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  • Euclid preparation. LXXIV. Euclidised observations of Hubble Frontier Fields and CLASH galaxy clusters
    • Virtual Journal - Volume 23, Issue 27 - article #14
    • Euclid Collaboration, P. Bergamini (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), 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), G. Angora (Dipartimento di Fisica e Scienze della Terra, Universit`a degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), L. Bazzanini (Dipartimento di Fisica e Scienze della Terra, Universit`a degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), P. Rosati (Dipartimento di Fisica e Scienze della Terra, Universit`a degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), C. Grillo (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), M. Lombardi (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy), D. Abriola (Dipartimento di Fisica "Aldo Pontremoli", Universit`a degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy), A. Mercurio (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, Universita di Salerno, Dipartimento di Fisica "E.R. Caianiello", Via Giovanni Paolo II 132, I-84084 Fisciano, INFN -- Gruppo Collegato di Salerno - Sezione di Napoli, Dipartimento di Fisica "E.R. Caianiello", Universita di Salerno, via Giovanni Paolo II, 132 - I-84084 Fisciano), F. Calura (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), G. Despali (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), J. M. Diego (Instituto de F'isica de Cantabria, Edificio Juan Jord'a, Avenida de los Castros, 39005 Santander, Spain), R. Gavazzi (Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France, Institut d'Astrophysique de Paris, UMR 7095, CNRS,, Sorbonne Universit'e, 98 bis boulevard Arago, 75014 Paris, France), P. Hudelot (Institut d'Astrophysique de Paris, UMR 7095, CNRS,, Sorbonne Universit'e, 98 bis boulevard Arago, 75014 Paris, France), L. Leuzzi (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), G. Mahler (STAR Institute, University of Li`ege, Quartier Agora, All'ee du six Ao^ut 19c, 4000 Li`ege, Belgium, Department of Physics, Centre for Extragalactic Astronomy, Durham University, South Road, Durham, DH1 3LE, UK, Department of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, UK), E. Merlin (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), C. Scarlata (Minnesota Institute for Astrophysics, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, USA), 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), N. Auricchio (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, 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), R. Bender (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), 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), C. Bodendorf (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), 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, INFN section of Naples, Via Cinthia 6, 80126, 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), G. Ca~nas-Herrera (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, Institute Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands), 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), F. J. Castander (Institute of Space Sciences, Institut d'Estudis Espacials de Catalunya), M. Castellano (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), 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), K. C. Chambers (Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA), 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), C. J. Conselice (Jodrell Bank Centre for Astrophysics, Department of Physics, Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, 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), Y. Copin (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), F. Courbin (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F'ed'erale de Lausanne), 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), 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), J. Dinis (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. Dole (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), M. Douspis (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), F. Dubath (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), X. Dupac (ESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Ca~nada, Madrid, Spain), S. Dusini (INFN-Padova, Via Marzolo 8, 35131 Padova, Italy), S. Escoffier (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), M. Farina (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), R. Farinelli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), S. Farrens (Universit'e Paris-Saclay, Universit'e Paris Cit'e, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France), S. Ferriol (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), F. Finelli (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), M. Frailis (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), E. Franceschi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Fumana (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), S. Galeotta (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), B. Garilli (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, 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), B. Gillis (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), C. Giocoli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy), J. Gracia-Carpio (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), 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), S. V. H. Haugan (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), 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), K. Jahnke (Max-Planck-Institut f"ur Astronomie, K"onigstuhl 17, 69117 Heidelberg, Germany), E. Keih"anen (Department of Physics, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, 00014 Helsinki, Finland), S. Kermiche (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), A. Kiessling (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), M. Kilbinger (Universit'e Paris-Saclay, Universit'e Paris Cit'e, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France), B. Kubik (Universit'e Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France), 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. 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, University of Helsinki, 00014 Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, 00014 Helsinki, Finland), R. Laureijs (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), S. Ligori (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese), 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, University of Helsinki, 00014 Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, 00014 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. Maurogordato (Universit'e C^ote d'Azur, Observatoire de la C^ote d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France), E. Medinaceli (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), S. Mei (Universit'e Paris Cit'e, CNRS, Astroparticule et Cosmologie, 75013 Paris, France), 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), G. Meylan (Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique F'ed'erale de Lausanne), 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), 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), E. Munari (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), R. Nakajima (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Auf dem H"ugel 71, 53121 Bonn, Germany), 