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Euclid preparation. XVIII. The NISP photometric system [PDF]
Astronomy & Astrophysics, 2022 Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95-2.02 $\mu$m range, to a 5$\sigma$ point-source median depth of 24.4 AB mag. This unique photometric data set will find wide use beyond Euclid's core science.Euclid Collaboration M. Schirmer, K. Jahnke, G. Seidel, H. Aussel, C. Bodendorf, F. Grupp, F. Hormuth, S. Wachter, P. Appleton, R. Barbier, J. Brinchmann, J. M. Carrasco, F. Castander, J. Coupon, F. Paolis, A. Franco, K. Ganga, P. Hudelot, E. Jullo, A. Lançon, A. Nucita, S. Paltani, G. Smadja, L. Venancio, F. Strafella, M. Weiler, A. Amara, T. Auphan, N. Auricchio, A. Balestra, R. Bender, D. Bonino, E. Branchini, M. Brescia, V. Capobianco, C. Carbone, J. Carretero, R. Casas, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, Y. Copin, L. Corcione, A. Costille, F. Courbin, A. D. Silva, H. Degaudenzi, M. Douspis, F. Dubath, X. Dupac, S. Dusini, A. Ealet, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, L. Guzzo, S. Haugan, H. Hoekstra, W. Holmes, A. Hornstrup, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, M. Kummel, M. Kunz, H. Kurki-Suonio, R. Laureijs, S. Ligori, P. Lilje, I. Lloro, T. Maciaszek, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, S. Maurogordato, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, E. Munari, R. Nakajima, R. Nichol, S. Niemi, C. Padilla, F. Pasian, K. Pedersen, W. Percival, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, É. Prieto, F. Raison, J. Rhodes, H. Rix, M. Roncarelli, E. Rossetti, R. Saglia, B. Sartoris, R. Scaramella, P. Schneider, A. Secroun, S. Serrano, C. Sirignano, G. Sirri, L. Stanco, P. Tallada-Cresp'i, A. Taylor, H. Teplitz, I. Tereno, R. Toledo-Moreo, F. Torradeflot, M. Trifoglio, E. Valentijn, L. Valenziano, Y. Wang, J. Weller, G. Zamorani, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, S. Camera, R. Farinelli, J. Graci'a-Carpio, D. Maino, E. Medinaceli, S. Mei, N. Morisset, G. Polenta, A. Renzi, E. Romelli, M. Tenti, T. Vassallo, A. Zacchei, E. Zucca, C. Baccigalupi, A. Balaguera-Antol'inez, A. Biviano, A. Blanchard, S. Borgani, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, C. Carvalho, S. Casas, G. Castignani, C. Colodro-Conde, A. Cooray, H. Courtois, M. Crocce, J. Cuby, S. Davini, S. D. Torre, D. Ferdinando, J. Escartín, M. Farina, P. Ferreira, F. Finelli, S. Fotopoulou, S. Galeotta, J. García-Bellido, E. Gaztañaga, K. George, G. Gozaliasl, I. Hook, S. Ili'c, Vanshika Kansal, A. Kashlinsky, E. Keihanen, C. Kirkpatrick, V. Lindholm, G. Mainetti, R. Maoli, M. Martinelli, N. Martinet, M. Maturi, N. Mauri, H. McCracken, R. Metcalf, P. Monaco, G. Morgante, J. Nightingale, L. Patrizii, A. Peel, V. Popa, C. Porciani, D. Potter, P. Reimberg, G. Riccio, A. S'anchez, D. Sapone, V. Scottez, E. Sefusatti, R. Teyssier, I. Tutusaus, C. Valieri, J. Valiviita, M. Viel, H. D. A. F. Astronomie, 17 Konigstuhl, D. Heidelberg, H Germany, Aim, Cea, Cnrs, Universit'e Paris-Saclay, U. Paris, F-91191 Gif-sur-Yvette, France, M. F. P. Physics, 1. Giessenbachstr., D. Garching, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, C. Observatories, Pasadena, CA 91101, Usa, Infrared Processing, A. Center, C. I. O. Technology., CA 91125, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, I. Lyon, Umr 5822, F-69622, Villeurbanne, Centro de Astrof'isica da Universidade do Porto, Rua das Estrelas, 4169-007 Porto, Portugal, I. D. A. E. C. D. Espaco, U. Porto, Caup, P. Porto, Institut de Ci'encies del Cosmos, U. Barcelona, 1. MartiiFranques, 08193 Barcelona, Spain., I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, Institute of Space Sciences, Campus Uab, Carrer de Can Magrans, sn., 08193 Barcelona, D. O. Astronomy, U. 