Zobrazeno 1 - 10
of 42
pro vyhledávání: '"K. Sobkowiak"'
Autor:
E Wilawer, D Oszkiewicz, A Kryszczyńska, A Marciniak, V Shevchenko, I Belskaya, T Kwiatkowski, P Kankiewicz, J Horbowicz, V Kudak, P Kulczak, V Perig, K Sobkowiak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 513:3242-3251
The amount of sparse asteroid photometry being gathered by both space- and ground-based surveys is growing exponentially. This large volume of data poses a computational challenge owing to both the large amount of information to be processed and the
Akademický článek
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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
Autor:
Emmanuel Jehin, Neil Parley, E. Podlewska-Gaca, Anna Marciniak, Thomas G. Müller, Josep M. Bosch, Zouhair Benkhaldoun, Lawrence A. Molnar, L. Bernasconi, K. Sobkowiak, A. Farkas, Bojan Dintinjana, Grzegorz Dudziński, Rene Duffard, M. Audejean, Raoul Behrend, A. Chapman, K. Żukowski, Aled Jones, Erika Verebélyi, R. Poncy, Victor Ali-Lagoa, V. Asenjo, Nicolás Morales, Karolina Dziadura, J. Grice, Róbert Szakáts, R. Roy, M. Butkiewicz-Bąk, S. Geier, Bálint Seli, Przemyslaw Bartczak, D. Molina, Roman Hirsh, P. Antonini, Marin Ferrais, András Pál, Toni Santana-Ros, Herve Jacquinot
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Universidad de Alicante (UA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Context. Thanks to the Gaia mission, it will be possible to determine the masses of approximately hundreds of large main belt asteroids with very good precision. We currently have diameter estimates for all of them that can be used to compute their v
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f152887b78639a7e7a649ed26abc3363
http://hdl.handle.net/10045/108361
http://hdl.handle.net/10045/108361
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:
Jose Luis Ortiz, A. Kruszewki, R. Hirsch, Rodolfo Alfredo Artola, Paweł Kankiewicz, P. Antonini, Filip Berski, David Vernet, Josef Hanus, Orhan Erece, Myung-Jin Kim, I. Konstanciak, Hong-Kyu Moon, S. Pastor, E. Forne, Małgorzata Bronikowska, Krzysztof Kamiński, Young-Jun Choi, Murat Kaplan, K. Sobkowiak, Frederick Pilcher, P. Trela, Federico Manzini, Toni Santana-Ros, F. Reyes, Paul Hickson, Waldemar Ogloza, Paolo Tanga, J.-G. Bosch, T. Kwiatkowski, M. Murawiecka, Lyu Abe, Maxime Devogele, V. Kudak, F. Char, Jean Surdej, R. Durkee, Anna Marciniak, P. Bendjoya, J. M. Coloma, Dagmara Oszkiewicz, David Coward, Raoul Behrend, R. Poncy, J. Horbowicz, C. Colazo, J. P. Rivet, J.A. de los Reyes, M. C. Quiñones, Jakub Nadolny, Nuno Peixinho, Albino Carbognani, M. Audejean, H. Pallares
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
NASA Astrophysics Data System
instname
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
NASA Astrophysics Data System
Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barbara, the first on which such properties were identified. As has been s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9ac59db71fae9ba36cd505a70b3fae7
http://arxiv.org/abs/1707.07503
http://arxiv.org/abs/1707.07503
Autor:
Toni Santana-Ros, Przemyslaw Bartczak, F. Manzini, Th. Müller, I. Konstanciak, Paweł Kankiewicz, J. J. Sanabria, R. Stoss, Krzysztof Kamiński, Waldemar Ogloza, Grzegorz Dudziński, Nicolás Morales, K. Sobkowiak, Rene Duffard, L. Jerosimic, K. Żukowski, Frederick Pilcher, M. Butkiewicz-Bąk, Raoul Behrend, R. Poncy, V. Kudak, E. Kosturkiewicz, L. Bernasconi, R. Hirsch, S. Fauvaud, Tom Polakis, Aleksandar Cikota, Michal Siwak, Brian A. Skiff, R. Crippa, S. Geier, J. Horbowicz, Victor Ali-Lagoa, Karolina Dziadura, Michał Żejmo, M. Hren, P. Korlevic, P. Antonini, Dagmara Oszkiewicz, Małgorzata Bronikowska, R. Ditteon, M. Murawiecka, A. Marciniak
Publikováno v:
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Marciniak, A. et. al..-- 33 p.
The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. This is due to the observing selection effects. As a consequence,
The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. This is due to the observing selection effects. As a consequence,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea08fe559dfe2ebf300399fc47ceb483
Autor:
A. Marciniak, Krzysztof Kamiński, R. Hirsch, K. Sobkowiak, Tadeusz Michalowski, L. Bernasconi, Magdalena Polińska, S. Starczewski, J. Michałowski, Agnieszka Kryszczyńska, M. Fagas, Raoul Behrend, T. Kwiatkowski
Publikováno v:
Astronomy & Astrophysics. 498:313-320
We present a set of new photometric observations of three main belt asteroids: 160 Una, 747 Winchester, and 849 Ara. This, combined with the available data, allowed us to construct their physical models. The lightcurve inversion method was used to ob
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