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, Department of Physics, Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, 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 (Department of Physics, Astronomy, University of Aarhus, Ny Munkegade 120, DK-8000 Aarhus C, Denmark), V. Pettorino (European Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands), S. Pires (Universit'e Paris-Saclay, Universit'e Paris Cit'e, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France), 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, 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), A. G. S'anchez (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), 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), 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), 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), S. Serrano (Institut d'Estudis Espacials de Catalunya, Institute of Space Sciences, Satlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, Spain), P. Simon (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Auf dem H"ugel 71, 53121 Bonn, Germany), 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), G. Sirri (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), A. Spurio Mancini (Department of Physics, Royal Holloway, University of London, Surrey TW20 0EX, UK, Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK), 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), 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, University of Helsinki, 00014 Helsinki, Finland, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, 00014 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 degli studi di Genova,, INFN-Sezione 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), G. Zamorani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, 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), A. Boucaud (Universit'e Paris Cit'e, CNRS, Astroparticule et Cosmologie, 75013 Paris, France), E. Bozzo (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), C. Burigana (INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, Italy, INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), M. Calabrese (Astronomical Observatory of the Autonomous Region of the Aosta Valley, INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), D. Di Ferdinando (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), J. A. Escartin Vigo (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), N. Mauri (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), 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. Tenti (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), 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), M. Wiesmann (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), Y. Akrami (Instituto de F'isica Te'orica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain, CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106, USA), V. Allevato (INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy), S. Anselmi (INFN-Padova, Via Marzolo 8, 35131 Padova, Italy, Dipartimento di Fisica e Astronomia "G. Galilei", Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy, Laboratoire Univers et Th'eorie, Observatoire de Paris, Universit'e PSL, Universit'e Paris Cit'e, CNRS, 92190 Meudon, France), M. Ballardini (Dipartimento di Fisica e Scienze della Terra, Universit`a degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy), M. Bethermin (Universit'e de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, 67000 Strasbourg, France, Aix-Marseille Universit'e, CNRS, CNES, LAM, Marseille, France), A. Blanchard (Institut de Recherche en Astrophysique et Plan'etologie), L. Blot (Kavli Institute for the Physics, Mathematics of the Universe, Laboratoire Univers et Th'eorie, Observatoire de Paris, Universit'e PSL, Universit'e Paris Cit'e, CNRS, 92190 Meudon, France), S. Borgani (Dipartimento di Fisica - Sezione di Astronomia, Universit`a di Trieste, Via Tiepolo 11, 34131 Trieste, Italy, 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), A. S. Borlaff (NASA Ames Research Center, Moffett Field, CA 94035, USA, Bay Area Environmental Research Institute, Moffett Field, California 94035, USA), S. Bruton (Minnesota Institute for Astrophysics, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, USA), R. Cabanac (Institut de Recherche en Astrophysique et Plan'etologie), A. Calabro (INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), A. Cappi (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, Universit'e C^ote d'Azur, Observatoire de la C^ote d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France), C. S. Carvalho (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), T. Castro (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, INFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, ICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy), S. Contarini (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), T. Contini (Institut de Recherche en Astrophysique et Plan'etologie), A. R. Cooray (Department of Physics & Astronomy, University of California Irvine, Irvine CA 92697, USA), O. Cucciati (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), B. De Caro (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), G. Desprez (Department of Astronomy & Physics, Institute for Computational Astrophysics, Saint Mary's University, 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, Canada), A. D'iaz-S'anchez (Departamento F'isica Aplicada, Universidad Polit'ecnica de Cartagena, Campus Muralla del Mar, 30202 Cartagena, Murcia, Spain), S. Di Domizio (Dipartimento di Fisica, Universit`a di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy), A. G. Ferrari (Dipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Universit`a di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), I. Ferrero (Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway), F. Fornari (INFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy), L. Gabarra (Department of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK), K. Ganga (Universit'e Paris Cit'e, CNRS, Astroparticule et Cosmologie, 75013 Paris, France), J. Garc'ia-Bellido (Instituto de F'isica Te'orica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain), V. Gautard (CEA Saclay, DFR/IRFU, Service d'Astrophysique, Bat. 709, 91191 Gif-sur-Yvette, France), E. Gaztanaga (Institute of Space Sciences, Institut d'Estudis Espacials de Catalunya, Institute of Cosmology, Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK), F. Giacomini (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), G. Gozaliasl (Department of Computer Science, Aalto University, PO Box 15400, Espoo, FI-00 076, Finland, Department of Physics, P.O. Box 64, University of Helsinki, 00014 Helsinki, Finland), A. Hall (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), H. Hildebrandt (Ruhr University Bochum, Faculty of Physics, Astronomy, Astronomical Institute), J. Hjorth (DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark), M. Huertas-Company (Instituto de Astrof'isica de Canarias, V'ia L'actea, 38205 La Laguna, Tenerife, Spain, Instituto de Astrof'isica de Canarias, Universit'e PSL, Observatoire de Paris, Sorbonne Universit'e, CNRS, LERMA, 75014, Paris, France, Universit'e Paris-Cit'e, 5 Rue Thomas Mann, 75013, Paris, France), A. Jimenez Mu~noz (Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France), J. J. E. Kajava (Department of Physics, Astronomy, Vesilinnantie 5, University of Turku, 20014 Turku, Finland, Serco