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Results 1 - 49 of 49
  • Euclid: The potential of slitless infrared spectroscopy: A z=5.4 quasar and new ultracool dwarfs
    • Virtual Journal - Volume 23, Issue 27 - article #15
    • E. Ba~nados (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), V. Le Brun (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), S. Belladitta (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), I. Momcheva (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), D. Stern (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), J. Wolf (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), M. Ezziati (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), D. J. Mortlock (Astrophysics Group, Blackett Laboratory, Imperial College London, London SW7 2AZ, UK, Department of Mathematics, Imperial College London, London SW7 2AZ, UK), A. Humphrey (Instituto de Astrof'isica e Ci^encias do Espac{c}o, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal, DTx -- Digital Transformation CoLAB, Building 1, Azur'em Campus, University of Minho, 4800-058 Guimar~aes, Portugal), R. L. Smart (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, Department of Physics, Astronomy, Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK), S. L. Casewell (School of Physics, Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK), A. P'erez-Garrido (Departamento F'isica Aplicada, Universidad Polit'ecnica de Cartagena, Campus Muralla del Mar, 30202 Cartagena, Murcia, Spain), B. Goldman (International Space University, 1 rue Jean-Dominique Cassini, 67400 Illkirch-Graffenstaden, France, Universit'e de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, 67000 Strasbourg, France), E. L. Mart'in (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain, Universidad de La Laguna, Departamento de Astrof'isica, 38206 La Laguna, Tenerife, Spain), A. Mohandasan (Universite Marie et Louis Pasteur, CNRS, Observatoire des Sciences de l'Univers THETA Franche-Comte Bourgogne, Institut UTINAM, Observatoire de Besanc{c}on, BP 1615, 25010 Besanc{c}on Cedex, France), C. Reyl'e (Universite Marie et Louis Pasteur, CNRS, Observatoire des Sciences de l'Univers THETA Franche-Comte Bourgogne, Institut UTINAM, Observatoire de Besanc{c}on, BP 1615, 25010 Besanc{c}on Cedex, France), C. Dominguez-Tagle (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain, Universidad de La Laguna, Departamento de Astrof'isica, 38206 La Laguna, Tenerife, Spain), Y. Copin (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), E. Lusso (INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy, Dipartimento di Fisica e Astronomia, Universit`a di Firenze, via G. Sansone 1, 50019 Sesto Fiorentino, Firenze, Italy), Y. Matsuoka (Research Center for Space, Cosmic Evolution, Ehime University, 2-5 Bunkyo-cho, Matsuyama, Ehime 790-8577, Japan), K. McCarthy (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), F. Ricci (Department of Mathematics, Physics, Roma Tre University, Via della Vasca Navale 84, 00146 Rome, Italy, INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), H. -W. Rix (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), H. J. A. Rottgering (Leiden Observatory, Leiden University, Einsteinweg 55, 2333 CC Leiden, The Netherlands), J. -T. Schindler (Hamburger Sternwarte, University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany), J. R. Weaver (Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA), A. Allaoui (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), T. Bedrine (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), M. Castellano (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), P. -Y. Chabaud (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), G. Daste (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), F. Dufresne (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), J. Gracia-Carpio (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), M. K"ummel (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany), M. Moresco (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Scodeggio (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), C. Surace (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), D. Vibert (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), A. Balestra (INAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy), A. Bonnefoi (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), A. Caillat (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), F. Cogato (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), A. Costille (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), S. Dusini (INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), S. Ferriol (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), E. Franceschi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), W. Gillard (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), K. Jahnke (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), D. Le Mignant (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), S. Ligori (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), E. Medinaceli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), G. Morgante (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), F. Passalacqua (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy, INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), K. Paterson (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), S. Pires (Universit'e Paris-Saclay, Universit'e Paris Cit'e, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France), C. Sirignano (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy, INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), I. T. Andika (Technical University of Munich, TUM School of Natural Sciences, Physics Department, James-Franck-Str.~1, 85748 Garching, Germany, Max-Planck-Institut f"ur Astrophysik, Karl-Schwarzschild-Str.~1, 85748 Garching, Germany), H. Atek (Institut d'Astrophysique de Paris, UMR 7095, CNRS,, Sorbonne Universit'e, 98 bis boulevard Arago, 75014 Paris, France), D. Barrado (Centro de Astrobiolog'ia), S. Bisogni (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), C. J. Conselice (Jodrell Bank Centre for Astrophysics, Department of Physics, Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK), H. Dannerbauer (Instituto de Astrof'isica de Canarias), R. Decarli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), H. Dole (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), T. Dupuy (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), A. Feltre (INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy), S. Fotopoulou (School of Physics, HH Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL, UK), B. Gillis (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), X. Lopez Lopez (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Onoue (Kavli Institute for the Physics, Mathematics of the Universe, Center for Data-Driven Discovery, Kavli IPMU), G. Rodighiero (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy, INAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy), N. Sedighi (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain, Universidad de La Laguna, Departamento de Astrof'isica, 38206 La Laguna, Tenerife, Spain), F. Shankar (School of Physics & Astronomy, University of Southampton, Highfield Campus, Southampton SO17 1BJ, UK), M. Siudek (Instituto de Astrof'isica de Canarias, Institute of Space Sciences), L. Spinoglio (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), D. Vergani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), G. Vietri (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), F. Walter (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), G. Zamorani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. R. Zapatero Osorio (Centro de Astrobiolog'ia), J. -Y. Zhang (Universidad de La Laguna, Departamento de Astrof'isica, 38206 La Laguna, Tenerife, Spain, Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain), M. Bethermin (Universit'e de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, 67000 Strasbourg, France), N. Aghanim (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), B. Altieri (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Ca~nada, Madrid, Spain), A. Amara (School of Mathematics, Physics, University of Surrey, Guildford, Surrey, GU2 7XH, UK), S. Andreon (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), C. Baccigalupi (IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, SISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy), M. Baldi (Dipartimento di Fisica e Astronomia, Universit`a di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), S. Bardelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), A. Basset (Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France), P. Battaglia (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), A. Biviano (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy), A. Bonchi (Space Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy), D. Bonino (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), E. Branchini (Dipartimento di Fisica, Universit`a di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), M. Brescia (Department of Physics "E. Pancini", University Federico II, Via Cinthia 6, 80126, Napoli, Italy, INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), J. Brinchmann (Instituto de Astrof'isica e Ci^encias do Espac{c}o, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal, Faculdade de Ci^encias da Universidade do Porto, Rua do Campo de Alegre, 4150-007 Porto, Portugal), S. Camera (Dipartimento di Fisica, Universit`a degli Studi di Torino, Via P. Giuria 1, 10125 Torino, Italy, INFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy, INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), V. Capobianco (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), C. Carbone (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), J. Carretero (Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, Port d'Informaci'o Cient'ifica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), S. Casas (Institute for Theoretical Particle Physics, Cosmology), G. Castignani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), S. Cavuoti (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, INFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy), A. Cimatti (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), C. Colodro-Conde (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain), G. Congedo (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), L. Conversi (European Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, Italy, ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Ca~nada, Madrid, Spain), F. Courbin (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F'ed'erale de Lausanne, Institut de Ci`encies del Cosmos, Instituci'o Catalana de Recerca i Estudis Avanc{c}ats), H. M. Courtois (UCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, 69622 Villeurbanne, France), M. Cropper (Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK), J. -G. Cuby (Canada-France-Hawaii Telescope, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743, USA, Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), A. Da Silva (Departamento de F'isica, Faculdade de Ci^encias, Universidade de Lisboa, Edif'icio C8, Campo Grande, PT1749-016 Lisboa, Portugal, Instituto de Astrof'isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal), H. Degaudenzi (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), G. De Lucia (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), A. M. Di Giorgio (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), C. Dolding (Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK), F. Dubath (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), C. A. J. Duncan (Jodrell Bank Centre for Astrophysics, Department of Physics, Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK), X. Dupac (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Ca~nada, Madrid, Spain), A. Ealet (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), M. Farina (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), F. Faustini (Space Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy, INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), N. Fourmanoit (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), M. Frailis (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), S. Galeotta (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), K. George (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany), C. Giocoli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), B. R. Granett (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), A. Grazian (INAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy), F. Grupp (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany), L. Guzzo (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy, INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, INFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy), S. V. H. Haugan (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), J. Hoar (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Ca~nada, Madrid, Spain), H. Hoekstra (Leiden Observatory, Leiden University, Einsteinweg 55, 2333 CC Leiden, The Netherlands), W. Holmes (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), I. Hook (Department of Physics, Lancaster University, Lancaster, LA1 4YB, UK), F. Hormuth (Felix Hormuth Engineering, Goethestr. 