided abstracts.

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The provided paper does not mention Amanda W. Harrist or K. Denise Bradley. The paper is about selected physics results from the AMANDA neutrino telescope.
Journal ArticleDOI
E. Andres, P. Askebjer, Xinhua Bai, G. Barouch, Steven W. Barwick, R. C. Bay, K. H. Becker, Lars Bergström, D. Bertrand, D. Bierenbaum, A. Biron, J. Booth, Olga Botner, Adam Bouchta, M. M. Boyce, Staffan Carius, A. Chen, D. Chirkin, Jan Conrad, Jodi Cooley, Caroline Costa, D. F. Cowen, J. Dailing, E. Dalberg, T. De Young, Paolo Desiati, J. P Dewulf, P. Doksus, Joakim Edsjö, P. Ekström, B. Erlandsson, T. Feser, M. Gaug, A. Goldschmidt, Ariel Goobar, L. Gray, H. Haase, Allan Hallgren, Francis Halzen, Kael Hanson, R. Hardtke, Y. D. He, M. Hellwig, H. Heukenkamp, G. C. Hill, P. O. Hulth, S. Hundertmark, J. E. Jacobsen, V. Kandhadai, Albrecht Karle, J. Kim, B. Koci, L. Köpke, Marek Kowalski, H. Leich, Matthias Leuthold, P. Lindahl, I. Liubarsky, P. Loaiza, D. M. Lowder, J. Ludvig, James Madsen, Pawel Marciniewski, H. S. Matis, A. Mihalyi, T. Mikolajski, T. C. Miller, Y. Minaeva, P. Miocinovic, P. C. Mock, R. Morse, T. Neunhöffer, F. M. Newcomer, P. Niessen, D. R. Nygren, Hakki Ögelman, C. Pérez de los Heros, R. Porrata, P. B. Price, K. Rawlins, C. Reed, Wolfgang Rhode, A. Richards, Stefan Richter, J. Rodríguez Martino, P. Romenesko, D. Ross, H. Rubinstein, H. G. Sander, T. Scheider, T. O. B. Schmidt, D. Schneider, E. Schneider, R. Schwarz, A. Silvestri, M. Solarz, Glenn Spiczak, Christian Spiering, N. Starinsky, D. Steele, P. Steffen, R. G. Stokstad, Ole Streicher, Q. Sun, I. Taboada, L. Thollander, T. Thon, S. Tilav, Nicholas G. Usechak, M. Vander Donckt, C. Walck, Ch. Weinheimer, C. H. Wiebusch, R. Wischnewski, H. Wissing, Kurt Woschnagg, W. Wu, G. B. Yodh, S. Young 
3 Citations
The provided paper does not mention Amanda W. Harrist or K. Denise Bradley.
Open accessProceedings Article
James da Silva, Olafur Guthmundsson 
05 Nov 1993
35 Citations
The provided paper does not mention Amanda W. Harrist or K. Denise Bradley.
The provided paper does not mention Amanda W. Harrist or K. Denise Bradley. The paper is about the AMANDA computerized document management system.
The paper does not mention Amanda W. Harrist or K. Denise Bradley. The paper is about implementing robust background representation and exploring the intrinsic data structure of hyperspectral imagery for anomaly detection.

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What is k nearest neighbor?3 answersThe K Nearest Neighbors (KNN) classifier is a widely used machine learning tool for classification, clustering, and regression applications. It determines the class membership of an unlabeled sample based on the class memberships of the K labeled samples that are closest to it. The choice of K has been the subject of various studies, and different variants of KNN have been proposed. However, no variant has been proven to outperform all others. Some proposed variants ensure that the K nearest neighbors are close to the unlabeled sample and find K along the way. These variants have been tested and compared to the standard KNN in theoretical scenarios and for indoor localization based on ion-mobility spectrometry fingerprints, achieving higher classification accuracy while maintaining the same computational demand. Another variation of KNN uses the Nk interaction graph to determine the K nearest neighbors, allowing for the formation of clusters with arbitrary shapes. Two algorithms based on the Nk interaction graph have been proposed and compared to the original KNN in experiments with datasets of different properties. Additionally, a novel classifier called Power Muirhead Mean K-Nearest Neighbors (PMM-KNN) has been proposed to overcome issues with outliers, small datasets, and unbalanced datasets. PMM-KNN calculates the local means of every class using the Power Muirhead Mean operator and has outperformed three state-of-the-art classification methods in experiments with five well-known datasets.
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