for European Space Agency), V. Kansal (ARC Centre of Excellence for Dark Matter Particle Physics, Melbourne, Australia, Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia), D. Karagiannis (School of Physics, Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UK, Department of Physics, Astronomy, University of the Western Cape, Bellville, Cape Town, 7535, South Africa), C. C. Kirkpatrick (Department of Physics, Helsinki Institute of Physics, Gustaf H"allstr"omin katu 2, University of Helsinki, 00014 Helsinki, Finland), L. Legrand (ICTP South American Institute for Fundamental Research, Instituto de F'isica Te'orica, Universidade Estadual Paulista, S~ao Paulo, Brazil), G. Libet (Centre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France), A. Loureiro (Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, Stockholm, SE-106 91, Sweden, Astrophysics Group, Blackett Laboratory, Imperial College London, London SW7 2AZ, UK), G. Maggio (INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy), M. Magliocchetti (INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy), C. Mancini (INAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy), F. Mannucci (INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy), R. Maoli (Dipartimento di Fisica, Sapienza Universit`a di Roma, Piazzale Aldo Moro 2, 00185 Roma, Italy, INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy), C. J. A. P. Martins (Centro de Astrof'isica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal, Instituto de Astrof'isica e Ci^encias do Espac{c}o, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal), S. Matthew (Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), L. Maurin (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), R. B. Metcalf (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), P. Monaco (Dipartimento di Fisica - Sezione di Astronomia, Universit`a di Trieste, Via Tiepolo 11, 34131 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, IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy), C. Moretti (SISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, ICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, 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. Morgante (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), Nicholas A. Walton (Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK), J. Odier (Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France), L. Patrizii (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), A. Pezzotta (Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany), M. P"ontinen (Department of Physics, P.O. Box 64, University of Helsinki, 00014 Helsinki, Finland), V. Popa (Institute of Space Science, Str. Atomistilor, nr. 409 Mu{a}gurele, Ilfov, 077125, Romania), C. Porciani (Universit"at Bonn, Argelander-Institut f"ur Astronomie, Auf dem H"ugel 71, 53121 Bonn, Germany), D. Potter (Department of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland), I. Risso (Dipartimento di Fisica, Universit`a degli studi di Genova,, INFN-Sezione di Genova, via Dodecaneso 33, 16146, Genova, Italy), P. -F. Rocci (Universit'e Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France), M. Sahl'en (Theoretical astrophysics, Department of Physics, Astronomy, Uppsala University, Box 516, 751 37 Uppsala, Sweden), A. Schneider (Department of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland), M. Sereno (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. A. Stanford (Department of Physics, Astronomy, University of California, Davis, CA 95616, USA), C. Tao (Aix-Marseille Universit'e, CNRS/IN2P3, CPPM, Marseille, France), G. Testera (INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy), R. Teyssier (Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA), S. Tosi (Dipartimento di Fisica, Universit`a di Genova, Via Dodecaneso 33, 16146, Genova, Italy, INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy), A. Troja (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), M. Tucci (Department of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland), C. Valieri (INFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy), D. Vergani (INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), G. Verza (Center for Cosmology, Particle Physics, Department of Physics, New York University, New York, NY 10003, USA, Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USA)
    • https://arxiv.org/abs/2508.20860
  • 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
  • Current Galactic Chemical Evolution models fail to explain rising Na-abundances of young thick disc stars
    • Virtual Journal - Volume 23, Issue 18 - article #3
    • E. K. Owusu (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia, ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany), A. J. Ruiter (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia, ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany, OzGrav: The ARC Centre of Excellence for Gravitational Wave Discovery, Hawthorn, Australia), A. J. Kemp (Institute of Astronomy), S. Buder (ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Research School of Astronomy, Astrophysics, Australian National University, Australia), I. R. Seitenzahl (Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany), N. Rodriguez-Segovia (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia), R. Pakmor (Max Planck Institute for Astrophysics, Garching, Germany), G. C. Cinquegrana (ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, School of Physics, Astronomy, Monash University, Clayton, Australia), N. Storm (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberg University, Heidelberg, Germany), P. Eitner (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberg University, Heidelberg, Germany), M. Bergemann (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany)
    • https://arxiv.org/abs/2506.17711
  • The bright, dusty aftermath of giant eruptions & H-rich supernovae. Late interaction of supernova shocks & dusty circumstellar shells
  • Precision mass measurements of $^{74-76}$Sr using TITAN's Multiple-Reflection Time-of-Flight Mass Spectrometer
    • Virtual Journal - Volume 23, Issue 3 - article #9
    • Z. Hockenbery (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Manitoba, Winnipeg, Manitoba, Canada), T. Murb"ock (TRIUMF, Vancouver, British Columbia, Canada, II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany), B. Ashrafkhani (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Calgary, Calgary, Alberta, Canada), J. Bergmann (II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany), C. Brown (TRIUMF, Vancouver, British Columbia, Canada, School of Physics, Astronomy, University of Edinburgh, Edinburgh, United Kingdom), T. Brunner (Department of Physics, McGill University, Montr'eal, QC, Canada), J. Cardona (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Manitoba, Winnipeg, Manitoba, Canada), T. Dickel (II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany, GSI Helmholtzzentrum f"ur Schwerionenforschung GmbH, Darmstadt, Germany), E. Dunling (TRIUMF, Vancouver, British Columbia, Canada), J. D. Holt (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, McGill University, Montr'eal, QC, Canada), C. Hornung (GSI Helmholtzzentrum f"ur Schwerionenforschung GmbH, Darmstadt, Germany), B. S. Hu (National Center for Computational Sciences, Oak Ridge National Laboratory, Oak Ridge, Tennessee, USA, Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee, USA), C. Izzo (Facility