Results 1 to 10 of about 169,328 (165)
Euclid preparation. XXIX. Forecasts for ten different higher-order weak lensing statistics [PDF]
Astronomy & Astrophysics, 2023 Recent cosmic shear studies have shown that higher-order statistics (HOS) developed by independent teams now outperform standard two-point estimators in terms of statistical precision thanks to their sensitivity to the non-Gaussian features of large ...Euclid Collaboration V. Ajani, M. Baldi, A. Barthelemy, A. Boyle, P. Burger, V. Cardone, S. Cheng, S. Codis, C. Giocoli, J. Harnois-D'eraps, S. Heydenreich, Vanshika Kansal, M. Kilbinger, L. Linke, C. Llinares, N. Martinet, C. Parroni, A. Peel, S. Pires, L. Porth, I. Tereno, C. Uhlemann, M. Vicinanza, S. Vinciguerra, N. Aghanim, N. Auricchio, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, F. Castander, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, L. Corcione, F. Courbin, M. Cropper, A. D. Silva, H. Degaudenzi, A. D. Giorgio, J. Dinis, M. Douspis, F. Dubath, X. Dupac, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, S. Galeotta, B. Garilli, B. Gillis, A. Grazian, F. Grupp, H. Hoekstra, W. Holmes, A. Hornstrup, P. Hudelot, K. Jahnke, M. Jhabvala, M. Kummel, T. Kitching, M. Kunz, H. Kurki-Suonio, P. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, S. Mei, Y. Mellier, M. Meneghetti, Michele Moresco, L. Moscardini, S. Niemi, J. Nightingale, T. Nutma, C. Padilla, S. Paltani, K. Pedersen, V. Pettorino, G. Polenta, M. Poncet, L. Popa, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, T. Schrabback, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, L. Stanco, J. Starck, P. Tallada-Cresp'i, A. Taylor, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, G. Zamorani, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, E. Bozzo, C. Colodro-Conde, D. Ferdinando, G. Fabbian, M. Farina, J. Graci'a-Carpio, E. Keihanen, V. Lindholm, D. Maino, N. Mauri, C. Neissner, M. Schirmer, V. Scottez, E. Zucca, Y. Akrami, C. Baccigalupi, A. Balaguera-Antol'inez, M. Ballardini, F. Bernardeau, A. Biviano, A. Blanchard, S. Borgani, A. Borlaff, C. Burigana, R. Cabanac, A. Cappi, C. Carvalho, S. Casas, G. Castignani, T. Castro, K. Chambers, A. Cooray, J. Coupon, H. Courtois, S. Davini, S. D. Torre, G. Lucia, G. Desprez, H. Dole, J. Escartín, S. Escoffier, I. Ferrero, F. Finelli, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, H. Hildebrandt, A. Munoz, B. Joachimi, J. Kajava, C. Kirkpatrick, L. Legrand, A. Loureiro, M. Magliocchetti, R. Maoli, S. Marcin, M. Martinelli, C. Martins, S. Matthew, L. Maurin, R. Metcalf, P. Monaco, G. Morgante, S. Nadathur, A. Nucita, V. Popa, D. Potter, A. Pourtsidou, M. Pontinen, P. Reimberg, A. S'anchez, Z. Sakr, A. Schneider, E. Sefusatti, M. Sereno, A. Shulevski, A. Mancini, J. Steinwagner, R. Teyssier, J. Valiviita, A. Veropalumbo, M. Viel, I. -. Paris-Saclay, Universit'e de Paris Cit'e, Cea, Cnrs, Astrophysique, Instrumentation et Mod'elisation Paris-Saclay, 91191 Gif-sur-Yvette, France, I. F. Physics, Astrophysics, D. Physics, E. Zurich, 27 Wolfgang-Pauli-Strasse, 8093 Zurich, Switzerland., D. Bologna, V. G. 932, 40129 Bologna, Italy, I. Bologna, V. G. 933, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, University Observatory, F. O. Physics, Ludwig-Maximilians-Universitat, 1. Scheinerstr., 81679 Munich, H Germany, Aim, Universit'e Paris-Saclay, U. Paris, Argelander Institut fur Astronomie, U. Bonn, 71 AufdemHugel, 53121 Bonn, Infn Roma, P. A. Moro, 2. -. C. D. D. Fisica, E. Marconi, 00133 Roma, I. Roma, 33 viaFrascati, 00078 Monte Porzio Catone, J. Baltimore, MD 21218, Usa, S. O. Mathematics, Statistics, Physics, N. University, Herschel Building, Newcastle-upon-Tyne, NE1 7RU, Uk, Departament de