Zobrazeno 1 - 10
of 25
pro vyhledávání: '"M. Fauvaud"'
Autor:
D. Athanasopoulos, J. Hanuš, C. Avdellidou, R. Bonamico, M. Delbo, M. Conjat, A. Ferrero, K. Gazeas, J. P. Rivet, N. Sioulas, G. van Belle, P. Antonini, M. Audejean, R. Behrend, L. Bernasconi, J. W. Brinsfield, S. Brouillard, L. Brunetto, M. Fauvaud, S. Fauvaud, R. Gonzalez, D. Higgins, T. W.-S. Holoien, G. Kober, R. A. Koff, A. Kryszczynska, F. Livet, A. Marciniak, J. Oey, O. Pejcha, J. J. Rives, R. Roy
Publikováno v:
Astronomy & Astrophysics. 666:A116
Families of asteroids generated by the collisional fragmentation of a common parent body have been identified using clustering methods of asteroids in their proper orbital element space. An alternative method has been developed in order to identify c
Autor:
J. Strajnic, M. Pawłowski, Rene Duffard, Victor Ali-Lagoa, J.-G. Bosch, P. Pinel, Tamás Müller, Raoul Behrend, K. Wagrez, Dagmara Oszkiewicz, A. Pal, Brian A. Skiff, J. Krajewski, L. Brunetto, R. Szakats, T. Santana-Ros, F. Del Freo, E. Verebelyi, Paweł Kankiewicz, F. Richard, M. Evangelista-Santana, J. Michimani-Garcia, S. Fauvaud, T. Kundera, László Molnár, M. Butkiewicz Bąk, K. Sobkowiak, D. Lazzaro, Tom Polakis, J. Skrzypek, G. Farroni, S. Geier, Seitaro Urakawa, J. Golonka, R. Hirsch, P. Arcoverde, H. Medeiros, Eda Sonbas, Michał Żejmo, Doeon Kim, Frederick Pilcher, J. J. Sanabria, L. Bernasconi, Myung-Jin Kim, I. Konstanciak, Krzysztof Kamiński, M. Fauvaud, E. Pakštienė, V. Perig, E. Rondon, G. Stachowski, T. Rodrigues, Łukasz Tychoniec, Josef Ďurech, Cs. Kalup, V. Kecskeméthy, Zouhair Benkhaldoun, J. Grice, E. Podlewska-Gaca, F. Manzini, J. Horbowicz, Marin Ferrais, M. K. Kamińska, Jakub Nadolny, P. Julien, S. Brincat, Waldemar Ogloza, K. Żukowski, V. Kudak, A. Marciniak, Emmanuel Jehin, F. Monteiro, P. Kulczak, P. Trela, Nicolás Morales, Rupak Roy
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 654, ⟨10.1051/0004-6361/202140991⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, 2021, 654, ⟨10.1051/0004-6361/202140991⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Full list of authors: Marciniak, A.; Ďurech, J.; Alí-Lagoa, V.; Ogłoza, W.; Szakáts, R.; Müller, T. G.; Molnár, L.; Pál, A.; Monteiro, F.; Arcoverde, P.; Behrend, R.; Benkhaldoun, Z.; Bernasconi, L.; Bosch, J.; Brincat, S.; Brunetto, L.; Butki
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d4809ad4a72255fae155c9a3e8cf4e5
https://hal-insu.archives-ouvertes.fr/insu-03667381/file/aa40991-21.pdf
https://hal-insu.archives-ouvertes.fr/insu-03667381/file/aa40991-21.pdf
Akademický článek
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Autor:
F. Richard, Jakub Nadolny, E. Kosturkiewicz, K. Sobkowiak, A. Marciniak, Shin-ichiro Okumura, I. Konstanciak, Dagmara Oszkiewicz, Seitaro Urakawa, Magdalena Polińska, Krzysztof Kamiński, Łukasz Tychoniec, S. Fauvaud, Frederick Pilcher, Kota Nishiyama, M. Murawiecka, P. Trela, T. Sakamoto, Paweł Kankiewicz, M. Fauvaud, R. Hirsch, G. Stachowski, J. Horbowicz, Toni Santana-Ros
Publikováno v:
Planetary and Space Science. 118:256-266
Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse naturally have more data available, so their synodic periods are confirmed from multiple sources. Also, thanks to availability of
Autor:
L. Bernasconi, Michael Fauerbach, Frederick Pilcher, S. A. Marks, Mikko Kaasalainen, M. Fauvaud, Raoul Behrend, S. Fauvaud, Brian D. Warner, J. Durech, J.-M. Vugnon
Publikováno v:
Astronomy & Astrophysics. 493:291-297
Aims. Shape and spin state are basic physical characteristics of a n asteroid. They can be derived from disc-integrated photometry by the lightcurve inversion method. Increasing the number of asteroids with known basic physical properties is necessar
Autor:
F. Richard, P. Scheirich, François Colas, E. Morelle, Lawrence A. Molnar, Emmanuel Jehin, M. Bonnardeau, A. Marciniak, M. Birlan, Richard P. Binzel, S. Fauvaud, Stefano Mottola, P. Farissier, M. Fauvaud, A. Leroy, Francesca E. DeMeo, R. Hirsch, C. Gillier, Jean Manfroid, F. Vachier, Marco Delbo, A. Carbognani, Michaël Gillon, Raoul Behrend, Benoit Carry, S. Hellmich, J. Strajnic, K. Sobkowiak, E. Barbotin, A. Matter, Petr Pravec, J. Montier
Publikováno v:
Icarus
Icarus, Elsevier, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
Icarus, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
arXiv
Icarus, Elsevier, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
Icarus, 2014, 248, pp.516-525. ⟨10.1016/j.icarus.2014.11.002⟩
arXiv
In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here at characterizing the surface composition, mutual orbit, size, mass, and density of the small main-belt binary as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e86b05ed4ee305763b854bd76bbf2835
https://hal.sorbonne-universite.fr/hal-01122881
https://hal.sorbonne-universite.fr/hal-01122881
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
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Autor:
J. Hanuš, J. Ďurech, M. Brož, A. Marciniak, B. D. Warner, F. Pilcher, R. Stephens, R. Behrend, B. Carry, D. Čapek, P. Antonini, M. Audejean, K. Augustesen, E. Barbotin, P. Baudouin, A. Bayol, L. Bernasconi, W. Borczyk, J.-G. Bosch, E. Brochard, L. Brunetto, S. Casulli, A. Cazenave, S. Charbonnel, B. Christophe, F. Colas, J. Coloma, M. Conjat, W. Cooney, H. Correira, V. Cotrez, A. Coupier, R. Crippa, M. Cristofanelli, Ch. Dalmas, C. Danavaro, C. Demeautis, T. Droege, R. Durkee, N. Esseiva, M. Esteban, M. Fagas, G. Farroni, M. Fauvaud, S. Fauvaud, F. Del Freo, L. Garcia, S. Geier, C. Godon, K. Grangeon, H. Hamanowa, N. Heck, S. Hellmich, D. Higgins, R. Hirsch, M. Husarik, T. Itkonen, O. Jade, K. Kamiński, P. Kankiewicz, A. Klotz, R. A. Koff, A. Kryszczyńska, T. Kwiatkowski, A. Laffont, A. Leroy, J. Lecacheux, Y. Leonie, C. Leyrat, F. Manzini, A. Martin, G. Masi, D. Matter, J. Michałowski, M. J. Michałowski, T. Michałowski, J. Michelet, R. Michelsen, E. Morelle, S. Mottola, R. Naves, J. Nomen, J. Oey, W. Ogłoza, A. Oksanen, D. Oszkiewicz, P. Pääkkönen, M. Paiella, H. Pallares, J. Paulo, M. Pavic, B. Payet, M. Polińska, D. Polishook, R. Poncy, Y. Revaz, C. Rinner, M. Rocca, A. Roche, D. Romeuf, R. Roy, H. Saguin, P. A. Salom, S. Sanchez, G. Santacana, T. Santana-Ros, J.-P. Sareyan, K. Sobkowiak, S. Sposetti, D. Starkey, R. Stoss, J. Strajnic, J.-P. Teng, B. Trégon, A. Vagnozzi, F. P. Velichko, N. Waelchli, K. Wagrez, H. Wücher