17, 69181 Leimen, Germany), A. Hornstrup (Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark, Cosmic Dawn Center), P. Hudelot (Institut d'Astrophysique de Paris, UMR 7095, CNRS,, Sorbonne Universit'e, 98 bis boulevard Arago, 75014 Paris, France), M. Jhabvala (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA), B. Joachimi (Department of Physics, Astronomy, University College London, Gower Street, London WC1E 6BT, UK), E. Keih"anen (Department of Physics, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, 00014 University of Helsinki, Finland), S. Kermiche (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), B. Kubik (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), K. Kuijken (Leiden Observatory, Leiden University, Einsteinweg 55, 2333 CC Leiden, The Netherlands), M. Kunz (Universit'e de Gen`eve, D'epartement de Physique Th'eorique, Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, CH-1211 Gen`eve 4, Switzerland), H. Kurki-Suonio (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), P. B. Lilje (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), V. Lindholm (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), I. Lloro (NOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD, Dwingeloo, The Netherlands), G. Mainetti (Centre de Calcul de l'IN2P3/CNRS, 21 avenue Pierre de Coubertin 69627 Villeurbanne Cedex, France), D. Maino (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy, INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, INFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy), E. Maiorano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), O. Mansutti (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), O. Marggraf (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Auf dem H"ugel 71, 53121 Bonn, Germany), K. Markovic (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), M. Martinelli (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, INFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy), N. Martinet (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), F. Marulli (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), R. Massey (Department of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, UK), S. Mei (Universit'e Paris Cit'e, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, CNRS-UCB International Research Laboratory, Centre Pierre Bin'etruy, IRL2007, CPB-IN2P3, Berkeley, USA), Y. Mellier (Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, France, Institut d'Astrophysique de Paris, UMR 7095, CNRS,, Sorbonne Universit'e, 98 bis boulevard Arago, 75014 Paris, France), M. Meneghetti (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), E. Merlin (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), G. Meylan (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F'ed'erale de Lausanne), A. Mora (Aurora Technology for European Space Agency), L. Moscardini (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), C. Neissner (Institut de F'isica d'Altes Energies, Port d'Informaci'o Cient'ifica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), S. -M. Niemi (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), J. W. Nightingale (School of Mathematics, Statistics, Physics, Newcastle University, Herschel Building, Newcastle-upon-Tyne, NE1 7RU, UK), C. Padilla (Institut de F'isica d'Altes Energies), S. Paltani (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), F. Pasian (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), K. Pedersen (DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark), W. J. Percival (Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada, Department of Physics, Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada, Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada), V. Pettorino (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), G. Polenta (Space Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy), M. Poncet (Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France), L. A. Popa (Institute of Space Science, Str. Atomistilor, nr. 409 Mu{a}gurele, Ilfov, 077125, Romania), L. Pozzetti (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), F. Raison (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), R. Rebolo (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain, Consejo Superior de Investigaciones Cientificas, Calle Serrano 117, 28006 Madrid, Spain, Universidad de La Laguna, Departamento de Astrof'isica, 38206 La Laguna, Tenerife, Spain), A. Renzi (Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy, INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), J. Rhodes (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), G. Riccio (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), E. Romelli (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), M. Roncarelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), E. Rossetti (Dipartimento di Fisica e Astronomia, Universit`a di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy), R. Saglia (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), Z. Sakr (Institut f"ur Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany, Institut de Recherche en Astrophysique et Plan'etologie, Universit'e St Joseph, Faculty of Sciences, Beirut, Lebanon), D. Sapone (Departamento de F'isica, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile), B. Sartoris (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), J. A. Schewtschenko (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), M. Schirmer (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), P. Schneider (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Auf dem H"ugel 71, 53121 Bonn, Germany), T. Schrabback (Universit"at Innsbruck, Institut f"ur Astro- und Teilchenphysik, Technikerstr. 25/8, 6020 Innsbruck, Austria), A. Secroun (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), E. Sefusatti (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy), G. Seidel (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), M. Seiffert (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), S. Serrano (Institut d'Estudis Espacials de Catalunya, Satlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, Spain, Institute of Space Sciences), G. Sirri (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), L. Stanco (INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), J. Steinwagner (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), P. Tallada-Cresp'i (Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, Port d'Informaci'o Cient'ifica, Campus UAB, C. Albareda s/n, 08193 Bellaterra), A. N. Taylor (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), H. I. Teplitz (Infrared Processing, Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA), I. Tereno (Departamento de F'isica, Faculdade de Ci^encias, Universidade de Lisboa, Edif'icio C8, Campo Grande, PT1749-016 Lisboa, Portugal, Instituto de Astrof'isica e Ci^encias do Espac{c}o, Faculdade de Ci^encias, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal), S. Toft (Cosmic Dawn Center, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark), R. Toledo-Moreo (Universidad Polit'ecnica de Cartagena, Departamento de Electr'onica y Tecnolog'ia de Computadoras, Plaza del Hospital 1, 30202 Cartagena, Spain), F. Torradeflot (Port d'Informaci'o Cient'ifica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas), I. Tutusaus (Institut de Recherche en Astrophysique et Plan'etologie), L. Valenziano (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), J. Valiviita (Department of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, Helsinki, Finland), T. Vassallo (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), G. Verdoes Kleijn (Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands), A. Veropalumbo (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, Dipartimento di Fisica, Universit`a di Genova, Via Dodecaneso 33, 16146, Genova, Italy), Y. Wang (Infrared Processing, Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA), J. Weller (Universit"ats-Sternwarte M"unchen, Fakult"at f"ur Physik, Ludwig-Maximilians-Universit"at M"unchen, Scheinerstrasse 1, 81679 M"unchen, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), F. M. Zerbi (INAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy), E. Zucca (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Bolzonella (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), C. Burigana (INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), R. Cabanac (Institut de Recherche en Astrophysique et Plan'etologie), L. Gabarra (Department of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK), V. Scottez (Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, France, ICL, Junia, Universit'e Catholique de Lille, LITL, 59000 Lille, France), M. Viel (IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, SISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, ICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy), D. Scott (Department of Physics, Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada)
    • https://arxiv.org/abs/2506.13945
  • Cross Section Measurements of Large Angle Fragments Production in the Interaction of Carbon Ion Beams with Thin Targets
    • Virtual Journal - Volume 23, Issue 2 - article #3
    • The FOOT Collaboration, Y. Dong (INFN Section of Milano, Milano, Italy), I. Mattei (INFN Section of Milano, Milano, Italy), A. Alexandrov (INFN Section of Napoli, Napoli, Italy), B. Alpat (INFN Section of Perugia, Perugia, Italy), G. Ambrosi (INFN Section of Perugia, Perugia, Italy), S. Argir`o (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Barbanera (INFN Section of Perugia, Perugia, Italy), N. Bartosik (INFN Section of Torino, Torino, Italy), G. Battistoni (INFN Section of Milano, Milano, Italy), M. G. Bisogni (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), V. Boccia (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), F. Cavanna (INFN Section of Torino, Torino, Italy), P. Cerello (INFN Section of Torino, Torino, Italy), E. Ciarrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), A. De Gregorio (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), G. De Lellis (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), A. Di Crescenzo (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), B. Di Ruzza (University of Foggia, Foggia, Italy, INFN Section of Bari, Bari, Italy), M. Dondi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Donetti (INFN Section of Torino, Torino, Italy, CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), M. Durante (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Faccini (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), V. Ferrero (INFN Section of Torino, Torino, Italy), C. Finck (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), E. Fiorina (INFN Section of Torino, Torino, Italy), M. Francesconi (INFN Section of Napoli, Napoli, Italy), M. Franchini (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), G. Franciosini (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), G. Galati (University of Bari, Department of Physics, Bari Italy, INFN Section of Bari, Bari, Italy), L. Galli (INFN Section of Pisa, Pisa, Italy), M. Ionica (INFN Section of Perugia, Perugia, Italy), A. Iuliano (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), K. Kanxheri (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), A. C. Kraan (INFN Section of Pisa, Pisa, Italy), C. La Tessa (University of Miami, Radiation Oncology, Miami, FL, United States, Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), A. Lauria (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Physics "E. Pancini", Napoli, Italy), E. Lopez Torres (INFN Section of Torino, Torino, Italy, CEADEN, Centro de Aplicaciones Tecnologicas y Desarrollo Nuclear, Havana, Cuba), M. Magi (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), A. Manna (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Marafini (INFN Section of Roma 1, Rome, Italy, Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy), M. Massa (INFN Section of Pisa, Pisa, Italy), C. Massimi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Mengarelli (INFN Section of Bologna, Bologna, Italy), A. Mereghetti (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), T. Minniti (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), A. Moggi (INFN Section of Pisa, Pisa, Italy), M. C. Montesi (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Chemistry, Napoli, Italy), M. C. Morone (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), M. Morrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), S. Muraro (INFN Section of Milano, Milano, Italy), N. Pastrone (INFN Section of Torino, Torino, Italy), V. Patera (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), F. Peverini (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), F. Pennazio (INFN Section of Torino, Torino, Italy), C. Pisanti (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), P. Placidi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Engineering, Perugia, Italy), M. Pullia (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Ramello (INFN Section of Torino, Torino, Italy, University of Piemonte Orientale, Department for Sustainable Development, Ecological Transition, Vercelli, Italy), C. Reidel (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Ridolfi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), L. Sabatini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), L. Salvi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), C. Sanelli (INFN Laboratori Nazionali di Frascati, Frascati, Italy), O. Sato (Nagoya University, Department of Physics, Nagoya, Japan), S. Savazzi (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Scavarda (Nagoya University, Department of Physics, Nagoya, Japan), A. Schiavi (INFN Section of Roma 1, Rome, Italy, Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), C. Schuy (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), E. Scifoni (University of Miami, Radiation Oncology, Miami, FL, United States), L. Servoli (INFN Section of Perugia, Perugia, Italy), G. Silvestre (INFN Section of Perugia, Perugia, Italy), M. Sitta (INFN Section of Torino, Torino, Italy, ALTEC, Aerospace Logistic Technology Engineering Company, Corso Marche 79, 10146 Torino, Italy), R. Spighi (INFN Section of Bari, Bari, Italy), E. Spiriti (University of Piemonte Orientale, Department for Sustainable Development, Ecological Transition, Vercelli, Italy), L. Testa (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), V. Tioukov (INFN Section of Napoli, Napoli, Italy), S. Tomassini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), F. Tommasino (University of Miami, Radiation Oncology, Miami, FL, United States, University of Trento, Department of Physics, Trento, Italy), M. Toppi (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria), A. Trigilio (INFN Laboratori Nazionali di Frascati, Frascati, Italy), G. Traini (INFN Section of Roma 1, Rome, Italy), G. Ubaldi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Valetti (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Vanstalle (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), M. Villa (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), U. Weber (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Zarrella (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Zoccoli (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Sarti (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria)