for Rare Isotope Beams, East Lansing, Michigan, USA), A. Jacobs (Argonne National Laboratory, Lemont, Illinois, USA), A. Javaji (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Manitoba, Winnipeg, Manitoba, Canada), S. Kakkar (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Manitoba, Winnipeg, Manitoba, Canada), B. Kootte (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Manitoba, Winnipeg, Manitoba, Canada), G. Kripko-Koncz (II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany, Helmholtz Research Academy Hesse for FAIR), Ali Mollaebrahimi (GSI Helmholtzzentrum f"ur Schwerionenforschung GmbH, Darmstadt, Germany), D. Lascar (Center for Fundamental Physics, Northwestern University, Evanston, Illinois, USA), E. M. Lykiardopoulou (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of British Columbia, Vancouver, British Columbia, Canada), I. Mukul (TRIUMF, Vancouver, British Columbia, Canada), S. F. Paul (TRIUMF, Vancouver, British Columbia, Canada), W. R. Pla{ss} (II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany, GSI Helmholtzzentrum f"ur Schwerionenforschung GmbH, Darmstadt, Germany), W. S. Porter (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of British Columbia, Vancouver, British Columbia, Canada), M. P. Reiter (School of Physics, Astronomy, University of Edinburgh, Edinburgh, United Kingdom), J. Ringuette (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Colorado School of Mines, Golden, Colorado, USA), H. Schatz (Facility for Rare Isotope Beams, East Lansing, Michigan, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, Michigan, USA, Joint Institute for Nuclear Astrophysics Center for the Evolution of the Elements), C. Scheidenberger (II. Physikalisches Institut, Justus-Liebig-Universit"at Gie{ss}en, Gie{ss}en, Germany, GSI Helmholtzzentrum f"ur Schwerionenforschung GmbH, Darmstadt, Germany, Helmholtz Forschungsakademie Hessen f"ur FAIR), C. Walls (TRIUMF, Vancouver, British Columbia, Canada), Y. Wang (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of British Columbia, Vancouver, British Columbia, Canada), A. A. Kwiatkowski (TRIUMF, Vancouver, British Columbia, Canada, Department of Physics, Astronomy, University of Victoria, Victoria, British Columbia, Canada)
    • https://arxiv.org/abs/2501.06723
  • 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
  • Investigating the Electron Capture Supernova Candidate AT 2019abn with JWST Spectroscopy
    • Virtual Journal - Volume 22, Issue 31 - article #6
    • Sam Rose (Division of Physics, Mathematics,, Astronomy, California Institute of Technology, Pasadena, CA, USA), Ryan M. Lau (NSF NOIRLab, Tucson, AZ, USA), Jacob E. Jencson (Caltech/IPAC, Pasadena, CA, USA), Mansi M. Kasliwal (Division of Physics, Mathematics,, Astronomy, California Institute of Technology, Pasadena, CA, USA), Kishalay De (MIT-Kavli Institute for Astrophysics, Space Research, Cambridge, MA, USA), Michael E. Ressler (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA), Ori D. Fox (Space Telescope Science Institute, Baltimore, MD, USA), Matthew J. Hankins (Arkansas Tech University, Russellville, AR, USA)
    • https://arxiv.org/abs/2407.20430
  • Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
  • 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
  • Constraints on the dense matter equation of state from young and cold isolated neutron stars
    • Virtual Journal - Volume 22, Issue 15 - article #2
    • Alessio Marino (Institute of Space Sciences ICE, CSIC, Institut d'Estudis Espacials de Catalunya IEEC), Clara Dehman (Institute of Space Sciences ICE, CSIC, Institut d'Estudis Espacials de Catalunya IEEC), Konstantinos Kovlakas (Institute of Space Sciences ICE, CSIC, Institut d'Estudis Espacials de Catalunya IEEC), Nanda Rea (Institute of Space Sciences ICE, CSIC, Institut d'Estudis Espacials de Catalunya IEEC), Jose A. Pons (Universitat d'Alacant), D. Vigan`o (Institute of Space Sciences ICE, CSIC, Institut d'Estudis Espacials de Catalunya IEEC)
    • https://arxiv.org/abs/2404.05371
  • X-ray characterization of the pulsar PSR J1849$-$0001 and its wind nebula G32.64+0.53 associated with TeV sources detected by H.E.S.S., HAWC, Tibet AS$gamma$, and LHAASO. (arXiv:2311.12376v1 [astro-ph.HE])
  • Fast neutron production at the LNL Tandem from the $^7$Li($^{14}$N,xn)X reaction. (arXiv:2311.06143v1 [nucl-ex])
  • Optimal colliding energy for the synthesis of superheavy element $Z$=119. (arXiv:2311.07145v1 [nucl-th])
    • Virtual Journal - Volume 21, Issue 44 - article #16
    • Avazbek Nasirov (1, 2), Bakhodir Kayumov (3, 2) ((1) Joint Institute for Nuclear Research, Dubna 141980, Russia, (2) Institute of Nuclear Physics, Tashkent 100214, Uzbekistan, (3) School of Humanities, Natural Sciences, New Uzbekistan University, Tashkent 100007, Uzbekistan)
    • http://arxiv.org/abs/2311.07145
  • J1046+4047: an extremely low-metallicity dwarf star-forming galaxy with O32 = 57. (arXiv:2311.01799v1 [astro-ph.GA])
    • Virtual Journal - Volume 21, Issue 43 - article #18
    • Y. I. Izotov (1), T. X. Thuan (2, 3), N. G. Guseva (1) ((1) Bogolyubov Institute for Theoretical Physics, National Academy of Sciences of Ukraine, Kyiv, Ukraine, (2) Astronomy Department, University of Virginia, Charlottesville, USA, (3) Institut d'Astrophysique de Paris, Paris, France)
    • http://arxiv.org/abs/2311.01799
  • Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System. (arXiv:2305.16787v1 [astro-ph.SR])
    • Virtual Journal - Volume 21, Issue 22 - article #2
    • Hannah E. Brinkman (1, 2, 3), C. L. Doherty (4), M. Pignatari (1,5,6), O. R. Pols (7), M. Lugaro (1,4,8) ((1) Konkoly Observatory, Research Centre for Astronomy, Earth Sciences (CSFK), Eötvös Loránd Research Network (ELKH), MTA Center of Excellence, Budapest, Hungary (2) Graduate School of Physics, University of Szeged, Hungary (3) Institute of Astronomy, KU Leuven, Leuven, Belgium (4) School of Physics, Astronomy, Monash University, Australia (5) E. A. Milne Centre for Astrophysics, Department of Physics, Mathematics, University of Hull, United Kingdom (6) NuGrid Collaboration, (7) {Department of Astrophysics/IMAPP, Radboud University, Nijmegen, The Netherlands, (8) ELTE Eötvös Loránd University, Institute of Physics, Budapest, Hungary)
    • http://arxiv.org/abs/2305.16787
  • Synthesis of elements in compact stars in pycnonuclear reactions with Carbon isotopes: Quasibound states versus states of zero-points vibrations. (arXiv:2305.09389v1 [nucl-th])
  • 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
  • Accelerating and scaling mentoring strategies to build infrastructure that supports underrepresented groups in STEM. (arXiv:2302.13691v1 [astro-ph.IM])
    • Virtual Journal - Volume 21, Issue 9 - article #1