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 551 (A67), 16 p. ⟨10.1051/0004-6361/201220701⟩
The larger number of models of asteroid shapes and their rotational states derived by the lightcurve inversion give us better insight into both the nature of individual objects and the whole asteroid population. With a larger statistical sample we ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4f9941a036a9dd815e01cce509f1298
https://hal.science/hal-00794404
https://hal.science/hal-00794404
Autor:
J. Hanuš, J. Ďurech, D. A. Oszkiewicz, R. Behrend, B. Carry, M. Delbo, O. Adam, V. Afonina, R. Anquetin, P. Antonini, L. Arnold, M. Audejean, P. Aurard, M. Bachschmidt, B. Baduel, E. Barbotin, P. Barroy, P. Baudouin, L. Berard, N. Berger, L. Bernasconi, J-G. Bosch, S. Bouley, I. Bozhinova, J. Brinsfield, L. Brunetto, G. Canaud, J. Caron, F. Carrier, G. Casalnuovo, S. Casulli, M. Cerda, L. Chalamet, S. Charbonnel, B. Chinaglia, A. Cikota, F. Colas, J.-F. Coliac, A. Collet, J. Coloma, M. Conjat, E. Conseil, R. Costa, R. Crippa, M. Cristofanelli, Y. Damerdji, A. Debackère, A. Decock, Q. Déhais, T. Déléage, S. Delmelle, C. Demeautis, M. Dróżdż, G. Dubos, T. Dulcamara, M. Dumont, R. Durkee, R. Dymock, A. Escalante del Valle, N. Esseiva, R. Esseiva, M. Esteban, T. Fauchez, M. Fauerbach, M. Fauvaud, S. Fauvaud, E. Forné, C. Fournel, D. Fradet, J. Garlitz, O. Gerteis, C. Gillier, M. Gillon, R. Giraud, J.-P. Godard, R. Goncalves, Hiroko Hamanowa, Hiromi Hamanowa, K. Hay, S. Hellmich, S. Heterier, D. Higgins, R. Hirsch, G. Hodosan, M. Hren, A. Hygate, N. Innocent, H. Jacquinot, S. Jawahar, E. Jehin, L. Jerosimic, A. Klotz, W. Koff, P. Korlevic, E. Kosturkiewicz, P. Krafft, Y. Krugly, F. Kugel, O. Labrevoir, J. Lecacheux, M. Lehký, A. Leroy, B. Lesquerbault, M. J. Lopez-Gonzales, M. Lutz, B. Mallecot, J. Manfroid, F. Manzini, A. Marciniak, A. Martin, B. Modave, R. Montaigut, J. Montier, E. Morelle, B. Morton, S. Mottola, R. Naves, J. Nomen, J. Oey, W. Ogłoza, M. Paiella, H. Pallares, A. Peyrot, F. Pilcher, J.-F. Pirenne, P. Piron, M. Polińska, M. Polotto, R. Poncy, J. P. Previt, F. Reignier, D. Renauld, D. Ricci, F. Richard, C. Rinner, V. Risoldi, D. Robilliard, D. Romeuf, G. Rousseau, R. Roy, J. Ruthroff, P. A. Salom, L. Salvador, S. Sanchez, T. Santana-Ros, A. Scholz, G. Séné, B. Skiff, K. Sobkowiak, P. Sogorb, F. Soldán, A. Spiridakis, E. Splanska, S. Sposetti, D. Starkey, R. Stephens, A. Stiepen, R. Stoss, J. Strajnic, J.-P. Teng, G. Tumolo, A. Vagnozzi, B. Vanoutryve, J. M. Vugnon, B. D. Warner, M. Waucomont, O. Wertz, M. Winiarski, M. Wolf
