Search Results - "Audejean, M"

Spin states of asteroids in the Eos collisional family by Hanuš, J., Delbo’, M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, Hiroko, Hamanowa, Hiromi, Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P.A., Warner, B.D.

“…•We present updated and new shape model determinations for 31 asteroids from the Eos collisional family.•We compiled a sample of shapes and rotation state…”
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Historical vanishing of the Blazhko effect of RR Lyr from the GEOS and Kepler surveys by Le Borgne, J. F., Poretti, E., Klotz, A., Denoux, E., Smith, H. A., Kolenberg, K., Szabó, R., Bryson, S., Audejean, M., Buil, C., Caron, J., Conseil, E., Corp, L., Drillaud, C., de France, T., Graham, K., Hirosawa, K., Klotz, A. N., Kugel, F., Loughney, D., Menzies, K., Rodríguez, M., Ruscitti, P. M.

“…RR Lyr is one of the most studied variable stars. Its light curve has been regularly monitored since the discovery of its periodic variability in 1899. The…”
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The non-convex shape of (234) Barbara, the first Barbarian by Tanga, P., Carry, B., Colas, F., Delbo, M., Matter, A., Hanuš, J., Alí Lagoa, V., Andrei, A. H., Assafin, M., Audejean, M., Behrend, R., Camargo, J. I. B., Carbognani, A., Cedrés Reyes, M., Conjat, M., Cornero, N., Coward, D., Crippa, R., de Ferra Fantin, E., Devogéle, M., Dubos, G., Frappa, E., Gillon, M., Hamanowa, H., Jehin, E., Klotz, A., Kryszczyńska, A., Lecacheux, J., Leroy, A., Manfroid, J., Manzini, F., Maquet, L., Morelle, E., Mottola, S., Polińska, M., Roy, R., Todd, M., Vachier, F., Vera Hernández, C., Wiggins, P.

“…Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever…”
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Asteroid spin-states of a 4 Gyr collisional family by Athanasopoulos, D, Hanus, J, Avdellidou, C, Bonamico, R, Delbo, M, Conjat, M, Ferrero, A, Gazeas, K, Rivet, J. P, Sioulas, N, van Belle, G, Antonini, P, Audejean, M, Behrend, R, Bernasconi, L, Brinsfield, J. W, Brouillard, S, Brunetto, L, Fauvaud, M, Fauvaud, S, González, R, Higgins, D, Holoien, T. W. -S, Kobber, G, Koff, R. A, Kryszczynska, A, Livet, F, Marciniak, A, Oey, J, Pejcha, O, Rives, J. J, Roy, R

“…Families of asteroids generated by the collisional fragmentation of a common parent body have been identified using clustering methods of asteroids in their…”
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Physical parameters of selected Gaia mass asteroids by Podlewska-Gaca, E, Marciniak, A, Alí-Lagoa, V, Bartczak, P, Müller, T. G, Szakáts, R, Duffard, R, Molnár, L, Pál, A, Butkiewicz-Bąk, M, Dudziński, G, Dziadura, K, Antonini, P, Asenjo, V, Audejean, M, Benkhaldoun, Z, Behrend, R, Bernasconi, L, Bosch, J. M, Chapman, A, Dintinjana, B, Farkas, A, Ferrais, M, Geier, S, Grice, J, Hirsh, R, Jacquinot, H, Jehin, E, Jones, A, Molina, D, Morales, N, Parley, N, Poncy, R, Roy, R, Santana-Ros, T, Seli, B, Sobkowiak, K, Verebélyi, E, Żukowski, K

“…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…”
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Spin states of asteroids in the Eos collisional family by Hanuš, J, Delbo', M, Alí-Lagoa, V, Bolin, B, Jedicke, R, Ďurech, J, Cibulková, H, Pravec, P, Kušnirák, P, Behrend, R, Marchis, F, Antonini, P, Arnold, L, Audejean, M, Bachschmidt, M, Bernasconi, L, Brunetto, L, Casulli, S, Dymock, R, Esseiva, N, Esteban, M, Gerteis, O, de Groot, H, Gully, H, Hamanowa, H, Krafft, P, Lehký, M, Manzini, F, Michelet, J, Morelle, E, Oey, J, Pilcher, F, Reignier, F, Roy, R, Salom, P. A, Warner, B. D