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Science, Technology, 08193 Bellaterra, Port d'Informacio Cientifica, C. Sn, I. Roma, 33 viaFrascati, I. Catone, Department of PhysicsE. Pancini, U. Federico, 6. ViaCinthia, I-80126, Napoli, I. Naples, D. Bologna, 62 vialeBertiPichat, I. Bologna, Inaf - Arcetri, 5. LargoE.Fermi, I-50125, Firenze, Centre National d'Etudes Spatiales, Toulouse, Institut national de physique nucl'eaire et de physique des particules, 3. R. Michel-Ange, 16 75794ParisCedex, 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, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, D. D. Fisica, F. Ciencias, Universidade de Lisboa, C. Edificio, C. Grande, P. Lisboa, P. Lisboa, I. D. Spatiale, 91405, Orsay, INFN-Padova, 8. viaMarzolo, Inaf - Padova, Inaf Trieste, 11 ViaG.B.Tiepolo, I. Trieste, Istituto Nazionale di Astrofisica - Osservatorio di Astrofi Spazio, V. G. 933, Istituto Nazionale Fisica Nucleare, Sezione Infn di Bologna, 46 ViaIrnerio, I. Bologna, Dipartimento di FisicaAldo Pontremoli, U. Milano, 16 viaCeloria, I. Brera, 28 ViaBrera, Infn Milano, Infn Milano, Institute of Theoretical Astrophysics, U. Oslo, P. O. B. 1. Blindern, N. Oslo, Norway, L. Observatory, Leiden University, 2. NielsBohrweg, 2333 CA Leiden, Jet propulsion Laboratory, 4800 Oak Grove Drive, Ca, 91109, T. Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark., Mullard Space Science Laboratory, U. London, H. Mary, Dorking, Surrey RH5 6NT, U. Geneve, Departement de Physique Theorique, Centre for Theoretical Physics, 24 quai Ernest-Ansermet, 4. CH-1211Geneve, H. I. O. Physics, 2. GustafHallstrominkatu, 0. Helsinki, Finland., Nova Optical IR Instrumentation Group at Astron, 4. OudeHoogeveensedijk, 7991PD, Dwingeloo, Argelander Institut fur Astronomie, U. Bonn, 71 AufdemHugel, 53121 Bonn, D. Bologna, V. G. 932, I. Bologna, Institute for Computational Cosmology, D. University, South Road, Durham, DH1 3LE, Universit'e Cote d'Azur, Observatoire Cote d'Azur, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 4. 06304Nicecedex, C. Saclay, Dfrirfu, S. d’Astrophysique, Bat. 709, 91191 Gif-sur-Yvette, Sorbonne Universités, U. U. P. 6. E. Cnrs, Umr 7095, 98 bis bd Arago, 7. Paris, U. Aarhus, Ny Munkegade 120, C. DK-8000Aarhus, Centre for Gravitational Astrophysics, U. Waterloo, Waterloo, Ontario N2L 3G1, Canada, P. I. O. T. Physics, Ontario N2L 2Y5, Institute of Space Science, Bucharest, Ro-077125, România, M. F. Astrophysik, 1. Karl-SchwarzschildStr. +499 moresemanticscholar +1 more sourceOn Shunkov Groups Saturated with Finite Groups
Известия Иркутского государственного университета: Серия "Математика", 2018 The structure of the group consisting of elements of finite order depends to a large extent on the structure of the finite subgroups of the group under consideration. One of the effective conditions for investigating an infinite group containing elements A.A. Shlepkindoaj +1 more sourceGenomic Epidemiology of SARS-CoV-2 in Madrid, Spain, during the First Wave of the Pandemic: Fast Spread and Early Dominance by D614G Variants
Microorganisms, 2021 Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) was first detected in Madrid, Spain, on 25 February 2020. It increased in frequency very fast and by the end of May more than 70,000 cases had been confirmed by reverse transcription-polymerase E. Viedma, E. Dahdouh, J. González-Alba, S. González-Bodí, L. Martínez-García, F. Lázaro-Perona, R. Recio, María Rodríguez-Tejedor, M. D. Folgueira, R. Cantón, R. Delgado, J. García-Rodríguez, J. Galán, J. Mingorance, On Behalf Of The Sars-CoV-Working Groups +14 moresemanticscholar +1 more sourceCrystal structure of {2,2′-[N,N′-bis(pyridin-2-ylmethyl)cyclohexane-trans-1,2-diyldi(nitrilo)]diacetato}cobalt(III) hexafluoridophosphate
Acta Crystallographica Section E: Crystallographic Communications, 2015 The title compound [Co(C22H26N4O4)]PF6, commonly known as [Co(bpcd)]PF6, where bpcd2− is derived from the historical ligand name N,N′-bis(2-pyridylmethyl)-trans-1,2-diaminocyclohexane-N,N′-diacetate, crystallized by slow evaporation of a saturated ...Craig C. McLauchlan, Daniel S. Kissel, Albert W. Herlinger +2 moredoaj +1 more sourceScientific advice related to nutrient profiling for the development of harmonised mandatory front‐of‐pack nutrition labelling and the setting of nutrient profiles for restricting nutrition and health claims on foods
EFSA Journal, 2022 Following a request from the European Commission, the EFSA Panel on Nutrition, Novel Foods and Food Allergens (NDA) was asked to deliver scientific advice related to nutrient profiling for the development of harmonised mandatory front‐of‐pack nutrition ...EFSA Panel on Nutrition, Novel Foods and Food Allergens (NDA), Dominique Turck, Torsten Bohn, Jacqueline Castenmiller, Stefaan de Henauw, Karen Ildico Hirsch‐Ernst, Helle Katrine Knutsen, Alexandre Maciuk, Inge Mangelsdorf, Harry J McArdle, Androniki Naska, Carmen Peláez, Kristina Pentieva, Frank Thies, Sophia Tsabouri, Marco Vinceti, Jean‐Louis Bresson, Alfonso Siani +17 moredoaj +1 more source