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A108. ⟨10.1051/0004-6361/201527441⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Context. Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. These efforts already provided deep insight into physical properties of main-belt asteroids or larg
Autor:
Jari J. E. Kajava, K. Sobkowiak, F. Manzini, G. Santacana, C. Bembrick, A. Marciniak, R. Hirsch, Raoul Behrend, R. Poncy, Tayyaba Zafar, Desiree Della Monica Ferreira, Magdalena Polińska, Krzysztof Kamiński, S. Starczewski, Florent Colas, R. P. Hein Bertelsen, L. Bernasconi, S. Fauvaud, David Higgins, N. Esseiva, Michał J. Michałowski, R. Crippa, P. Antonini, T. Kwiatkowski, M. Fauvaud, F. P. Velichko, M. Fagas, A. Paschke, R. Roy, M. Stasik, J. M. Coloma, Tadeusz Michalowski, J. Michałowski, Agnieszka Kryszczyńska, Przemyslaw Bartczak, W. Borczyk, H. Wücher, Toni Santana-Ros
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 545, ⟨10.1051/0004-6361/201219542⟩
Marciniak, A, Bartczak, P, Santana-Ros, T, Michałowski, T, Borczyk, W, Fagas, M, Hirsch, R, Kamiński, K, Kryszczyńska, A, Kwiatkowski, T, Polińska, M, Sobkowiak, K, Stasik, M, Antonini, P, Behrend, R, Bembrick, C, Bernasconi, L, Colas, F, Coloma, J, Crippa, R, Manzini, F, Esseiva, N, Santacana, G, Wucher, H, Fauvaud, M, Fauvaud, S, Ferreira, D D M, Hein Bertelsen, R P, Higgins, D, Kajava, J J E, Michałowski, J, Michałowski, M J, Paschke, A, Poncy, R, Roy, R, Starczewski, S, Velichko, F & Zafar, T 2012, ' Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM) ', Astronomy and Astrophysics, vol. 545, A131 . https://doi.org/10.1051/0004-6361/201219542
Astronomy and Astrophysics-A&A, 2012, 545, ⟨10.1051/0004-6361/201219542⟩
Astronomy & astrophysics, 545:A131. EDP Sciences
Astronomy and Astrophysics-A&A, EDP Sciences, 2012, 545, ⟨10.1051/0004-6361/201219542⟩
Marciniak, A, Bartczak, P, Santana-Ros, T, Michałowski, T, Borczyk, W, Fagas, M, Hirsch, R, Kamiński, K, Kryszczyńska, A, Kwiatkowski, T, Polińska, M, Sobkowiak, K, Stasik, M, Antonini, P, Behrend, R, Bembrick, C, Bernasconi, L, Colas, F, Coloma, J, Crippa, R, Manzini, F, Esseiva, N, Santacana, G, Wucher, H, Fauvaud, M, Fauvaud, S, Ferreira, D D M, Hein Bertelsen, R P, Higgins, D, Kajava, J J E, Michałowski, J, Michałowski, M J, Paschke, A, Poncy, R, Roy, R, Starczewski, S, Velichko, F & Zafar, T 2012, ' Photometry and models of selected main belt asteroids: IX. Introducing interactive service for asteroid models (ISAM) ', Astronomy and Astrophysics, vol. 545, A131 . https://doi.org/10.1051/0004-6361/201219542
Astronomy and Astrophysics-A&A, 2012, 545, ⟨10.1051/0004-6361/201219542⟩
Astronomy & astrophysics, 545:A131. EDP Sciences
Context. The shapes and spin states of asteroids observed with photometric techniques can be reconstructed using the lightcurve inversion method. The resultant models can then be confirmed or exploited further by other techniques, such as adaptive op
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73592359de720ef5d353e6c2544f12ec
https://hal.archives-ouvertes.fr/hal-01442146
https://hal.archives-ouvertes.fr/hal-01442146