Results 11 to 20 of about 6,030 (145)
Characterizing cool, neutral gas and ionized metals in the outskirts of low-z galaxy clusters [PDF]
Monthly notices of the Royal Astronomical Society, 2023
We present the first detection of cool, neutral gas in the outskirts of low-z galaxy clusters using a statistically significant sample of 3191 z ≈ 0.2 background quasar–foreground cluster pairs by cross-matching the Hubble Spectroscopic Legacy Archive ...Sapna Mishra, S. Muzahid, Sayak Dutta, R. Srianand, J. C. I. C. F. Astronomy, Astrophysics, India, P. S. University, Usa +8 moresemanticscholar +1 more sourceFlexible, integrated modeling of tokamak stability, transport, equilibrium, and pedestal physics [PDF]
Physics of Plasmas, 2023 The STEP (Stability, Transport, Equilibrium, and Pedestal) integrated-modeling tool has been developed in OMFIT to predict stable, tokamak equilibria self-consistently with core-transport and pedestal calculations.B. Lyons, J. McClenaghan, T. Slendebroek, O. Meneghini, T. Neiser, S. Smith, D. Weisberg, E. Belli, J. Candy, J. Hanson, L. Lao, N. Logan, S. Saarelma, O. Sauter, P. Snyder, G. Staebler, K. Thome, A. D. T. G. Atomics, Oak Ridge Institute for Science, Education, Columbia University, Lawrence Livermore National Laboratory, UK XMM-Newton Science Operations Centre, Ecole Polytechnique Federale de Lausanne Swiss Plasma Center, Oak Ridge National Laboratory +24 moresemanticscholar +1 more sourceMurchison Widefield Array detection of steep-spectrum, diffuse, non-thermal radio emission within Abell 1127 [PDF]
Publications Astronomical Society of Australia, 2020 Diffuse, non-thermal emission in galaxy clusters is increasingly being detected in low-frequency radio surveys and images. We present a new diffuse, steep-spectrum, non-thermal radio source within the cluster Abell 1127 found in survey data from the ...S. Duchesne, M. Johnston-Hollitt, Zhenghao Zhu, R. Wayth, Jack L. B. Line International Centre for Radio Astronom University, Perth, Australia., S. O. Physics, Astronomy, S. University, P. R. China, A. C. F. A. A. I. 3. Dimensions +11 moresemanticscholar +1 more sourceMonitoring of the radio galaxy M 87 during a low-emission state from 2012 to 2015 with MAGIC [PDF]
Monthly notices of the Royal Astronomical Society, 2020
M 87 is one of the closest (z = 0.004 36) extragalactic sources emitting at very high energies (VHE, E > 100 GeV). The aim of this work is to locate the region of the VHE gamma-ray emission and to describe the observed broad-band spectral energy ...M. Acciari, S. Ansoldi, L. A. Antonelli, A. Engels, C. Arcaro, D. Baack, A. Babi'c, B. Banerjee, P. Bangale, U. D. Almeida, J. Barrio, J. Gonz'alez, W. Bednarek, L. Bellizzi, E. Bernardini, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, vZ. Bovsnjak, G. Busetto, R. Carosi, G. Ceribella, Y. Chai, A. Chilingaryan, S. Cikota, S. M. Colak, U. Colin, E. Colombo, J. Contreras, J. Cortina, S. Covino, V. D’Elia, P. D. Vela, F. Dazzi, A. Angelis, B. Lotto, M. Delfino, J. Delgado, D. Depaoli, F. Pierro, L. Venere, E. Espineira, D. Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Ramazani, A. Fattorini, A. Fern'andez-Barral, G. Ferrara, D. Fidalgo, L. Foffano, M. Fonseca, L. Font, C. Fruck, S. Fukami, R. L'opez, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, N. Godinovi'c, D. Green, D. Guberman, D. Hadasch, A. Hahn, J. Herrera, J. Hoang, D. Hrupec, M. Hutten, T. Inada, S. Inoue, K. Ishio, Y. Iwamura, L. Jouvin, D. Kerszberg, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, S. Lombardi, F. Longo, M. L'opez, R. L'opez-Coto, A. L'opez-Oramas, S. Loporchio, B. Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Mart'inez, S. Masuda, D. Mazin, S. Mi'canovi'c, D. Miceli, M. Minev, J. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, V. Moreno, E. Moretti, P. Munar-Adrover, V. Neustroev, C. Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogu'es, M. Nothe, S. Nozaki, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. Paredes, P. Peñil, Michele Peresano, M. Persic, P. Moroni, E. Prandini, I. Puljak, W. Rhode, M. Rib'o, J. Rico, C. Righi, A. Rugliancich, L. Saha, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, K. Schmidt, T. Schweizer, J. Sitarek, I. vSnidari'c, D. Sobczynska, A. Somero, A. Stamerra, D. Strom, M. Strzys, Y. Suda, T. Suri'c, M. Takahashi, F. Tavecchio, P. Temnikov, T. Terzi'c, M. Teshima, N. Torres-Albà, L. Tosti, S. Tsujimoto, V. Vagelli, J. Scherpenberg, G. Vanzo, M. Acosta, C. Vigorito, V. Vitale, I. Vovk, M. Will, D. Zari'c, M. C. K. Asano, K. Hada, D. Harris, M. Giroletti, H. Jermak, J. Madrid, F. Massaro, S. Richter, F. Spanier, I. Steele, R. C. Walker, Instituto de Astrof'isica de Canarias, La Laguna, Spain., U. Udine, Infn, Sezione di Trieste, Italy., Udine, I. I. F. Astrophysics, Roma, E. Zurich, I. F. Physics, Zurich, Switzerland., Technische Universitat Dortmund, Dortmund, H Germany, Croatian Magic Consortium Rudjer Boskovic Institute, University of Rijeka, U. O. S. -. Fesb, University of Zagreb-FER, University of Osijek, Split, Croatia., S. S. I. O. Physics, Hbni, Kolkata, India., Centro Brasileiro de Pesquisas F'isicas, R. Janeiro, Brasil., I. Institute, Emftel Department, U. Madrid, Madrid, Division of Astrophysics, U. Lodz, Lodz, Poland, Dipartimento Sfta, S. D. Fisica, U. Siena, I. Pisa, Siena, D. Zeuthen, Zeuthen, Infn Consortium, Romé, M. F. Physik, Munchen, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, E-08193 Bellaterra, Bellaterra, D. Universita, S. Infn, Padova, U. Pisa, I. Pisa, Pisa, RA TheArmenianConsortiumICRANet-ArmeniaatNAS, A. A. N. Laboratory, Yerevan, Armenia, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Institut fur Theoretische Physik und Astrophysik - Fakultat Wurzburg, Wurzburg, Finnish Magic Consortium Finnish Centre of Astronomy with Eso, U. Turku, F. Turku, A. Division, U. Oulu, F. Oulu, Finland., Turku, U. Barcelona, Barcelona, J. Icrr, T. U. O. Tokyo, 277-8582 Chiba, Japan., D. Physics, Kyoto University, 606-8502 Kyoto, T. University, 259-1292 Kanagawa, Riken, 351-0198 Saitama, Kyoto, Inst. for Nucl. Research, Nucl. Energy, Sofía, Bulgaria., U. Barcelona, A. Spain, A. N. D. D. Fisica, Universita di UdineI.N.F.N. Trieste, I. Trieste, also at INAF-Trieste, D. Astronomy, U. Bologna, Centre for Astrophysics Research, North-West University, Potchefstroom 2520, S. Africa, Inaf - Padova, 5. vicolodell'Osservatorio, 35122, Icrr, U. Tokyo, Kashiwa-shi, Chiba 277-8582, Mizusawa Vlbi Observatory, N. A. O. O. Japan, 2-12 Hoshigaoka-cho, Mizusawa, Oshu, Iwate 023-0861, Department of Materials Science, The Graduate University for Advanced Studies, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, Usa, I. D. Radioastronomia, V. G. 101, 40129 