    • https://arxiv.org/abs/2501.04392
  • Angular differential and elemental fragmentation cross sections of a $400,text{MeV/nucleon}$ $^{16}text{O}$ beam on a graphite target with the FOOT experiment
    • Virtual Journal - Volume 23, Issue 1 - article #7
    • FOOT Collaboration, R. Ridolfi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Toppi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), A. Mengarelli (INFN Section of Bologna, Bologna, Italy), M. Dondi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Alexandrov (INFN Section of Napoli, Napoli, Italy), B. Alpat (INFN Section of Perugia, Perugia, Italy), G. Ambrosi (INFN Section of Perugia, Perugia, Italy), S. Argir`o (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Barbanera (INFN Section of Perugia, Perugia, Italy), N. Bartosik (INFN Section of Torino, Torino, Italy), G. Battistoni (INFN Section of Milano, Milano, Italy), M. G. Bisogni (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), V. Boccia (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), F. Cavanna (INFN Section of Torino, Torino, Italy), P. Cerello (INFN Section of Torino, Torino, Italy), E. Ciarrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), A. De Gregorio (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), G. De Lellis (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), A. Di Crescenzo (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), B. Di Ruzza (University of Foggia, Foggia, Italy, INFN Section of Bari, Bari, Italy), M. Donetti (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy, INFN Section of Torino, Torino, Italy), Y. Dong (INFN Section of Milano, Milano, Italy), M. Durante (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Faccini (University of Rome La Sapienza, Department of Physics, Rome, Italy, INFN Section of Roma 1, Rome, Italy), V. Ferrero (INFN Section of Torino, Torino, Italy), C. Finck (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), E. Fiorina (INFN Section of Torino, Torino, Italy), M. Francesconi (INFN Section of Napoli, Napoli, Italy), M. Franchini (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), G. Franciosini (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), G. Galati (University of Bari, Department of Physics, Bari, Italy, INFN Section of Bari, Bari, Italy), L. Galli (INFN Section of Pisa, Pisa, Italy), M. Ionica (INFN Section of Perugia, Perugia, Italy), A. Iuliano (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), K. Kanxheri (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), A. C. Kraan (INFN Section of Pisa, Pisa, Italy), C. La Tessa (University of Miami, Radiation Oncology, Miami, FL, United States, Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), A. Lauria (University of Napoli, Department of Physics "E. Pancini", Napoli, Italy, INFN Section of Napoli, Napoli, Italy), E. Lopez Torres (CEADEN, Centro de Aplicaciones Tecnologicas y Desarrollo Nuclear, Havana, Cuba, INFN Section of Torino, Torino, Italy), M. Magi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), A. Manna (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Marafini (Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Rome, Italy, INFN Section of Roma 1, Rome, Italy), M. Massa (INFN Section of Pisa, Pisa, Italy), C. Massimi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), I. Mattei (INFN Section of Milano, Milano, Italy), A. Mereghetti (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), T. Minniti (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), A. Moggi (INFN Section of Pisa, Pisa, Italy), M. C. Montesi (INFN Section of Napoli, Napoli, Italy, University of Napoli, Department of Chemistry, Napoli, Italy), M. C. Morone (University of Rome Tor Vergata, Department of Physics, Rome, Italy, INFN Section of Roma Tor Vergata, Rome, Italy), M. Morrocchi (University of Pisa, Department of Physics, Pisa, Italy, INFN Section of Pisa, Pisa, Italy), S. Muraro (INFN Section of Milano, Milano, Italy), N. Pastrone (INFN Section of Torino, Torino, Italy), V. Patera (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), F. Peverini (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), F. Pennazio (INFN Section of Torino, Torino, Italy), C. Pisanti (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), P. Placidi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Engineering, Perugia, Italy), M. Pullia (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Ramello (INFN Section of Torino, Torino, Italy, University of Piemonte Orientale, Department for Sustainable Development, Ecological Transition, Vercelli, Italy), C. Reidel (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), L. Sabatini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), L. Salvi (INFN Section of Perugia, Perugia, Italy, University of Perugia, Department of Physics, Geology, Perugia, Italy), C. Sanelli (INFN Laboratori Nazionali di Frascati, Frascati, Italy), A. Sarti (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), O. Sato (Nagoya University, Department of Physics, Nagoya, Japan), S. Savazzi (CNAO Centro Nazionale di Adroterapia Oncologica, Pavia, Italy), L. Scavarda (ALTEC, Aerospace Logistic Technology Engineering Company, Corso Marche 79, 10146 Torino, Italy), A. Schiavi (University of Rome La Sapienza, Department of Scienze di Base e Applicate per l'Ingegneria, INFN Section of Roma 1, Rome, Italy), C. Schuy (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), E. Scifoni (Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), L. Servoli (INFN Section of Perugia, Perugia, Italy), G. Silvestre (INFN Section of Perugia, Perugia, Italy), M. Sitta (INFN Section of Torino, Torino, Italy, University of Piemonte Orientale, Department of Science, Technological Innovation, Alessandria, Italy), R. Spighi (INFN Section of Bologna, Bologna, Italy), E. Spiriti (INFN Laboratori Nazionali di Frascati, Frascati, Italy), L. Testa (INFN Section of Roma 1, Rome, Italy, University of Rome La Sapienza, Department of Physics, Rome, Italy), V. Tioukov (INFN Section of Napoli, Napoli, Italy), S. Tomassini (INFN Laboratori Nazionali di Frascati, Frascati, Italy), F. Tommasino (University of Trento, Department of Physics, Trento, Italy, Trento Institute for Fundamental Physics, Applications, Istituto Nazionale di Fisica Nucleare), A. Trigilio (INFN Laboratori Nazionali di Frascati, Frascati, Italy), G. Traini (INFN Section of Roma 1, Rome, Italy), G. Ubaldi (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Valetti (University of Torino, Department of Physics, Torino, Italy, INFN Section of Torino, Torino, Italy), M. Vanstalle (Universit'e de Strasbourg, CNRS, IPHC UMR 7871, F-67000 Strasbourg, France), U. Weber (Biophysics Department, GSI Helmholtzzentrum f"ur Schwerionenforschung, Darmstadt, Germany), R. Zarrella (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), A. Zoccoli (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy), M. Villa (INFN Section of Bologna, Bologna, Italy, University of Bologna, Department of Physics, Astronomy, Bologna, Italy)