F'isica, F. Ciencias, Universidade de Lisboa, C8 Edif'icio, C. Grande, P. Lisboa, Portugal, I. D. A. E. C. D. Espacco, Tapada da Ajuda, 1049-001 Lisboa, A. Universit'e, Cnes, Lam, Marseille, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, D. Fisica, S. Roma, 2. PiazzaleAldoMoro, I. D. Spatiale, 91405, Orsay, I. Torino, 20 viaOsservatorio, 1. P. Torinese, U. Genova, 33 viaDodecaneso, 16146, Genova, I. R. Tre, 84 viadellaVascaNavale, 00146, Roma, Department of PhysicsE. Pancini, U. Federico, 6. ViaCinthia, 80126, Napoli, U. Porto, Caup, Rua das Estrelas, P. Porto, U. Torino, 1. ViaP.Giuria, 10125 Torino, I. Torino, Inaf-Iasf Milano, 12 ViaAlfonsoCorti, 20133 Milano, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, 08193 Bellaterra, Spain., Port d'Informaci'o Cient'ifica, C. Sn, I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, Institute of Space Sciences, Carrer de Can Magrans, sn., 08193 Barcelona, I. -. Capodimonte, 16 viaMoiariello, 80131 Napoli, I. Naples, D. Bologna, Centre National d'Etudes Spatiales, Toulouse, Institut national de physique nucl'eaire et de physique des particules, 3. R. Michel-Ange, 16 75794ParisC'edex, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, J. B. C. F. Astrophysics, D. Physics, Astronomy, U. Manchester, Oxford Road, M13 9PL, Esacesa, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Mullard Space Science Laboratory, U. London, H. Mary, Dorking, Surrey RH5 6NT, 1049-001 Lisboa, D. O. Astronomy, U. Geneva, 16 ch.d'Ecogia, I. D. A. E. P. Spaziali, V. Cavaliere, 100, 00133 Roma, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, I. Lyon, Umr 5822, 69622, Villeurbanne, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, Inaf - Padova, 5. Viadell'Osservatorio, 35131 Padova, M. F. P. Physics, 1. Giessenbachstr., 85748 Garching, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, L. Observatory, Leiden University, 2. NielsBohrweg, 2333 CA Leiden, The Netherlands., Jet propulsion Laboratory, C. I. O. Technology., 4800 Oak Grove Drive, Pasadena, Ca, 91109, T. Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark., Cosmic Dawn Center, I. Paris, 98 bis boulevard Arago, 75014, París, M. Astronomie, 17 Konigstuhl, 69117 Heidelberg, Nasa Goddard Space Flight Center, Greenbelt, MD 20771, U. Geneve, D'epartement de Physique Th'eorique, Centre for Theoretical Physics, 24 quai Ernest-Ansermet, 4. CH-1211Geneve, 64 P.O.Box, 0. Helsinki, Finland., H. I. O. Physics, 2. GustafHallstrominkatu, U. Helsinki, Helsinki, Institute of Theoretical Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, Nova Optical IR Instrumentation Group at Astron, 4. OudeHoogeveensedijk, 7991PD, Dwingeloo, Institute for Computational Cosmology, D. University, South Road, DH1 3LE, Astroparticule et Cosmologie, 7. Paris, Umr 7095, Sorbonne Universit'e, 98 bis boulevard Arago, 7. Paris, European Space AgencyESTEC, 1. Keplerlaan, 2. Noordwijk, K. Institute, U. Groningen, PO Box 800, 9700 AV Groningen, U. Aarhus, Ny Munkegade 120, C. DK-8000Aarhus, S. Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Institute of Space Science, Bucharest, 077125, România, Dipartimento di Fisica e AstronomiaG.Galilei, U. Padova, 8. viaMarzolo, 35131 Padova, INFN-Padova, D. Astronomia, U. Bologna, V. G. 932, Fcfm, U. D. Chile, Blanco Encalada 2008, Santiago, Chile., Institut fur Teilchenphysik, U. Innsbruck, Technikerstr. 258, 6020 Innsbruck, Austria, Cppm, Institut de Ci'encies de l'Espai, sn Cerdanyola del Vall'es, Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, 40 AvenidaComplutense, 28014 Madrid, Universidad Polit'ecnica de Cartagena +499 moresemanticscholar +1 more sourceOptimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) [PDF]