Bologna, A. R. Institute, Liverpool John Moore's University, Liverpool, UK., University of Texas Rio Grande Valley, Astronomy, One West University Blvd. Brownsville, TX 78520, D. Fisica, U. Torino, 1. viaPietroGiuria, I-10133 Torino, S. D. Torino, I. Torino, 20 viaOsservatorio, I. P. Torinese, Consorzio Interuniversitario per la Fisica Spaziale, I-10125, Torino, National Radio Astronomy Observatory, Socorro, Nm Usa, I. F. Astrophysik, U. Heidelberg +344 moresemanticscholar +1 more sourceThe inner structure of ΛCDM haloes – III. Universality and asymptotic slopes [PDF]
, 2003 We investigate the mass profile of cold dark matter (ACDM) haloes using a suite of numerical simulations spanning five decades in halo mass, from dwarf galaxies to rich galaxy clusters.J. Navarro, E. Hayashi, C. Power, A. Jenkins, C. Frenk, S. White, V. Springel, J. Stadel, T. Q. U. O. Victoria, University fo Durham, Max Planck Institute for Astrophysics, U. Zurich, U. Washington +12 moresemanticscholar +1 more sourcePrivacy and Data Protection Practices of Digital Lending Apps in Kenya
Journal of Intellectual Property and Information Technology Law (JIPIT), 2021 The Centre for Intellectual Property and Information Technology Law (CIPIT) has been studying the impact of digital identities on society. This has included policy research on the legal and technical aspects of the national digital ID system Huduma ...Centre for Intellectual Property and Information Technolo (CIPIT)semanticscholar +1 more sourceCRIRES high-resolution near-infrared spectroscopy of diffuse interstellar band profiles. Detection of twelve new DIBs in the YJ band and an introduction of a combined ISM sight line and stellar analysis approach [PDF]
Astronomy & Astrophysics, 2022 A high spectral resolution investigation of diffuse interstellar bands (DIBs) in the near-infrared ($YJ$ band) is conducted to test new methods, to confirm and improve existing parameters, and to search for new DIBs.Alexander Ebenbichler, A. Postel, N. Przybilla, A. Seifahrt, D. Weßmayer, W. Kausch, M. Firnstein, K. Butler, H. Kaufl, A. Kaufer, Harold Linnartz Institut fur Astro- und Teilchenphysik, U. Innsbruck, D. O. Astronomy, Astrophysics, U. Chicago, D. Remeis-Sternwarte, Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universitat Erlangen-Nurnberg, Lmu Munchen, E. Observatory, Laboratory for Multiwavelength Astrophysics, L. Observatory +21 moresemanticscholar +1 more sourceSlave voices and experiences in the later medieval Europe
History Compass, Volume 21, Issue 10, October 2023., 2023 Abstract
Late medieval slavery was profoundly entangled in urban life in particular. Cities all around the Mediterranean coast were implicated in the trade—although this article focuses on the Christian Mediterranean which was bound together by a general reliance on Roman law (alongside local customary laws and the canon law of the Church).Hannah Skodawiley +1 more sourceSubstructures in cold dark matter haloes [PDF]
, 2003 We analyse the properties of substructures within dark matter haloes (subhaloes) using a set of high-resolution numerical simulations of the formation of structure in a ACDM universe.G. Lucia, G. Kauffmann, V. Springel, S. White, B. Lanzoni, F. Stoehr, G. Tormen, N. Y. Mpa, Garching, H Germany, I. Bologna, D. Astronomia, U. Padova, H. C. F. Astrophysics +13 moresemanticscholar +1 more source
