Relevant bibliographies by topics / Halo

Academic literature on the topic 'Halo'

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Published: 4 June 2021
Last updated: 6 September 2023

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Journal articles on the topic "Halo"

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Izosimov, I. N. "Isospin in halo nuclei: Borromean halo, tango halo, and halo isomers." Physics of Atomic Nuclei 80, no. 5 (September 2017): 867–76. http://dx.doi.org/10.1134/s1063778817050118.

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Nufer, Gerd. "“Say hello to Halo”: the halo effect in sports." Innovative Marketing 15, no. 3 (September 30, 2019): 116–29. http://dx.doi.org/10.21511/im.15(3).2019.09.

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In daily life, people tend to use mental shortcuts to simplify and speed up their decision-making processes. A halo effect exists if the impression created by a dominant attribute influences how other attributes of an object or subject are judged. It involves a cognitive bias that leads to distorted assessments. However, the halo effect has barely been researched in a sports-related context, although it can substantially contribute to understanding how sport fans think and behave. The objective of this paper is to answer the question that is of interest for both theory and practice of sports marketing: Is there a halo effect in sports? Does the sporting success or failure of a professional soccer team radiate or even outshine other sports-related and non-sports aspects and influence or distort how the club is perceived by its fans? Fans of six soccer clubs selected from the first German soccer league Bundesliga were interviewed. This paper presents the results of an empirical study based on a data set consisting of a total of 4,180 cases. The results of the analyses substantiate the distortion of the fans’ perception with regard to a very diverse range of aspects that is triggered by the sporting success or failure of their favorite club.
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Jonson, B., and K. Riisager. "Halo and halo excitations." Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences 356, no. 1744 (September 15, 1998): 2063–81. http://dx.doi.org/10.1098/rsta.1998.0263.

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Suzuki, Nathalie, Monique Dalapicola, Giuseppe Argenziano, Aimilios Lallas, Caterina Longo, Simonetta Piana, Gerardo Ferrara, Margherita Raucci, and Elvira Moscarella. "Halo and pseudo-halo melanoma." Journal of the American Academy of Dermatology 74, no. 4 (April 2016): e59-e61. http://dx.doi.org/10.1016/j.jaad.2015.09.027.

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Izosimov, Igor. "Borromean halo, Tango halo, and halo isomers in atomic nuclei." EPJ Web of Conferences 107 (2016): 09003. http://dx.doi.org/10.1051/epjconf/201610709003.

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Nakatsukasa, Takashi, Kazuhiro Yabana, Makoto Ito, Minoru Kobayashi, and Manabu Ueda. "Fusion Reaction of Halo Nuclei: Proton Halo versus Neutron Halo." Progress of Theoretical Physics Supplement 154 (2004): 85–91. http://dx.doi.org/10.1143/ptps.154.85.

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Vytiniotis, Dimitrios, Simon Peyton Jones, Koen Claessen, and Dan Rosén. "HALO." ACM SIGPLAN Notices 48, no. 1 (January 23, 2013): 431–42. http://dx.doi.org/10.1145/2480359.2429121.

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Sotiriadis, D., E. Lazaridou, A. Patsatsi, A. Kastanis, A. Trigoni, and D. Devliotou-Panagiotidou. "Does halo nevus without halo exist?" Journal of the European Academy of Dermatology and Venereology 20, no. 10 (November 2006): 1394–96. http://dx.doi.org/10.1111/j.1468-3083.2006.01760.x.

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Murphy, Kevin R., and Douglas H. Reynolds. "Does true halo affect observed halo?" Journal of Applied Psychology 73, no. 2 (1988): 235–38. http://dx.doi.org/10.1037/0021-9010.73.2.235.

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García, Rafael, and Eduardo Rozo. "Halo exclusion criteria impacts halo statistics." Monthly Notices of the Royal Astronomical Society 489, no. 3 (September 5, 2019): 4170–75. http://dx.doi.org/10.1093/mnras/stz2458.