    • 2030STEM Collaboration (1), Jennifer D. Adams (2), David Asai (3), Ruth Cohen (1), Alonso Delgado (4), Stephanie Danette Preston (5), Jacqueline K. Faherty (1,6), Mandë, Holford (1,6,7), Erich Jarvis (8), Marisela Martinez-Cola (9), Alfred, Mays (10), Louis J. Muglia (10,11,12), Veeshan Narinesingh (13), Caprice Phillips (4), Christine, Pfund (14), Patricia, Silveyra (15) ((1) 2030STEM Inc, New York, New York, USA (2) University of Calgary, Calgary, Alberta, CAN (3) Center for the Advancement of Science Leadership, Culture, Howard Hughes Medical Institute, Chevy Chase, Maryland, USA (4) The Ohio State University, Columbus, Ohio, USA (5) The Pennsylvania State University, State College, Pennsylvania, USA (6) American Museum of Natural History New York, NY, USA (7) Hunter College New York, NY, USA (8) The Rockefeller University, New York, New York, USA (9) Morehouse College, Atlanta, Georgia, USA (10) Burroughs Wellcome Fund, Apex, North Carolina, USA (11) Department of Pediatrics University of Cincinnati College of Medicine, Cincinnati, Ohio, USA (12) Division of Human Genetics, Cincinnati Children's Hospital Medical Center, Cincinnati, Ohio, USA (13) NOAA Geophysical Fluid Dynamics Laboratory, Program in Atmospheric, Oceanic Sciences, Princeton University, Princeton, New Jersey, USA (14) Wisconsin Center for Education Research, University of Wisconsin Madison, Madison, Wisconsin, USA (15) Department of Environmental, Occupational Health, Indiana University Bloomington School of Public Health, Bloomington, Indiana, USA)
    • http://arxiv.org/abs/2302.13691
  • Strongly magnetized accretion in ultracompact binary systems. (arXiv:2302.12318v1 [astro-ph.HE])
  • The Galactic Chemical Evolution of phosphorus observed with IGRINS. (arXiv:2210.04940v1 [astro-ph.SR])
  • Quantum design in study of pycnonuclear reactions in compact stars and new quasibound states. (arXiv:2205.13895v1 [nucl-th])
  • Stellar populations of the globular cluster NGC 5053 investigated using AstroSat-Ultra Violet Imaging Telescope. (arXiv:2205.13839v1 [astro-ph.GA])
  • The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study. (arXiv:2205.03232v1 [astro-ph.HE])
  • Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud. (arXiv:2203.11868v1 [astro-ph.GA])
  • Measurement of Galactic $^{26}$Al with the Compton Spectrometer and Imager. (arXiv:2202.11713v1 [astro-ph.HE])
  • Physical Publicly Verifiable Randomness from Pulsars. (arXiv:2201.05763v1 [astro-ph.HE])
    • Virtual Journal - Volume 20, Issue 3 - article #2
    • J. R. Dawson (1, 2), George Hobbs (1), Yansong Gao (3), Seyit Camtepe (4), Josef Pieprzyk (4, 5), Yi Feng (6, 7), Luke Tranfa (1, 2), Sarah Bradbury (1, 8), Weiwei Zhu (6, 7), Di Li (6, 7, 9). ((1) CSIRO Space, Astronomy, (2) Department of Physics, Astronomy, MQ Research Centre in Astronomy, Astrophysics, Astrophotonics, Macquarie University, Sydney (3) School of Computer Science, Engineering, Nanjing University of Science, Technology, (4) CSIRO Data 61, (5) Institute of Computer Science, Polish Academy of Sciences, (6) National Astronomical Observatories, Chinese Academy of Sciences, Beijing (7) University of Chinese Academy of Sciences, (8) School of Chemistry, Physics, Queensland University of Technology (QUT), (9) NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal)
    • http://arxiv.org/abs/2201.05763
  • Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System. (arXiv:2109.05842v1 [astro-ph.SR])
    • Virtual Journal - Volume 19, Issue 38 - article #1
    • Hannah E. Brinkman (1, 2), J.W. den Hartogh (1), C. L. Doherty (1, 3), M. Pignatari (4, 1, 5, 6), M. Lugaro (1, 7, 3) ((1) Konkoly Observatory, Research Centre for Astronomy, Earth Sciences (CSFK), Eötvös Loránd Research Network (ELKH), Budapest, Hungary (2) Graduate School of Physics, University of Szeged, Hungary (3) School of Physics, Astronomy, Monash University, Australia (4) E. A. Milne Centre for Astrophysics, Department of Physics, Mathematics, University of Hull, United Kingdom (5) NuGrid Collaboration, (6) Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements (7) ELTE Eötvös Loránd University, Institute of Physics, Budapest, Hungary)
    • http://arxiv.org/abs/2109.05842
  • Bayesian Estimation of the D(p,$gamma$)$^3$He Thermonuclear Reaction Rate. (arXiv:2109.00049v1 [astro-ph.CO])
    • Virtual Journal - Volume 19, Issue 36 - article #5
    • Joseph Moscoso (1, 2), Rafael S. de Souza (3), Alain Coc (4), Christian Iliadis (1, 2) ((1) Department of Physics & Astronomy University of North Carolina at Chapel Hill,(2) Triangle Universities Nuclear Laboratory (TUNL), Durham, (3) Key Laboratory for Research in Galaxies, Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, (4) CNRS/IN2P3, IJCLab, Université Paris-Saclay, Bâtiment)
    • http://arxiv.org/abs/2109.00049
  • 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
  • R-process-rich stellar streams in the Milky Way. (arXiv:2102.00066v1 [astro-ph.SR])
    • Virtual Journal - Volume 19, Issue 6 - article #7
    • Maude Gull (1,2), Anna Frebel (2), Karina Hinojosa (2), Ian U. Roederer (3,4), Alexander P. Ji (5), Kaley Brauer ((1) Department of Astronomy, University of California Berkeley, Berkeley, CA USA, (2) Department of Physics & Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA, (3) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA, (4) Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements (JINA-CEE), USA, (5) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA)
    • http://arxiv.org/abs/2102.00066
  • The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae II -- progenitor dependences --. (arXiv:2101.09618v1 [astro-ph.HE])
  • Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars. (arXiv:2010.13620v1 [astro-ph.SR])
    • Virtual Journal - Volume 18, Issue 44 - article #5
    • D. Karinkuzhi (1,2,3), S. Van Eck (2), S. Goriely (2), L. Siess (2), A. Jorissen (2), T. Merle (2), A. Escorza (2,4), T. Masseron (5,6) ((1). Department of Physics, Indian Institute of Science, Bangalore, India.560012, (2). Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium, (3). Department of Physics, Jnana Bharathi Campus, Bangalore University, Bangalore, India. 560056, (4). Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium, (5). Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain, (6). Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain)
    • http://arxiv.org/abs/2010.13620
  • Nucleosynthesis imprints from different Type Ia Supernova explosion scenarios and implications for galactic chemical evolution. (arXiv:2010.14084v1 [astro-ph.SR])
    • Virtual Journal - Volume 18, Issue 44 - article #10
    • F. Lach (1, 2), F. K. Roepke (1, 3), I. R. Seitenzahl (4), B. Coté, (5, 6, 7), S. Gronow (1, 2), A. J. Ruiter (4) ((1) Heidelberger Institut für Theoretische Studien, (2) Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, (3) Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, (4) School of Science, University of New South Wales, Australian Defence Force Academy, (5) Konkoly Observatory, Research Centre for Astronomy, Earth Sciences, MTA Centre for Excellence, (6) ELTE Eötvös Lorénd University, Institute of Physics, (7) National Superconducting Cyclotron Laboratory, Michigan State University)
    • http://arxiv.org/abs/2010.14084
  • Element Abundances in the Unshocked Ejecta of Cassiopeia A. (arXiv:2010.07718v1 [astro-ph.HE])
  • Mergers of binary neutron star systems: a multi-messenger revolution. (arXiv:2009.12255v1 [astro-ph.HE])
  • Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine. (arXiv:2008.10136v1 [astro-ph.SR])
    • Virtual Journal - Volume 18, Issue 35 - article #1
    • A. A. Mura-Guzmán (1,2), D. Yong (1,2), C. Abate (3), A. Karakas (4,2), C. Kobayashi (5,2), H. Oh (6), S. Chun (6), G. Mace (7). ((1) Research School of Astronomy, Astrophysics, Australian National University, Australia, (2) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia, (3) Deep Blue Srl, Rome, Italy, (4) School of Physics, Astronomy, Monash University, Australia, (5) Centre for Astrophysics Research, University of Hertfordshire, UK, (6) Korea Astronomy, Space Science Institute, Republic of Korea, (7) Department of Astronomy, McDonald Observatory, University of Texas at Austin, USA.)
