Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Frederick Pilcher"'
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:
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:
Josef Hanus, Luc Arnold, Maria J. Esteban, E. Morelle, H. Gully, P. Antonini, Peter Kusnirak, Silvano Casulli, Marco Delbo, F. Manzini, P. Pravec, H. Cibulková, Bryce Bolin, Victor Ali-Lagoa, J. Michelet, Josef Ďurech, M. Lehký, H. de Groot, R. Dymock, L. Bernasconi, M. Bachschmidt, M. Audejean, Julian Oey, P. A. Salom, Robert Jedicke, N. Esseiva, Brian D. Warner, L. Brunetto, Raoul Behrend, F. Marchis, Rupak Roy, Frederick Pilcher, Hiroko Hamanowa, F. Reignier, P. Krafft, Hiromi Hamanowa, O. Gerteis
Publikováno v:
Icarus
Icarus, Elsevier, 2018, 299, pp.84-96. ⟨10.1016/j.icarus.2017.07.007⟩
Icarus, Elsevier, 2018, 299, pp.84-96. ⟨10.1016/j.icarus.2017.07.007⟩
Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. We aim to increase the number of asteroid shape models and rotation sta
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:
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:
R. Dymock, F. Manzini, S. Boroumand, Stephen M. Slivan, Robert D. Stephens, R. A. Koff, Greg Bolt, M. Fagas, R. Roy, Michael Fauerbach, Brian D. Warner, Josef Ďurech, Margaret Pan, A. Marciniak, M. Crow, Angel F. Lopez, Mikko Kaasalainen, Merideth Frey, Frederick Pilcher, Rita Pacheco, Thomas Bennett, S. Fauvaud, L. Crespo da Silva, C. Bembrick, W. Pych, Donald P. Pray, R. Crippa, Raoul Behrend, R. Poncy, S. Sposetti, Jérôme Berthier, T. Kwiatkowski, Marek Wolf, G. Santacana, R. Durkee, D. Jardine, Krzysztof Kamiński, Tadeusz Michalowski, W. H. Allen, Rui Soles Gonçalves, L. Bernasconi, R. Hirsch
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2007, 465, pp.331-337. ⟨10.1051/0004-6361:20066347⟩
Astronomy and Astrophysics-A&A, 2007, 465, pp.331-337. ⟨10.1051/0004-6361:20066347⟩
International audience; Aims:We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network o
Autor:
Robert D. Stephens, Julian Oey, Josef Ďurech, Josef Hanus, Frederick Pilcher, Q. Ulisse, R. Girelli, R. A. Koff, Brian D. Warner, L. P. Strabla, James W. Brinsfield, Miroslav Brož, David Higgins, R. Durkee
Current amount of ~500 asteroid models derived from the disk-integrated photometry by the lightcurve inversion method allows us to study not only the spin-vector properties of the whole population of MBAs, but also of several individual collisional f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bf37504289286a28728eaf15a44bed9
http://arxiv.org/abs/1309.4296
http://arxiv.org/abs/1309.4296
Autor:
Josef Hanus, Brad Timerson, Josef Ďurech, Frederick Pilcher, D. Dunham, Mikko Kaasalainen, Adrian Galad, Brian D. Warner, D. Herald, E. Frappa, John Talbot, Tsutomu Hayamizu
Publikováno v:
Icarus
Icarus, Elsevier, 2011, 214 (2), pp.652. 〈10.1016/j.icarus.2011.03.016〉
Icarus, Elsevier, 2011, 214 (2), pp.652. ⟨10.1016/j.icarus.2011.03.016⟩
Icarus, Elsevier, 2011, 214 (2), pp.652. 〈10.1016/j.icarus.2011.03.016〉
Icarus, Elsevier, 2011, 214 (2), pp.652. ⟨10.1016/j.icarus.2011.03.016⟩
Asteroid sizes can be directly measured by observing occultations of stars by asteroids. When there are enough observations across the path of the shadow, the asteroid's projected silhouette can be reconstructed. Asteroid shape models derived from ph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aea00c3b006df05a720812385ce24b32
https://hal.archives-ouvertes.fr/hal-00786870
https://hal.archives-ouvertes.fr/hal-00786870
Autor:
S. Casulli, Brian D. Warner, Tomáš Henych, Julian Oey, Robert D. Stephens, Miroslav Brož, Frederick Pilcher, Raoul Behrend, Takashi Ito, L. Bernasconi, David Polishook, Josef Ďurech, Fumi Yoshida, M. Lehký, Josef Hanus
Tens of thousands of sparse-in-time lightcurves from astrometric projects are publicly available. We investigate these data and use them in the lightcurve inversion method to derive new asteroid models. By having a greater number of models with known
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2832944b1f606c12c7c9f33c41904ba5