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ABSTRACT Every halo-finding algorithm must make a critical yet relatively arbitrary choice: it must decide which structures are parent haloes, and which structures are subhaloes of larger haloes. We refer to this choice as percolation. We demonstrate that the choice of percolation impacts the statistical properties of the resulting halo catalogue. Specifically, we modify the halo-finding algorithm rockstar to construct three different halo catalogues from the same simulation data, each with identical mass definitions, but different choice of percolation. The resulting haloes exhibit significant differences in both halo abundance and clustering properties. Differences in the halo mass function reach 6 per cent for haloes of mass $10^{13}\ h^{-1}\ {\rm {\rm M}_{\odot }}$, larger than the few per cent precision necessary for current cluster abundance experiments such as the Dark Energy Survey. Comparable differences are observed in the large-scale clustering bias, while differences in the halo–matter correlation function reach 30 per cent on translinear scales. These effects can bias weak-lensing estimates of cluster masses at a level comparable to the statistical precision of current state-of-the-art experiments.
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Dissertations / Theses on the topic "Halo"

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PANOZZO, SIMONE. "THE SPECTRAL HALO." Doctoral thesis, Università degli Studi di Milano, 2019. http://hdl.handle.net/2434/657582.

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In this thesis, we construct a function defined over the space of integral overconvergent modular forms of Andreatta, Iovita and Pilloni, taking values in the module of continuous functions from p adic integers to a suitably constructed perfection of an overconvergence region of the formal weight space. The existence of this function is related to the possibility of proving Coleman's Halo conjecture about the distribution of eigenvalues of the Hecke operator at p acting on spaces of overconvergent modular forms. In the thesis, we construct the function, and we also compute explicitly the action of the operator over those continuous functions which are in the image of the map. Moreover, in chapter 3, we also show that the space of such continuous functions admits a Mahler basis.
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Arnold, Richard A. "The galactic stellar halo." Thesis, University of Cambridge, 1991. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.386335.

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O'Meara, Jeffrey A. "Dynamic kinetic resolution: Diastereoselective amination of alpha-halo esters and alpha-halo imidazolidinones." Thesis, University of Ottawa (Canada), 1995. http://hdl.handle.net/10393/9493.

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The synthesis of optically active N-protected $\alpha$-amino esters and $\alpha$-amino imidazolidinones via a dynamic kinetic resolution protocol will be discussed. The methodology is based on fundamental reactivity differences between diastereomeric $\alpha$-halo esters and $\alpha$-halo imidazolidinones. The process involves nucleophillic displacement of the diastereomeric $\alpha$-halogenated esters and imidazolidinones with benzylamine. The corresponding displacement products are obtained with 70 - $>$ 98% de. Both absolute configurations are possible at the aminated postion by appropriate choice of the chiral auxiliary. The application of this methodology towards the synthesis of several optically active $\alpha$-amino esters was investigated. A five step sequence, starting from commercially available acid chlorides, was developed for synthesizing $\alpha$-amino esters in $\sim$40% overall yield. By utilizing dibenzylamine as the nucleophile, the DKR process has been effectively utilized in an approach to Reetz aldehydes ($\alpha$-dibenzylamino aldehydes). The increased bulk of dibenzylamine provides increased diastereoselectivity relative to benzylamine and the Reetz aldehyde precursors are obtained with a high degree of optical purity. Mechanistic aspects the reaction will also be discussed.
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Daw, Edward John 1969. "A search for halo axions." Thesis, Massachusetts Institute of Technology, 1998. http://hdl.handle.net/1721.1/50335.

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Jiang, Lilian. "Cosmological halo formation and mergers." Thesis, Durham University, 2015. http://etheses.dur.ac.uk/11004/.