“…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…”
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Shape and spin determination of Barbarian asteroids by Devogèle, M, Tanga, P, Bendjoya, P, Rivet, J. P, Surdej, J, Hanus, J, Abe, L, Antonini, P, Artola, R. A, Audejean, M, Behrend, R, Berski, F, Bosch, J. G, Bronikowska, M, Carbognani, A, Char, F, Kim, M. -J, Choi, Y. -J, Colazo, C. A, Coloma, J, Coward, D, Durkee, R, Erece, O, Forne, E, Hickson, P, Hirsch, R, Horbowicz, J, Kamiński, K, Kankiewicz, P, Kaplan, M, Kwiatkowski, T, Konstanciak, I, Kruszewki, A, Kudak, V, Manzini, F, Moon, H. -K, Marciniak, A, Murawiecka, M, Nadolny, J, Ogłoza, W, Ortiz, J. L, Oszkiewicz, D, Pallares, H, Peixinho, N, Poncy, R, Reyes, F, Reyes, J. A. de los, Santana-Ros, T, Sobkowiak, K, Pastor, S, Pilcher, F, Quiñones, M. C, Trela, P, Vernet, D

“…A&A 607, A119 (2017) Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and…”
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B.R.N.O. Contributions #39 Times of minima by Hoňková, K, Juryšek, J, Lehký, M, Šmelcer, L, Mašek, M, Mazanec, J, Hanžl, D, Urbaník, M, Magris, M, Vrašták, M, Walter, F, Hladík, B, Medulka, T, Bílek, F, Trnka, J, Jacobsen, J, Benáček, J, Kuchťák, B, Audejean, M, Ögmen, Y, Zíbar, M, Fatka, P, Marchi, F, Poddaný, S, Quinones, C, Tapia, L, Scaggiante, F, Zardin, D, Corfini, G, Hájek, P, Lomoz, F, Mravik, J, Grnja, J, Campos, F, Čaloud, J, Esseiva, N, Jakš, S, Horník, M, Filip, J, Uhlář, R, Mina, F, Artola, R, Zalazar, J, Müller, D, Pintr, P, Divišová, L

“…2015OEJV..168...1H This paper presents 1463 times of minima for 455 objects acquired by 46 members and cooperating observers of the Variable Star and Exoplanet…”
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The non-convex shape of (234) Barbara, the first Barbarian by Tanga, P, Carry, B, Colas, F, Delbo, M, Matter, A, Hanus, J, Lagoa, V. Ali, Andrei, A. H, Assafin, M, Audejean, M, Behrend, R, Camargo, J. I. B, Carbognani, A, Reyes, M. Cedres, Conjat, M, Cornero, N, Coward, D, Crippa, R, Fantin, E. de Ferra, Devogele, M, Dubos, G, Frappa, E, Gillon, M, Hamanowa, H, Jehin, E, Klotz, A, Kryszczynska, A, Lecacheux, J, Leroy, A, Manfroid, J, Manzini, F, Maquet, L, Morelle, E, Mottola, S, Polinska, M, Roy, R, Todd, M, Vachier, F, Hernandez, C. Vera, Wiggins, P

“…Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever…”
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The historical vanishing of the Blazhko effect of RR Lyr from GEOS and Kepler surveys by Borgne, J. F. Le, Poretti, E, Klotz, A, Denoux, E, Smith, H. A, Kolenberg, K, Szabó, R, Bryson, S, Audejean, M, Buil, C, Caron, J, Conseil, E, Corp, L, Drillaud, C, de France, T, Graham, K, Hirosawa, K, Klotz, A. N, Kugel, F, Loughney, D, Menzies, K, guez, M. Rodrí, Ruscitti, P. M