    • http://arxiv.org/abs/2008.10136
  • $^{44}rm Ti$ ejecta in young supernova remnants. (arXiv:2004.12688v1 [astro-ph.HE])
  • Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10. (arXiv:2002.01858v1 [astro-ph.GA])
    • Virtual Journal - Volume 18, Issue 6 - article #3
    • D. Burgarella (1), A. Nanni (1), H. Hirashita (2), P. Theule (1), A. K. Inoue (3,4), T. T. Takeuchi (5) ((1) Aix Marseille Univ, CNRS, CNES, LAM (2) Institute of Astronomy, Astrophysics, Academia Sinica, Astronomy-Mathematics Building, AS/NTU (3) Department of Physics, School of Advanced Science, Engineering, Faculty of Science, Engineering, Waseda University (4) Waseda Research Institute for Science, Engineering, Faculty of Science, Engineering, Waseda University (5) Division of Particle, Astrophysical Science, Nagoya University)
    • http://arxiv.org/abs/2002.01858
  • SNe Ia from double detonations: Impact of core-shell mixing on the carbon ignition mechanism. (arXiv:2002.00981v1 [astro-ph.SR])
  • Elemental Abundances in M31: The Kinematics and Chemical Evolution of Dwarf Spheroidal Satellite Galaxies. (arXiv:1912.02186v1 [astro-ph.GA])
  • Identification of strontium in the merger of two neutron stars. (arXiv:1910.10510v1 [astro-ph.HE])
    • Virtual Journal - Volume 17, Issue 43 - article #4
    • Darach Watson (1, 2), Camilla J. Hansen (3), Jonatan Selsing (1, 2), Andreas Koch (4), Daniele B. Malesani (1, 2, 5), Anja C. Andersen (1), Johan P. U. Fynbo (1, 2), Almudena Arcones (6, 7), Andreas Bauswein (7, 8), Stefano Covino (9), Aniello Grado (10), Kasper E. Heintz (1, 2, 11), Leslie Hunt (12), Chryssa Kouveliotou (13, 14), Giorgos Leloudas (1, 5), Andrew Levan (15, 16), Paolo Mazzali (17, 18), Elena Pian (19) ((1) Niels Bohr Institute, University of Copenhagen, (2) Cosmic Dawn Center (DAWN), (3) Max-Planck-Institut für Astronomie, Heidelberg, (4) Zentrum für Astronomie der Universität Heidelberg, (5) DTU Space, Technical University of Denmark, (6) Institut für Kernphysik, Technische Universität Darmstadt, (7) GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, (8) Heidelberger Institut für Theoretische Studien, Heidelberg, (9) INAF / Brera Astronomical Observatory, Merate, (10) INAF-OACN, Naples, (11) Centre for Astrophysics, Cosmology, University of Iceland, (12) INAF - Osservatorio Astrofisico di Arcetri, Firenze, (13) Physics Department, the George Washington University, (14) Astronomy, Physics, Statistics Institute of Sciences (APSIS), Washington, DC, (15) Department of Astrophysics/IMAPP, Radboud University Nijmegen, (16) Department of Physics, University of Warwick, (17) Astrophysics Research Institute, Liverpool John Moores University, (18) Max-Planck Institute for Astrophysics, Garching, (19) INAF, Astrophysics, Space Science Observatory, Bologna)
    • http://arxiv.org/abs/1910.10510
  • 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
  • A Constant LGRB Metallicity Distribution Across Redshifts z < 2.5. (arXiv:1904.02673v1 [astro-ph.HE])
    • Virtual Journal - Volume 17, Issue 14 - article #1
    • J. F. Graham (1), P. Schady (2,3), A. S. Fruchter (4) ((1) Kavli Institute for Astronomy, Astrophysics at Peking University, (2) Department of Physics, University of Bath, (3) Max-Planck Institut fur Extraterrestrische Physik, (4) Space Telescope Science Institute)
    • http://arxiv.org/abs/1904.02673
  • Single X-ray Bursts and the Model of a Spreading Layer of Accreting Matter over the Neutron Star Surface. (arXiv:1811.12865v1 [astro-ph.HE])
  • On the Progenitors of Type Ia Supernovae. (arXiv:1802.03125v1 [astro-ph.SR])
    • Virtual Journal - Volume 16, Issue 7 - article #12
    • Mario Livio (University of Nevada, Las Vegas, Visiting Scholar, The Weizmann Institute of Science), Paolo Mazzali (Visiting Scholar, The Weizmann Institute of Science, Liverpool John Moores University)
    • http://arxiv.org/abs/1802.03125
  • Chemical analysis of three barium stars: HD 51959, HD 88035, HD 121447. (arXiv:1802.01343v1 [astro-ph.SR])
  • The Soreq Applied Research Accelerator Facility (SARAF) - Overview, Research Programs and Future Plans. (arXiv:1801.06493v1 [physics.ins-det])
  • Ca II 8542 AA brightenings induced by a solar microflare. (arXiv:1709.06861v1 [astro-ph.SR])
  • New determination of proton spectroscopic factors and reduced widths for $^{8}$Be states in the $16.5-18.0$ MeV excitation energy region via the study of the $^{7}$Li($^{3}$He,d)$^{8}$Be transfer reaction at E$_{lab}$ $= 20$ MeV. (arXiv:1709.05482v1 [nucl-ex])
  • Multiple X-ray bursts and the model of a spreading layer of accreting matter over the neutron star surface. (arXiv:1708.07016v1 [astro-ph.HE])
  • Star Formation Conditions in a Planck Galactic Cold Clump, G108.84–00.81
  • Measurement of fast neutron background at the China Jinping Underground Laboratory. (arXiv:1706.06831v1 [physics.ins-det])
  • An XMM-Newton and INTEGRAL view on the hard state of EXO 1745-248 during its 2015 outburst. (arXiv:1703.07389v1 [astro-ph.HE])
    • Virtual Journal - Volume 15, Issue 12 - article #2