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My research has centred around establishing the nature of dark matter haloes by investigating their abundance as a function of halo mass, the formation his- tory of each halo, commonly called the merger tree, and the internal structure of the halo, in terms of their radial density profiles and angular momentum. In the first part of this thesis, I present a new algorithm which groups the subhaloes found in cosmological N-body simulations by structure finders such as subfind into dark matter haloes whose formation histories are strictly hier- archical. One advantage of these ‘Dhaloes’ over the commonly used friends-of- friends (FoF) haloes is that they retain their individual identity in cases when FoF haloes are artificially merged by tenuous bridges of particles or by an over- lap of their outer diffuse haloes. Dhaloes are thus well suited for modelling galaxy formation and their merger trees form the basis of the Durham semi- analytic galaxy formation model, galform. Applying the Dhalo construction to the ΛCDM Millennium-2 simulation we find that approximately 90% of Dhaloes have a one-to-one, bijective match with a corresponding FoF halo. The remaining 10% are typically secondary components of large FoF haloes. Although the mass functions of both types of haloes are similar, the mass of Dhaloes correlates much more tightly with the virial mass, M200, than FoF masses. Approximately 80% of FoF and bijective and non-bijective Dhaloes are relaxed according to standard criteria. For these relaxed haloes all three types have similar concentration– M200 relations and, at fixed mass, the concentration distributions are described accurately by log-normal distributions. In the second part of this thesis, I present distributions of orbital parameters of infalling satellite haloes at the time of crossing the virial radius of their host halo. Detailed investigation of the orbits is crucial as it represents the initial conditions which determine the later evolution of the substructure within the host. I use merger trees in a high resolution cosmological N-body simulation to trace the satellite haloes and measure their orbits when they first infall into the host halo. I find that there is a trend of the orbital parameters with the ratio between the satellite halo mass and the host halo mass at infall. I find that the more massive satellites move along more eccentric orbits with lower specific angular momentum than less massive satellites. I also search for possible correlations between different orbital parameters and provide accurate fitting formulae for the two independent orbital parameters (the total velocity and the radial-to-total velocity ratio). Using combinations of these formulae, we successfully fit all the other orbital parameters.
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McCaine, Gina. "Halo orbit design and optimization." Thesis, Monterey, Calif. : Springfield, Va. : Naval Postgraduate School ; Available from National Technical Information Service, 2004. http://library.nps.navy.mil/uhtbin/hyperion/04Mar%5FMcCaine.pdf.

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Thesis (M.S. in Astronautical Engineering)--Naval Postgraduate School, March 2004.
Thesis advisor(s): I. Michael Ross, Don Danielson. Includes bibliographical references (p. 39-40). Also available online.
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Totten, Edward James. "Carbon stars in the Galactic Halo." Thesis, Queen's University Belfast, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.263490.

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Vale, António Manuel Dias de Sousa. "Linking halo mass to galaxy luminosity." Thesis, University of Cambridge, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.614222.

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Fermani, Francesco. "Modelling the Milky Way stellar halo." Thesis, University of Oxford, 2013. http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915.

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We motivate the importance of understanding the kinematics and dynamics of the Milky Way stellar halo both in unravelling the formation history and evolution of our host Galaxy and in the more general context of galaxy dynamics. We present a cleaned picture of the kinematics of the smooth component of the stellar halo: we develop a method to quantify the average distance error on a sample of stars based on the idea of Schoenrich et al. (2012), but adapted so that it uses velocity information only on average. We use this scheme to construct an analytic distance calibration for Blue Horizontal Branch (BHB) field halo stars in Sloan colours and demonstrate that our calibration is a) more accurate than the ones available and b) unbiased w.r.t. metallicity and colour. We measure the rotation of the smooth component of the stellar halo with a tool-set of four estimators that use either only the l.o.s. velocities or the full 3D motion. From two samples of BHB stars from the Sloan Digital Sky Survey, we favour a non-rotating single halo. We critique conflicting results in the literature based on similar samples and trace back the disagreement (either in the sign of rotation or in the morphology of the halo) to sample contaminations and/or neglect account of the halo geometry. We propose a scheme that generalizes any isotropic spherical model to a model where the potential is axisymmetric and the distribution function is a function of the three actions. The idea is to approximate the Hamiltonian as a function of the actions with a library of quadratic fits to surfaces of constant energy in action space and then make explicit the dependence of the energy on the three actions in the ergodic distribution function. The transparency of the physics implied by the model we achieve, should make it possible to combine our spheroidal models to the f(J)-models of Binney (2010) for the disks and of Pontzen & Governato (2013) for the dark-matter halo, and obtain a complete actions-defined dynamical model of the Milky Way Galaxy.
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Werner, Kim Fiona [Verfasser]. "Halo bias renormalisation / Kim Fiona Werner." Bonn : Universitäts- und Landesbibliothek Bonn, 2020. http://d-nb.info/1218301570/34.