    • https://arxiv.org/abs/2501.00553
  • Nucleosynthesis Conditions in Outflows of White Dwarfs Collapsing to Neutron Stars
  • Magnetic dipole strength in $^{58}$Ni from forward-angle inelastic proton scattering
    • Virtual Journal - Volume 22, Issue 17 - article #7
    • I. Brandherm (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany), P. von Neumann-Cosel (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany), R. Mancino (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany, GSI Helmholzzentrum f"ur Schwerionenforschung, Planckstra{ss}e 1, Darmstadt, Germany, , Faculty of Mathematics, Physics, Charles University, Prague, Czech Republic), G. Mart'inez-Pinedo (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany, GSI Helmholzzentrum f"ur Schwerionenforschung, Planckstra{ss}e 1, Darmstadt, Germany), H. Matsubara (Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka, Japan, Faculty of Radiological Technology, Fujita Health University, Aichi, Japan), V. Yu. Ponomarev (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany), A. Richter (Institut f"ur Kernphysik, Technische Universit"at Darmstadt, Darmstadt, Germany), M. Scheck (School of Computing, Engineering,, Physical Sciences, University of the West of Scotland, Paisley, United Kingdom, SUPA, Scottish Universities Physics Alliance, Glasgow, United Kingdom), A. Tamii (Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka, Japan)
    • https://arxiv.org/abs/2404.15906
  • First Detection of the Powerful Gamma Ray Burst GRB221009A by the THEMIS ESA and SST particle detectors on October 9, 2022. (arXiv:2304.11225v1 [astro-ph.HE])
    • Virtual Journal - Volume 21, Issue 17 - article #4
    • O.V. Agapitov (1), M. Balikhin (2), A. J. Hull (1), Y.Hobara (3,4,5), V. Angelopoulos (6), F.S. Mozer (1) ((1) Space Sciences Laboratory, University of California, Berkeley, CA 94720, (2) University of Sheffield, Sheffield, UK, (3) Graduate School of Informatics, Engineering, The University of Electro-Communications (UEC), Chofu, Tokyo 1828585, Japan, (4) Center for Space Science, Radio Engineering, UEC, Chofu, Tokyo 1828585, Japan, (5) Research Center for Realizing Sustainable Societies, UEC, 1-5-1 Chofugaoka, Chofu, Tokyo 1828585, Japan (6) University of California Los Angeles, Los Angeles, CA)
    • http://arxiv.org/abs/2304.11225
  • Supernova remnants: Types and evolution. (arXiv:2211.02217v1 [astro-ph.HE])
  • The Galactic Chemical Evolution of phosphorus observed with IGRINS. (arXiv:2210.04940v1 [astro-ph.SR])
  • On the Use of Field RR Lyrae as Galactic Probes. III. The $alpha$-element abundances. (arXiv:2104.08113v1 [astro-ph.GA])
    • Virtual Journal - Volume 19, Issue 17 - article #2
    • J. Crestani (1,2,3), V.F. Braga (3,4), M. Fabrizio (3,4), G. Bono (2,3), C. Sneden (5), G.W. Preston (6), I. Ferraro (3), G. Iannicola (3), M. Nonino (7), G. Fiorentino (3), F. Thévenin (8), B. Lemasle (9), Z. Prudil (8), A. Alves-Brito (1), G. Altavilla (3,4), B. Chaboyer (10), M. Dall'Ora (11), V. D'Orazi (12,13), C.K. Gilligan (10), E. Grebel (8), A.J. Koch-Hansen (9), H. Lala (9), M. Marengo (14), S. Marinoni (3,4), P.M. Marrese (3,4), C.E. Martínez-Vázquez (15), N. Matsunaga (16), M. Monelli (17), J.P. Mullen (14), J. Neeley (18), R. da Silva (3,4), P.B. Stetson (19), M. Salaris (20), J. Storm (21), E. Valenti (22), M. Zoccali (23,24) ((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil, (2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy, (3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (4) Space Science Data Center, Roma, Italy, (5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA, (6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy, (8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France, (9) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany, (10) Department of Physics, Astronomy, Dartmouth College, Hanover, USA, (11) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (12) INAF-Osservatorio Astronomico di Padova, Padova, Italy, (13) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia, (14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (15) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile, (16) Department of Astronomy, The University of Tokyo, Tokyo, Japan, (17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (18) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA, (19) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada, (20) Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK, (21) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany, (22) European Southern Observatory, Garching bei Munchen, Germany, (23) Instituto Milenio de Astrofísica, Santiago, Chile, (24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
    • http://arxiv.org/abs/2104.08113
  • The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae II -- progenitor dependences --. (arXiv:2101.09618v1 [astro-ph.HE])
  • The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at $z approx0.6-1.8$. (arXiv:2010.15847v1 [astro-ph.GA])
  • The Age and Metallicity Dependence of the Near-Infrared Magnitudes of Red Clump Stars. (arXiv:1904.12874v1 [astro-ph.SR])
    • Virtual Journal - Volume 17, Issue 18 - article #6
    • Hiroki Onozato (1, 2), Yoshifusa Ita (1), Yoshikazu Nakada (3), Shogo Nishiyama (4) ((1) Astronomical Institute, Graduate School of Science, Tohoku University, Aramaki Aoba, Aoba-ku, Sendai, Miyagi, Japan, (2) Nishi-Harima Astronomical Observatory, Center for Astronomy, Institute of Natural, Environmental Sciences, University of Hyogo, Nishigaichi, Sayo-cho, Sayo-gun, Hyogo, Japan, (3) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Mitake, Kiso-machi, Kiso-gun, Nagano, Japan, (4) Miyagi University of Education, Aramaki Aoba, Aoba-ku, Sendai, Miyagi, Japan)
    • http://arxiv.org/abs/1904.12874
  • Hybrid stars from the NJL model with a tensor-interaction. (arXiv:1806.04377v1 [hep-ph])
  • Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources. (arXiv:1710.05504v1 [astro-ph.HE])
  • Light curve analysis of ordinary type IIP supernovae based on neutrino-driven explosion simulations in three dimensions. (arXiv:1704.03800v1 [astro-ph.SR])
  • Test of the Brink-Axel hypothesis for the pygmy dipole resonance. (arXiv:1611.01789v1 [nucl-ex])
  • Gamma strength function and level densities of $^{208}$Pb from forward-angle proton scattering at 295 MeV. (arXiv:1609.00937v1 [nucl-ex])
  • The Deuterium Fraction in Massive Starless Cores and Dynamical Implications