    • M. Matranga (1), A. Papitto (2), T. Di Salvo (1), E. Bozzo (3), D. F. Torres (4), R. Iaria (1), L. Burderi (5), N. Rea (4,8), D. de Martino (6), C. Sanchez-Fernandez (7), A. F. Gambino (1), C. Ferrigno (3), L. Stella (2) ((1) Università degli Studi di Palermo, Palermo, Italy, (2) INAF, Osservatorio Astronomico di Roma, Monte Porzio Catone (Roma), Italy, (3) ISDC Data Centre for Astrophysics, Versoix, Switzerland, (4) Institut de Ciencies de l'Espai (IEEC-CSIC), Campus UAB, Barcelona, Spain, (5) Università degli Studi di Cagliari, Dipartimento di Fisica, Monserrato, Italy, (6) Osservatorio Astronomico di Capodimonte, Napoli, Italy, (7) ESA/ESAC, Science Operations Department Villanueva de la Canada Madrid, Spain, (8) Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, the Netherlands)
    • http://arxiv.org/abs/1703.07389
  • Color Me Intrigued: the Discovery of iPTF 16fnm, a Supernova 2002cx-like Object. (arXiv:1703.07449v1 [astro-ph.HE])
  • Thermonuclear burst observations for model comparisons: a reference sample. (arXiv:1703.07485v1 [astro-ph.HE])
  • Rise and fall of the dust shell of the classical nova V339 Delphini. (arXiv:1612.06241v1 [astro-ph.SR])
  • $^{22}$Ne and $^{23}$Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for $^{22}$Ne(p,$gamma$)$^{23}$Na. (arXiv:1611.07742v1 [astro-ph.SR])
  • Ultraluminous X-ray bursts in two ultracompact companions to nearby elliptical galaxies. (arXiv:1610.05781v1 [astro-ph.HE])
  • Maximizing Science in the Era of LSST: A Community-Based Study of Needed US Capabilities. (arXiv:1610.01661v1 [astro-ph.IM])
  • Intermittent dipping in a low-mass X-ray Binary. (arXiv:1607.00074v1 [astro-ph.HE])
  • The type Iax supernova, SN 2015H: a white dwarf deflagration candidate
  • Harassment victims deserve better
  • LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation
  • 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]
  • Interdisciplinarity: How to catalyse collaboration
  • Neutrino emissivity in the quark-hadron mixed phase of neutron stars
    • Virtual Journal - Volume 13, Issue 26 - article #23
    • William M. Spinella (1,2), Fridolin Weber (2,3), Gustavo A. Contrera (4,5,6), Milva G. Orsaria (4,6) ((1) Computational Science Research Center San Diego State University, San Diego, CA, USA, (2) Department of Physics, San Diego State University, San Diego, CA, USA, (3) Center for Astrophysics and Space Sciences, University of California San Diego, La Jolla, CA, USA, (4) CONICET, Rivadavia 1917, Buenos Aires, Argentina, (5) IFLP, CONICET - Dpto. de Fisica, UNLP, La Plata, Argentina, (6) Grupo de Gravitacion, Astrofisica y Cosmologia, Facultad de Ciencias Astronomicas y Geofisicas, Universidad Nacional de La Plata, Paseo del Bosqu, La Plata, Argentina.)
    • arXiv.org - Nuclear Theory - Volume: 2015, Issue: 24 Jul
    • arXiv:1507.06067 [pdf, ps, other]
  • Physics: The impulse of beauty
  • Data Reduction with the MIKE Spectrometer
  • A search for lithium in metal-poor L dwarfs
    • Virtual Journal - Volume 13, Issue 21 - article #2
    • N. Lodieu (1,2), A. J. Burgasser (3,4), Y. Pavlenko (5,6), R. Rebolo (1,2,7) ((1) IAC, Tenerife, Spain, (2) Universidad de La Laguna, Tenerife, Spain, (3) University of California San Diego, USA, (4) Visiting professor at the IAC in Tenerife, (5) Main Astronomical Observatory of the National Academy of Sciences of Ukraine, (6) University of Hertfordshire, UK, (7) CSIC, Spain)
    • arXiv.org - Astrophysics - Volume: 2015, Issue: 29 May
    • arXiv:1505.06858 [pdf, ps, other]
  • Statistics: P values are just the tip of the iceberg
  • Surface abundances of ON stars
  • In the beginning
  • History of science: Unshadowed lens on the past
  • The Open Cluster Chemical Abundances from Spanish Observatories survey (OCCASO)
    • Virtual Journal - Volume 12, Issue 25 - article #11
    • R. Carrera (1,2), L. Casamiquela (3), L. Balaguer-Núñez (3), C. Jordi (3), E. Pancino (4,5), C. Allende-Prieto (1,2), S. Blanco-Cuaresma (6,7), C. E. Mártinez-Vázquez (1,2), S. Murabito (1,2), A. del Pino (1,2), A. Aparicio (1,2), C. Gallart (1,2), A. Recio-Blanco (8) ((1) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain, (3) Dept. d'Astronomia i Meteorologia, Institut de Ciéncies del Cosmos, Universitat de Barcelona (IEEC-UB), Barcelona, Spain, (4) Osservatorio Astronomico di Bologna, Bologna, Italy, (5) ASI Science Data Center, Frascati, Italy, (6) CNRS/Univ. Bordeaux, LAB, UMR 5804, Floirac, France, (7) Observatoire de Genéve, Université de Genéve, Sauverny, Switzerland, (8) Laboratoire Lagrange (UMR7293), Université de Nice Sophia Antipolis, CNRS, Observatoire de la Cote d'Azur, Nice, France)
    • arXiv.org - Astrophysics - Volume: 2014, Issue: 12 Dec
    • arXiv:1412.3509 [pdf, other]
  • ASTRO-H White Paper - Low-mass X-ray Binaries
  • ASTRO-H White Paper - White Dwarf
  • Scientific method: Defend the integrity of physics
  • An Ultraluminous X-ray Source Powered by An Accreting Neutron Star
    • Virtual Journal - Volume 12, Issue 23 - article #17