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Books on the topic "Halo"

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Sindhi, Salim. Hurk halo dhima halo. Hyderabad: Islamik Waritarz Foram, n.d.

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MacDonald, Josh. Halo. Vancouver, B.C: Talonbooks, 2002.

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Halo. London: Fourth Estate, 1992.

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Halo. San Diego: Harcourt Brace, 1994.

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Halo. New York: TOR, 1991.

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Loveday, John. Halo. London: Sceptre, 1994.

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Nylund, Eric S. Halo. New York: Ballantine Books, 2003.

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Loveday, John. Halo. San Diego: Harcourt Brace, 1994.

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Halo. London: Atom, 2011.

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Biggs, Simon. Halo. London: Film and Video Umbrella, 1998.

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Book chapters on the topic "Halo"

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Glaser, Christian. "Halo-Effekt." In Risiko im Management, 9–12. Wiesbaden: Springer Fachmedien Wiesbaden, 2019. http://dx.doi.org/10.1007/978-3-658-25835-1_3.

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Yudin, Andrey. "Halo Sign." In Metaphorical Signs in Computed Tomography of Chest and Abdomen, 31. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-04013-4_16.

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Yudin, Andrey. "Periportal Halo." In Metaphorical Signs in Computed Tomography of Chest and Abdomen, 91. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-04013-4_46.

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Massi, Guido, and Philip E. Leboit. "Halo Nevus." In Histological Diagnosis of Nevi and Melanoma, 363–78. Heidelberg: Steinkopff, 2004. http://dx.doi.org/10.1007/978-3-7985-1943-5_23.

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Stefanaki, Christina. "Halo nevi." In Hypopigmentation, 149–52. New York, NY : CRC Press/Taylor & Francis Group, [2020]: CRC Press, 2019. http://dx.doi.org/10.1201/9781315146454-22.

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Gooch, Jan W. "Halo Effect." In Encyclopedic Dictionary of Polymers, 356. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-6247-8_5762.

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Orr, N. A. "Halo Nuclei." In Few-Body Problems in Physics ’98, 243–52. Vienna: Springer Vienna, 1999. http://dx.doi.org/10.1007/978-3-7091-6798-4_44.

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Laham, Simon M., and Joseph P. Forgas. "Halo effects." In Cognitive Illusions, 259–71. 3rd ed. London: Routledge, 2022. http://dx.doi.org/10.4324/9781003154730-19.

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Tanihata, Isao, and Björn Jonson. "Halo Nuclei." In Handbook of Nuclear Physics, 1–42. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-15-8818-1_63-1.

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Yudin, Andrey. "Halo Sign." In Metaphorical Signs in Computed Tomography of Chest and Abdomen, 37. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-24494-0_19.

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Conference papers on the topic "Halo"

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Pekkola, Marko. "Finnish Halo Observing Network: Search for Rare Halo Phenomena." In Light and Color in the Open Air. Washington, D.C.: Optica Publishing Group, 1990. http://dx.doi.org/10.1364/lcoa.1990.the3.

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During the first half of this century research on halo phenomena seems to have been in a chaotic state. Particularly the lists and theoretical views of Bravais (1847), Pernter and Exner (1922), Minnaert (1954) and Visser (1957, 1960) about the rarest known halos did not have much in common.
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Vytiniotis, Dimitrios, Simon Peyton Jones, Koen Claessen, and Dan Rosén. "HALO." In the 40th annual ACM SIGPLAN-SIGACT symposium. New York, New York, USA: ACM Press, 2013. http://dx.doi.org/10.1145/2429069.2429121.

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Baudisch, Patrick, and Ruth Rosenholtz. "Halo." In the conference. New York, New York, USA: ACM Press, 2003. http://dx.doi.org/10.1145/642611.642695.

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Panda, Reena, and Lizy K. John. "HALO." In ICS '18: 2018 International Conference on Supercomputing. New York, NY, USA: ACM, 2018. http://dx.doi.org/10.1145/3205289.3205323.