    • Virtual Journal - Volume 13, Issue 36 - article #24
    • Shuo Kong (1), Jonathan C. Tan (1 and 2), Paola Caselli (3), Francesco Fontani (4), Thushara Pillai (5 and 6), Michael J. Butler (7), Yoshito Shimajiri (8), Fumitaka Nakamura (9), Takeshi Sakai (10) ((1) Dept. of Astronomy, University of Florida, USA (2) Dept. of Physics, University of Florida, USA (3) Max-Planck-Institute for Extraterrestrial Physics (MPE), Germany, (4) INAF - Osservatorio Astrofisico di Arcetri, Italy, (5) California Institute of Technology, USA, (6) Max-Planck-Institute for Radioastronomy (MPIfR), Germany, (7) Institute for Computational Science, University of Zurich, Switzerland, (8) Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot, IRFU/Service d' Astrophysique, France, (9) National Astronomical Observatory of Japan, Japan, (10) Graduate School of Informatics and Engineering, The University of Electro-Communications, Japan)
    • arXiv.org - Astrophysics - Volume: 2015, Issue: 2 Oct
    • arXiv:1509.08684 [pdf, other]
  • Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf Spheroidal galaxy?
    • Virtual Journal - Volume 13, Issue 18 - article #4
    • L. Sbordone (1,2), L. Monaco (3,4), C. Moni Bidin (5), P. Bonifacio (6), S. Villanova (7), M. Bellazzini (8), R. Ibata (9), M. Chiba (10), D. Geisler (7), E. Caffau (6), S. Duffau (1,2) ((1) Millennium Institute for Astrophysics, Chile, (2) Pontificia Universidad Catolica de Chile, Santiago, Chile, (3) European Southern Observatory, Santiago, Chile, (4) Departamento de Ciencias Fisicas, Universidad Andres Bello, Santiago, Chile, (5) Instituto de Astronomia, Universidad Catolica del Norte, Antofagasta, Chile (6) GEPI, Observatoire de Paris, PSL Resarch University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cite, Meudon, France, (7) Departamento de Astronomia, Universidad de Concepcion, Concepcion, Chile, (8) INAF-Osservatorio Astronomico di Bologna, Bologna, Italy, (9) Observatoire Astronomique de Strasbourg, Universite de Strasbourg, CNRS, Strasbourg, France, (10) Astronomical Institute, Tohoku University, Sendai, Japan)
    • arXiv.org - Astrophysics - Volume: 2015, Issue: 8 May
    • arXiv:1505.01487 [pdf, other]
  • Fine structure of the isovector giant dipole resonance in 208Pb: Characteristic scales and level densities
    • Virtual Journal - Volume 12, Issue 14 - article #16
    • I. Poltoratska (1), R.W. Fearick (2), A.M. Krumbholz (1), E. Litvinova (3,4), H. Matsubara (5,6), P. von Neumann-Cosel (1), V.Yu. Ponomarev (1), A. Richter (1), A. Tamii (5) ((1) Institut für Kernphysik, Technische Universität Darmstadt, Germany, (2) Department of Physics, University of Cape Town, South Africa, (3) Department of Physics, Western Michigan University, USA, (4) National Superconducting Cyclotron Laboratory, Michigan State University, USA, (5) Research Center for Nuclear Physics, Osaka University, Japan, (6) National Institute of Radiological Sciences, Japan)
    • arXiv.org - Nuclear Experiment - Volume: 2014, Issue: 4 Apr
    • arXiv:1403.7652 [pdf, other]
  • Advanced burning stages and fate of 8-10 Mo stars
  • Main Sequence Star Populations in the Virgo Overdensity Region
    • Virtual Journal - Volume 11, Issue 13 - article #16
    • H. Jerjen (1), G.S. Da Costa (1), B. Willman (2), P. Tisserand (1), N. Arimoto (3,4), S. Okamoto (5), M. Mateo (6), I. Saviane (7), S. Walsh (8), M. Geha (9), A. Jordán (10,11), E. Olszewski (12), M. Walker (13), M. Zoccali (10,11), P. Kroupa (14) ((1) Research School of Astronomy and Astrophysics (2) Haverford College (3) National Astronomical Observatory of Japan (4) The Graduate University for Advanced Studies (5) Kavli Institute for Astronomy and Astrophysics (6) University of Michigan (7) European Southern Observatory (8) Australian Astronomical Observatory (9) Yale University (10) Pontificia Universidad Catolica de Chile (11) The Milky Way Millennium Nucleus (12) The University of Arizona (13) Harvard-Smithsonian Center for Astrophysics (14) Argelander Institute for Astronomy)
    • arXiv.org - Astrophysics - Volume: 2013, Issue: 29 Mar
    • arXiv:1303.5489 [pdf, other]
  • The Outer Halo of the Nearest Giant Elliptical: A VLT/VIMOS Survey of the Resolved Stellar Populations in Centaurus A to 85 kpc
    • Virtual Journal - Volume 11, Issue 12 - article #8
    • D. Crnojević, (1), A. M. N. Ferguson (1), M. J. Irwin (2), E. J. Bernard (1), N. Arimoto (3,4), P. Jablonka (5,6), C. Kobayashi (7,8) ((1) Institute for Astronomy, University of Edinburgh, Royal Observatory, UK, (2) Institute of Astronomy, Cambridge, UK, (3) Subaru Telescope, National Astronomical Observatory of Japan, Hawaii, USA, (4) Department of Astronomical Science, Graduate University for Advanced Studies, Tokyo, Japan, (5) Laboratoire d'Astrophysique, Ecole Polytechnique Fédérale de Lausanne, Switzerland, (6) GEPI, Observatoire de Paris, France, (7) School of Physics, Astronomy and Mathematics, University of Hertfordshire, UK, (8) Research School of Astronomy and Astrophysics, The Australian National University, Australia)
    • arXiv.org - Astrophysics - Volume: 2013, Issue: 22 Mar
    • arXiv:1303.4736 [pdf, ps, other]
  • Pygmy dipole resonance in 208Pb
  • Complete electric dipole response in 208Pb
  • Complete electric dipole response in 208Pb
  • The Case for the Dual Halo of the Milky Way
  • Chemical Abundances of the Outer Halo Stars in the Milky Way
  • Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. II. Ages, metallicities, detailed elemental abundances, and connections to the Galactic thick disc
    • Virtual Journal - Volume 7, Issue 48 - article #4
    • T. Bensby (1), S. Feltzing (2), J.A. Johnson (3), A. Gould (3), D. Adén (2), M. Asplund (4), J. Meléndez (5), A. Gal-Yam (6), S. Lucatello, (7) H. Sana (1 and 8), T. Sumi (9), N. Miyake (9), D. Suzuki (9), C. Han (10), I. Bond (11), A. Udalski (12) ((1) ESO, Chile, (2) Lund Observatory, Sweden, (3) Ohio state Univ., USA, (4) MPA-Garching, Germany, (5) Universidade do Porto, Portugal, (6) Benoziyo Center for Astrophysics, Weizmann Inst of Science, Israel, (7) INAF, Padova, Italy, (8) Universiteit van Amsterdam, Sterrenkundig Instituut, Netherlands, (9) Solar-Terrestrial Environment Laboratory, Nagoya Univ., Japan, (10) Chungbuk National Univ, Republic of Korea, (11) Massey Univ., New Zealand, (12) Warzaw University Observatory, Poland)
    • arXiv.org - Astrophysics - Volume: 2009, Issue: 26 Nov
    • arXiv:0911.5076 [ps, pdf, other]
  • Interpretation of CEMP(s) and CEMP(s + r) Stars with AGB Models
    • Virtual Journal - Volume 7, Issue 39 - article #4
    • S. Bisterzo (1), R. Gallino (1), O. Straniero (2), W. Aoki (3,4) ((1) Dipartimento di Fisica Generale, Università di Torino, Torino, Italy (2) INAF Osservatorio Astronomico di Collurania, Teramo, Italy (3) National Astronomical Observatory of Japan, Tokyo, Japan (4) Department of Astronomical Science, The Graduate University of Advanced Studies, Mitaka, Tokyo, Japan)
    • arXiv.org - Astrophysics - Volume: 2009, Issue: 25 Sep
    • arXiv:0909.3454 [ps, pdf, other]
  • What burns unstably on the neutron star of 4U 0614+091?