Astrophysical Journal, 2022 We present the first comprehensive release of photometric redshifts (photo- z's) from the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) team.D. Kodra, B. Andrews, J. Newman, S. Finkelstein, A. Fontana, N. Hathi, M. Salvato, T. Wiklind, S. Wuyts, Adam Broussard, N. Chartab, C. Conselice, M. Cooper, A. Dekel, M. Dickinson, H. Ferguson, E. Gawiser, N. Grogin, Kartheik G. Iyer, J. Kartaltepe, S. Kassin, A. Koekemoer, D. Koo, R. Lucas, K. Mantha, D. H. Mcintosh, B. Mobasher, C. Pacifici, P. P'erez-Gonz'alez, P. S. D. O. Physics, Astronomy, U. Pittsburgh, Pittsburgh Particle Physics, Astrophysics, C. Center, D. O. Astronomy, T. U. O. T. A. Austin, Oss. Astronomico di Roma, Space Telescope Science Institute, Max-Planck-Institut fur extraterrestrische Physik, D. Physics, Catholic University of America, U. Bath, Rutgers, The State University of New Jersey, U. California, Irvine, J. B. C. F. Astrophysics, U. Manchester, Center for Particle Cosmology, D. PhysicsAstronomy, R. I. O. Physics, The Hebrew University, NSF's NOIRlab, D. I. F. Astronomy, U. Toronto, S. O. Physics, R. I. O. Technology, T. W. H. M. I. D. O. PhysicsAstronomy, J. University, Santa Cruz, M. I. F. Astrophysics, U. Minnesota, University of Missouri, Kansas City, Riverside, C. D. Astrobiolog'ia, CABCSIC-INTA, C. Ajalvir +68 moresemanticscholar +1 more sourceOn Periodic Groups Saturated with Finite Frobenius Groups
Известия Иркутского государственного университета: Серия "Математика", 2021 A group is called weakly conjugate biprimitively finite if each its element of prime order generates a finite subgroup with any of its conjugate elements. A binary finite group is a periodic group in which any two elements generate a finite subgroup. If $B. E. Durakov, A.I. Sozutovdoaj +1 more sourceOn Two Properties of Shunkov Group
Известия Иркутского государственного университета: Серия "Математика", 2021 One of the interesting classes of mixed groups ( i.e. groups that can contain both elements of finite order and elements of infinite order) is the class of Shunkov groups.
The group $G$ is called Shunkov group if for any
finite subgroup $H$ of $G$ in the A.A. Shlepkin, I. V. Sabodakhdoaj +1 more sourceA spatial-temporal short-term traffic flow prediction model based on dynamical-learning graph convolution mechanism [PDF]
Information Sciences, 2022 Short-term traffic flow prediction is a vital branch of the Intelligent Traffic System (ITS) and plays an important role in traffic management. Graph convolution network (GCN) is widely used in traffic prediction models to better deal with the graphical structure Zhijun Chen, Zheng Lu, Qiushi Chen, Hongliang Zhong, Yishi Zhang, Jie Xue, Chaozhong Wu Intelligent Transportation Systems Research Center, Wuhan University of Technology, Wuhan, China., School of Transportation, Logistics Engineering, School of Materials Science, Technology, School of Management, Faculty of Information Technology, Policy., Management, Safety, Security Science Group, Delft University of Technology, Delft, The Netherlands +22 moresemanticscholar +1 more sourceSwiss Sepsis National Action Plan: A coordinated national action plan to stop sepsis-related preventable deaths and to improve the support of people affected by sepsis in Switzerland
Frontiers in Medicine, 2023 Background Sepsis is a devastating disease which causes yearly over 10 million deaths worldwide. In 2017, the World Health Organization (WHO) issued a resolution prompting member states to improve the prevention, recognition, and management of sepsis ...L. Schlapbach, E. Zimmermann, S. Meylan, M. Stocker, P. Suter, S. Jakob, on behalf of the Swiss Sepsis National Action Plan Working Group +6 moresemanticscholar +1 more source