    • M. Bachetti (1,2), F. A. Harrison (3), D. J. Walton (3), B. W. Grefenstette (3), D. Chakrabarty (4), F. Fürst (3), D. Barret (1,2), A. Beloborodov (5), S. E. Boggs (6), F. E. Christensen (7), W. W. Craig (8), A. C. Fabian (9), C. J. Hailey (10), A. Hornschemeier (11), V. Kaspi (12), S.R. Kulkarni (3), T. Maccarone (13), J. M. Miller (14), V. Rana (3), D. Stern (15), S. P. Tendulkar (3), J. Tomsick (6), N. A. Webb (1,2), W. W. Zhang (11) ((1) Université de Toulouse, UPS-OMP, IRAP, F-31400 Toulouse, France (2) CNRS, Institut de Recherche en Astrophysique et Planétologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France Toulouse, France. (3) Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA. (4) MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA (5) Physics Department, Columbia University. 538 W 120th Street, New York, NY 10027, USA 6Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA (7) DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Lyngby, Denmark (8) Lawrence Livermore National Laboratory, Livermore, CA 94550, USA (9) Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK (10) Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA (11) NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA (12) Department of Physics, McGill University, Montreal, Quebec, H3A 2T8, Canada (13) Department of Physics, Texas Tech University, Lubbock, TX 79409, USA (14) Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA (15) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA)
    • arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Oct
    • arXiv:1410.3590 [pdf]
  • A WISE view of novae. I. The data
  • Low-energy dipole strength in 112,120Sn
    • Virtual Journal - Volume 12, Issue 20 - article #182
    • B. Özel-Tashenov (1,2), J. Enders (1), H. Lenske (3), A.M. Krumbholz (1), E. Litvinova (4,5), P. von Neumann-Cosel (1), I. Poltoratska (1), A. Richter (1), G. Rusev (6), D. Savran (7,8), N. Tsoneva (3,9) ((1) Institut für Kernphysik, Technische Universität Darmstadt, (2) Faculty of Science and Letters, Nigde University, (3) Institut für Theoretische Physik, Justus-Liebig Universität, (4) Department of Physics, Western Michigan University, (5) NSCL, Michigan State University, (6) Chemistry Division, Los Alamos National LaboratoryA, (7) ExtreMe Matter Institute and Research Devision, (8) Frankfurt Institute for Advanced Studies FIAS, (9) Institute of Nuclear Research and Nuclear Energy)
    • arXiv.org - Nuclear Experiment - Volume: 2014, Issue: 6 Jun
    • arXiv:1406.1409 [pdf, other]
  • X-ray diagnostics of chemical composition of the accretion disk and donor star in UCXBs II: XMM-Newton observations
  • 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]
  • A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
    • Virtual Journal - Volume 12, Issue 8 - article #1
    • B. Mueller (1,2), H.-Th. Janka (2), ((1) Monash Centre for Astrophysics, School of Mathematical Sciences, Monash University, (2) Max-Planck-Institut fuer Astrophysik)
    • arXiv.org - Astrophysics - Volume: 2014, Issue: 21 Feb
    • arXiv:1402.3415 [pdf, ps, other]
  • Number crunch
  • The Detailed Photometric and Spectroscopic Study of the 2011 Outburst of the Recurrent Nova T Pyxidis from 0.8 to 250 Days after Discovery
  • Popular science: Get the word out
  • The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B
    • Virtual Journal - Volume 11, Issue 35 - article #13
    • T. Rauch (1), R. Bohlin (2), J. W. Kruk (3), K. Werner (1) ((1) Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Tuebingen, Germany, (2) Space Telescope Science Institute, Baltimore, MD, USA, (3) NASA Goddard Space Flight Center, Greenbelt, MD, USA)
    • arXiv.org - Astrophysics - Volume: 2013, Issue: 30 Aug
    • arXiv:1308.6450 [pdf, ps, other]
  • Collaborations: The fourth age of research
  • Science in schools
  • Practices in source code sharing in astrophysics
  • Tabulated equation of state for supernova matter including full nuclear ensemble
    • Virtual Journal - Volume 11, Issue 17 - article #18
    • N. Buyukcizmeci (1,2), A.S. Botvina (1,3,4), I.N. Mishustin (1,5) ((1) Frankfurt Institute for Advanced Studies (2) Department of Physics, Selcuk University (3) Institute for Nuclear Research, Russian Academy of Sciences (4) Institut für Kernphysik, J. Gutenberg Universitä (5) Kurchatov Institute, Russian Research Center)
    • arXiv.org - Nuclear Theory - Volume: 2013, Issue: 26 Apr
    • arXiv:1304.6741 [pdf, ps, 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]
  • A WISE view of novae
  • HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
  • The double pulsar: evidence for neutron star formation without an iron core-collapse supernova
    • Virtual Journal - Volume 11, Issue 7 - article #16
    • R. D. Ferdman (1 and 2), I. H. Stairs (3), M. Kramer (4 and 1), R. P. Breton (5), M. A. McLaughlin (6 and 7), P. C. C. Freire (4), A. Possenti (8), B. W. Stappers (1), V. M. Kaspi (2), R. N. Manchester (9), A. G. Lyne (1) ((1) University of Manchester, Jodrell Bank Centre for Astrophysics, United Kingdom, (2) McGill University, Montreal, Canada, (3) University of British Columbia, Vancouver, Canada, (4) Max Planck Institute for Radio Astronomy, Bonn, Germany, (5) University of Southampton, Southampton, United Kingdom, (6) West Virginia University, Morgantown, USA, (7) National Radio Astronomy Observatory, Green Bank, USA, (8) INAF - Osservatorio Astronomico di Cagliari, Capoterra, Italy, (9) CSIRO Astronomy and Space Science, Australia Telescope National Facility, Epping, Australia)
    • arXiv.org - Astrophysics - Volume: 2013, Issue: 15 Feb
    • arXiv:1302.2914 [pdf, ps, other]
  • Communication: Two minutes to impress
  • Novae in gamma-rays
    • Virtual Journal - Volume 11, Issue 2 - article #12
    • M. Hernanz (Institute of Space Sciences, CSIC-IEEC, Barcelona, Spain)
    • arXiv.org - Astrophysics - Volume: 2013, Issue: 11 Jan
    • arXiv:1301.1660 [pdf, ps, other]
  • Bayesian analysis of ages, masses, and distances to cool stars with non-LTE spectroscopic parameters
  • A vote for science
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