  • Structure and Kinematics of the Stellar Halos and Thick Disks of the Milky Way Based on Calibration Stars from SDSS DR7
  • Neutral absorber dips in the periodic burster LMXB XB 1323-619 from Suzaku
    • Virtual Journal - Volume 7, Issue 19 - article #7
    • M. Balucinska-Church (1,2), T. Dotani (3,4), T. Hirotsu (3,4), M.J. Church (1,2) ((1) University of Birmingham, U.K. (2) Jagiellonian University, Poland (3) Institute of Space and Astronautical Science, Japan (4) Tokyo Institute of Technology, Japan)
    • arXiv.org - Astrophysics - Volume: 2009, Issue: 8 May
    • arXiv:0905.0618 [ps, pdf, other]
  • The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
    • Virtual Journal - Volume 6, Issue 40 - article #5
    • M. Pignatari (1,2), R. Gallino (3,4), G. Meynet (5), R. Hirschi (1,6), F. Herwig (1,7), M. Wiescher (2) ((1) Keele University, Keele, UK, (2) JINA, University of Notre Dame, Notre Dame, IN, USA, (3) Dipartimento di Fisica Generale, Universita' di Torino, Via Pietro Giuria 1, Torino, Italy, (4) Center for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria, Australia, (5) Geneva Observatory, Sauverny, Switzerland, (6) IPMU, University of Tokyo, Kashiwa, Japan, (7) Department of Physics & Astronomy, University of Victoria, Victoria, BC, Canada)
    • arXiv.org - Astrophysics - Volume: 2008, Issue: 2 Oct
    • arXiv:0810.0182 [ps, pdf, other]
  • The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field Stars
  • The Dichotomy of the Galactic Halo of the Milky Way
  • Discovery of a New X-Ray Burst/Millisecond Accreting Pulsar HETE J1900.1-2455
  • Chemical Abundances in the Secondary Star of the Black Hole Binary V4641 Sagittarii (SAX J1819.3-2525)
  • The Epoch of Reionization
    • Virtual Journal - Volume 3, Issue 50 - article #5
    • A. J. Benson (1), Naoshi Sugiyama (2), Adi Nusser (3), C. G. Lacey (4) ((1) University of Oxford, UK, (2) NAOJ, Tokyo, Japan, (3) Technion, Haifa, Israel, (4) University of Durham (UK))
    • ArXiv – Astrophysics – December 2005
    • astro-ph/0512364 [abs, ps, pdf, other]
  • Long-term evolution of accretion disks around the neutron star in Be/X-ray binaries
    • Virtual Journal - Volume 3, Issue 47 - article #14
    • Kimitake Hayasaki (1,2), Atsuo T. Okazaki (3) ((1)Department of Applied Physics, Graduate School of Engineering, Hokkaido University, Kitaku N13W8, Sapporo 060-8628, Japan. (2)Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn Victoria 3122 Australia (3)Faculty of Engineering, Hokkai-Gakuen University, Toyohira-ku, Sapporo 062-8605, Japan)
    • ArXiv – Astrophysics – November 2005
    • astro-ph/0511527 [abs, ps, pdf, other]
  • Primordial binaries and intermediate mass black holes in globular clusters
    • Virtual Journal - Volume 3, Issue 34 - article #11
    • M. Trenti (1), E. Ardi (1), S. Mineshige (1), P. Hut (2) ((1) Yukawa Institute for Theoretical Physics Kyoto Japan, (2) Institute for Advanced Study Princeton NJ)
    • ArXiv - Astrophysics – August 2005
    • astro-ph/0508517 [ abs , ps , pdf , other ]
  • An Observational Pursuit for Population III Stars in a Ly_alpha Emitter at z=6.33 through HeII Emission
  • High velocity features in the spectra of the Type Ia SN 1999ee: a property of the explosion or evidence of circumstellar interaction?
    • Virtual Journal - Volume 2, Issue 47 - article #15
    • P.A. Mazzali (1,2,3,4), S. Benetti (5), M. Stehle (4,6), D. Branch (7), J. Deng (2,3), K. Maeda (2,3), K. Nomoto (2,3), M. Hamuy (8) ((1) INAF-Osservatorio Astronomico, Trieste, Italy, (2) Astronomy Dept., University of Tokyo, Japan, (3) Research Center for the Early Universe, University of Tokyo, Japan, (4) Max-Planck Institut fuer Astrophysik, Garching, Germany, (5) INAF-Osservatorio Astronomico, Padova, Italy, (6) Universitaets-Sternwarte Muenchen, Germany, (7) Astronomy Dept., Univ. of Oklahoma, Norman, OK, USA, (8) Carnegie Institution, Pasadena, CA, USA)
    • arXiv – Astrophysics – November 2004
    • astro-ph/0411566 [ abs , ps , pdf , other ]
  • Subaru/HDS Abundances in Three Giant Stars in the Ursa Minor Dwarf Spheroidal Galaxy
  • The Formation of Population III Binaries
  • A New Contributor to Chemical Evolution in High-Redshift Galaxies
    • Virtual Journal - Volume 2, Issue 26 - article #24
    • Takuji Tsujimoto (National Astronomical Observatory of Japan)
    • arXiv - Astrophysics – July 04
    • astro-ph/0406636 [ abs , ps , pdf , other ]
  • The Zenith Angle Distribution of Fully Contained Events in SuperKamiokande and the Impact of Quasi Elastic Scattering on their Direction
    • Virtual Journal - Volume 2, Issue 25 - article #23
    • E. Konishi (1), Y. Minorikawa (2), V.I. Galkin (3), M. Ishiwata (4), A. Misaki (5,6) ((1)Hirosaki University, Japan, (2)Kinki University, Japan, (3) Moscow State University, Russia, (4)Saitama University, Japan, (5)Waseda University, Japan, (6)Saitama University, Japan)
    • arXiv - Astrophysics – June 2004
    • astro-ph/0406497 [ abs , ps , pdf , other ]
  • A model of superoutbursts in binaries of SU UMa type
    • Virtual Journal - Volume 2, Issue 9 - article #11
    • D.V.Bisikalo(1), A.A.Boyarchuk(1), P.V.Kaygorodov(1), O.A.Kuznetsov(1,2), T.Matsuda(3) ((1) Institute of Astronomy of the Russian Acad. of Sci., Moscow, Russia; (2) Keldysh Institute of Applied Mathematics, Moscow, Russia; (3) Department of Earth and Planetary Sciences, Kobe University, Kobe, Japan)
    • arXiv.org – Astrophysics – March 2004
    • astro-ph/0403057 [ abs , ps , pdf , other ]
  • Disruption of a Dwarf Galaxy Under Strong Shocking: The Origin of omega Centauri
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