Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Martina Maestripieri"'
Autor:
Vishnu Reddy, Michael S. Kelley, Lance Benner, Jessie Dotson, Nicolas Erasmus, Davide Farnocchia, Tyler Linder, Joseph R. Masiero, Cristina Thomas, James Bauer, Miguel R. Alarcon, Paolo Bacci, Daniel Bamberger, Adam Battle, Zouhair Benkhaldoun, Guido Betti, Mirel Birlan, Marina Brozovic, Brian Burt, David C. Cantillo, Sunil Chandra, Gregoire Chomette, Ashley Coates, Francesca DeMeo, Maxime Devogèle, Petr Fatka, Marin Ferrais, Paolo Fini, Carel van Gend, Jon D. Giorgini, Dmitry Glamazda, Robert Holmes, Joseph L. Hora, Shinji Horiuchi, Kamil Hornoch, Marco Iozzi, Cristóvão Jacques, Emmanuel Jehin, Hai Jiang, Galina Kaiser, Peter Kušnirák, Eduard Kuznetsov, Julia de León, Alexios Liakos, Javier Licandro, Tim Lister, Jing Liu, Andy Lopez-Oquendo, Martina Maestripieri, Donovan Mathias, Marco Micheli, Shantanu P. Naidu, Alessandro Nastasi, Alin Nedelcu, Elisabeta Petrescu, Marcel Popescu, Stephen B. Potter, Petr Pravec, Juan Sanchez, Toni Santana-Ros, Miquel Serra-Ricart, Nick Sioulas, Adrian Sonka, Alessio Squilloni, Maura Tombelli, Madalina Trelia, David E. Trilling, Elizabeth Warner, Guy Wells, Lorien Wheeler, Mike Wiles
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 6, p 141 (2024)
We present the results of a fourth planetary defense exercise, focused this time on the small near-Earth asteroid (NEA) 2023 DZ2 and conducted during its close approach to the Earth in 2023 March. The International Asteroid Warning Network (IAWN), wi
Externí odkaz:
https://doaj.org/article/5803dc0c1d9f4ae3b0af7b6a2cfe0c0b
Autor:
Davide Farnocchia, Vishnu Reddy, James M. Bauer, Elizabeth M. Warner, Marco Micheli, Matthew J. Payne, Tony Farnham, Michael S. Kelley, Miguel R. Alarcon, Paolo Bacci, Roberto Bacci, Mauro Bachini, Kevin Baillié, Giorgio Baj, Daniel Bamberger, Anatoly P. Barkov, Stefan Beck, Guido Betti, Enrico Biancalani, Bryce T. Bolin, David Briggs, Luca Buzzi, Haowen Cheng, Eric Christensen, Alessandro Coffano, Luca Conversi, Christophe Demeautis, Larry Denneau, Josselin Desmars, Anlaug A. Djupvik, Leonid Elenin, Paolo Fini, Tobias Felber, Randy Flynn, Gianni Galli, Mikael Granvik, Bill Gray, Zuri Gray, Luca Grazzini, Werner Hasubick, Tobias Hoffmann, Robert Holmes, Marco Iozzi, Alexander L. Ivanov, Viktor A. Ivanov, Natalya V. Ivanova, Cristóvão Jacques, Hai Jiang, Zheng Jinghui, Anni Kasikov, Myung-Jin Kim, Balaji Kumar, Hee-Jae Lee, Bin Li, Jing Liu, Javier Licandro, Tyler Linder, Vadim E. Lysenkov, Martina Maestripieri, Andrea Mantero, Vladimiro Marinello, Jennie McCormick, Darrel Moon, Alessandro Nastasi, James D. Neill, Guenther Neue, Artem O. Novichonok, Francisco Ocaña, Gianpaolo Pizzetti, Anton Pomazan, Josiah N. Purdum, Christophe Ratinaud, Dong-Goo Roh, Filipp D. Romanov, Nello Ruocco, Toni Santana-Ros, Toni Scarmato, Anastasia Schmalz, Sergei Schmalz, Miquel Serra-Ricart, Clay Sherrod, Nick Sioulas, Andrea Soffiantini, Giacomo Succi, David J. Tholen, Jeppe S. Thomsen, William Thuillot, Richard Wainscoat, Guy Wells, Robert Weryk, Nikolai A. Yakovenko, Hong-Suh Yim, Chengxing Zhai
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 11, p 203 (2023)
The Earth close approach of near-Earth asteroid 2005 LW3 on 2022 November 23 represented a good opportunity for a second observing campaign to test the timing accuracy of astrometric observation. With 82 participating stations, the International Aste
Externí odkaz:
https://doaj.org/article/7cd61aae7b97417dbbf71cc872c9a4b7
Autor:
G. Scarfi, T. Pribulla, J. C. Guirado, L. Buzzi, Grzegorz Dudziński, A. Farkas-Takács, L. Mazzei, E. Meza, A. Aletti, J. M. Christille, C. Perelló, L. Morrone, V. Peris, Valerio Nascimbeni, J. Lecacheux, J. M. Madiedo, Rene Duffard, F. Mancini, Bruno Sicardy, J. Alikakos, Vassilis Charmandaris, Cs. Kiss, M. Conjat, Raoul Behrend, R. Komžík, Frédéric Vachier, Martina Maestripieri, J. Skvarc, Paolo Bacci, T. G. Mueller, Domenico Nardiello, R. Iglesias-Marzoa, F. Colas, Aleksandar Cikota, András Pál, N. Paschalis, R. Szakats, A. Campo Bagatin, P. J. Gutierrez, Giacomo Succi, Pablo Santos-Sanz, A. R. Gomes-Júnior, Gábor Marton, M. Butkiewicz-Bak, E. Varga-Verebélyi, M. Masucci, Estela Fernández-Valenzuela, V. Tsamis, Victor Ali-Lagoa, Felipe Braga-Ribas, M. Alighieri, Roberto Vieira-Martins, F. Manzano, Julio Camargo, E. Dal Canto, S. Hellmich, F. Roques, A. Vecchione, A. Navarro, Stefano Mottola, A. Noschese, Albino Carbognani, F. Lavalade, Josselin Desmars, Mónica Vara-Lubiano, Nora Morales, C. Schnabel, Mauro Bachini, Kosmas Gazeas, J. M. Mari, Przemyslaw Bartczak, W. Beisker, S. Sposetti, F. Ciabattari, A. Alvarez-Candal, Stefan Cikota, J. L. Ortiz, Marcelo Assafin, A. Marciniak, G. Benedetti-Rossi, H. Mikuz
Publikováno v:
Astronomy & Astrophysics
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Maz
Autor:
Valerio Nascimbeni, J. Lecacheux, Toni Santana-Ros, Agustín Sánchez-Lavega, Pablo Santos-Sanz, L. Nerli, D. T. Koseoglu, Frédéric Vachier, V. Peris, Przemyslaw Bartczak, R. Komžík, Eda Sonbas, Cs. Kiss, Gábor Marton, C. Ries, Yavuz Güney, Marcelo Assafin, Martina Maestripieri, Josselin Desmars, T. G. Mueller, Osman Demircan, O. Erece, V. Granata, A. R. Gomes-Júnior, Francesco Marzari, Ulrich Hopp, Cahit Yeşilyaprak, N. Paschalis, A. Campo Bagatin, B. Gaehrken, Paolo Bacci, V. Tsamis, O. Satir, F. Martinelli, F. L. Rommel, Santiago Pérez-Hoyos, F. Ciabattari, R. Iglesias-Marzoa, Stefano Mottola, Ricardo Hueso, Julio Camargo, Herman Mikuz, Françoise Roques, Mohammad Shameoni Niaei, Mauro Bachini, Vassilis Charmandaris, Jose Luis Ortiz, A. Takácsné Farkas, András Pál, A. Carbognani, L. Tzouganatos, Giuseppe Leto, Aleksandar Cikota, G. Benedetti-Rossi, Roberto Vieira-Martins, Nicolás Morales, José M. Madiedo, Bruno Sicardy, Róbert Szakáts, B. E. Morgado, Theodor Pribulla, Estela Fernández-Valenzuela, M. Butkiewicz-Bąk, Afşar Kabaş, Alvaro Alvarez-Candal, Giacomo Succi, Jérôme Berthier, J. Alikakos, Ç. Püsküllü, Kamil Hornoch, W. Beisker, E. Meza, Stefan Cikota, T. Ozisik, E. Varga-Verebélyi, J. M. Christille, J. C. Guirado, Grzegorz Dudziński, L. Mazzei, J. M. Ohlert, Rene Duffard, Raoul Behrend, S. Kalkan, A. Marciniak, N. Karaman, S. Hellmich, Kosmas Gazeas, Victor Ali-Lagoa, Ozan Ünsalan, Felipe Braga-Ribas, François Colas, Petr Pravec, Diane Berard
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Nature
Nature, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature, Nature Publishing Group, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩
Universidad de Alicante (UA)
Nature
Nature, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature, Nature Publishing Group, 2017, 550 (7675), pp.219-223. ⟨10.1038/nature24051⟩
Ortiz, José Luis et. al.
Haumea-one of the four known trans-Neptunian dwarf planets- is a very elongated and rapidly rotating body1-3. In contrast to other dwarf planets4-6, its size, shape, albedo and density are not well constrained. The Cent
Haumea-one of the four known trans-Neptunian dwarf planets- is a very elongated and rapidly rotating body1-3. In contrast to other dwarf planets4-6, its size, shape, albedo and density are not well constrained. The Cent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa292d0be284f3008c5a229e471447f1
http://hdl.handle.net/10045/70230
http://hdl.handle.net/10045/70230