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Zhao, Nan, and Joseph A. Paradiso. "HALO." In the 2015 ACM International Joint Conference. New York, New York, USA: ACM Press, 2015. http://dx.doi.org/10.1145/2800835.2801670.

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Yuan, Yifan, Yipeng Wang, Ren Wang, and Jian Huang. "HALO." In ISCA '19: The 46th Annual International Symposium on Computer Architecture. New York, NY, USA: ACM, 2019. http://dx.doi.org/10.1145/3307650.3322272.

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Tatarchuk, Natasha. "Halo." In ACM SIGGRAPH 2011 Computer Animation Festival. New York, New York, USA: ACM Press, 2011. http://dx.doi.org/10.1145/2019001.2019033.

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Izosimov, Igor. "Structure of β-Decay Strength Function Sβ(E) in Halo Nuclei. Borromean Halo, Tango Halo, and Mixed Halo." In Proceedings of the Ito International Research Center Symposium "Perspectives of the Physics of Nuclear Structure". Journal of the Physical Society of Japan, 2018. http://dx.doi.org/10.7566/jpscp.23.013005.

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Ng, Wai Shan (Florence), and Ehud Sharlin. "Tweeting halo." In Adjunct proceedings of the 23nd annual ACM symposium. New York, New York, USA: ACM Press, 2010. http://dx.doi.org/10.1145/1866218.1866264.

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SCHRIEDER, G. "NEUTRON HALO." In Proceedings of the Tours Symposium on Nuclear Physics II. WORLD SCIENTIFIC, 1995. http://dx.doi.org/10.1142/9789814447058_0016.

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Reports on the topic "Halo"

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Moskal, Rob, Garry Booker, Mark Williamson, Mike Lash, and Jim Kiessling. High Altitude Observatory (HALO) Uprade. Fort Belvoir, VA: Defense Technical Information Center, January 2000. http://dx.doi.org/10.21236/ada380997.

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Fermi Research Alliance, LLC. Development of a Beam Halo Monitor. Office of Scientific and Technical Information (OSTI), March 2020. http://dx.doi.org/10.2172/1712749.

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Chen, T., J. Irwin, and R. H. Siemann. Studies of halo distributions under beam-beam interaction. Office of Scientific and Technical Information (OSTI), June 1995. http://dx.doi.org/10.2172/71395.

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Hubbard, Richard F., Martin Lampe, Steven P. Slinker, and Glenn Joyce. Halo Formation and Hollowing in Relativistic Electron Beams. Fort Belvoir, VA: Defense Technical Information Center, August 1988. http://dx.doi.org/10.21236/ada199734.

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Brooksby, C. A., S. L. Allen, L. R. Pedrotti, T. C. Simonen, B. E. Wood, W. L. Hsu, and J. G. Watkins. Halo recycler for the Tandem Mirror Experiment Upgrade. Office of Scientific and Technical Information (OSTI), November 1985. http://dx.doi.org/10.2172/6122623.

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Chao, A. Halo Generation and Beam Cleaning by Resonance Trapping. Office of Scientific and Technical Information (OSTI), August 2004. http://dx.doi.org/10.2172/829712.

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Gluckstern, R. L., and S. S. Kurennoy. Stability and halo formation in axisymmetric intense beams. Office of Scientific and Technical Information (OSTI), October 1997. http://dx.doi.org/10.2172/532552.

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Li, Ting. Exploring Milkyway Halo Substructures with Large-Area Sky Surveys. Office of Scientific and Technical Information (OSTI), January 2016. http://dx.doi.org/10.2172/1343961.

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Ryne, R. D., and T. P. Wangler. Recent results in analysis and simulation of beam halo. Office of Scientific and Technical Information (OSTI), September 1994. http://dx.doi.org/10.2172/10180043.

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Fedotov, A. V., R. L. Gluckstern, S. S. Kurennoy, and R. D. Ryne. Halo formation in spheroidal bunches with self-consistent stationary distributions. Office of Scientific and Technical Information (OSTI), December 1998. http://dx.doi.org/10.2172/307945.

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