“…MNRAS 441 (2014) 1435-1443 RR Lyr is one of the most studied variable stars. Its light curve has been regularly monitored since the discovery of the periodic…”
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New and updated convex shape models of asteroids based on optical data from a large collaboration network by Ďurech, J, Oszkiewicz, D. A, Behrend, R, Carry, B, Delbo', M, Adam, O, Afonina, V, Antonini, P, Arnold, L, Audejean, M, Aurard, P, Badue, B, Barbotin, E, Barroy, P, Baudouin, P, Berard, L, Berger, N, Bernasconi, L, Bozhinova, I, Brinsfield, J, Canaud, G, Caron, J, Carrier, F, Casalnuovo, G, Casulli, S, Cerda, M, Chalamet, L, Charbonnel, S, Chinaglia, B, Cikota, A, Colas, F, Coliac, J-F, Coloma, J, Conseil, E, Costa, R, Debackere, A, Decock, A, Déhais, Q, Déléage, T, Dumont, M, Dymock, R, del Valle, A. Escalante, Esteban, M, Fauerbach, M, Fournel, C, Garlitz, J, Gillier, C, Gillon, M, Hay, K, Hellmich, S, Heterier, S, Hirsch, R, Hodosan, G, Hren, M, Jacquinot, H, Jawahar, S, Jehin, E, Jerosimic, L, Klotz, A, Koff, W, Korlevic, P, Kosturkiewicz, E, Krafft, P, Kugel, F, Lecacheux, J, Leroy, A, Lopez-Gonzales, M. J, Lutz, M, Mallecot, B, Manfroid, J, Manzini, F, Marciniak, A, Modave, B, Morelle, E, Oey, J, Ogłoza, W, Paiella, M, Peyrot, A, Pilcher, F, Pirenne, J-F, Polinska, M, Polotto, M, Poncy, R, Previt, J. P, Reignier, F, Renauld, D, Richard, F, Risoldi, V, Romeuf, D, Salom, P. A, Sanchez, S, Santana-Ros, T, Stephens, R, Stoss, R, Strajnic, J, Teng, J-P, Vagnozzi, A, Warner, B. D, Winiarski, M, Wolf, M

“…A&A 586, A108 (2016) Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation…”
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SOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet by Santerne, A, Hébrard, G, Deleuil, M, Havel, M, Correia, A. C. M, Almenara, J. -M, Alonso, R, Arnold, L, Barros, S. C. C, Behrend, R, Bernasconi, L, Boisse, I, Bonomo, A. S, Bouchy, F, Bruno, G, Damiani, C, Díaz, R. F, Gravallon, D, Guillot, T, Labrevoir, O, Montagnier, G, Moutou, C, Rinner, C, Santos, N. C, Abe, L, Audejean, M, Bendjoya, P, Gillier, C, Gregorio, J, Martinez, P, Michelet, J, Montaigut, R, Poncy, R, Rivet, J. -P, Rousseau, G, Roy, R, Suarez, O, Vanhuysse, M, Verilhac, D

“…A&A 571, A37 (2014) In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the…”
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Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution by Ďurech, J, Brož, M, Marciniak, A, Warner, B. D, Pilcher, F, Stephens, R, Behrend, R, Čapek, D, Antonini, P, Audejean, M, Augustesen, K, Barbotin, E, Bayol, A, Bernasconi, L, Borczyk, W, Bosch, J. -G, Brochard, E, Brunetto, L, Cazenave, A, Charbonnel, S, Christophe, B, Colas, F, Coloma, J, Conjat, M, Cooney, W, Correira, H, Coupier, A, Crippa, R, Cristofanelli, M, Dalmas, Ch, Danavaro, C, Demeautis, C, Droege, T, Durkee, R, Esseiva, N, Fagas, M, Farroni, G, Fauvaud, M, Fauvaud, S, Del Freo, F, Garcia, L, Geier, S, Godon, C, Grangeon, K, Hamanowa, H, Heck, N, Hellmich, S, Higgins, D, Husarik, M, Itkonen, T, Jade, O, Kamiński, K, Kankiewicz, P, Koff, R. A, Laffont, A, Leroy, A, Leonie, Y, Leyrat, C, Manzini, F, Martin, A, Michałowski, J, Michałowski, M. J, Michałowski, T, Michelet, J, Michelsen, R, Morelle, E, Mottola, S, Naves, R, Nomen, J, Oey, J, Ogloza, W, Oksanen, A, Pääkkönen, P, Paiella, M, Pavic, M, Payet, B, Polińska, M, Polishook, D, Poncy, R, Revaz, Y, Rocca, M, Roche, A, Romeuf, D, Roy, R, Saguin, H, Salom, P. A, Sanchez, S, Santacana, G, Santana-Ros, T, Sareyan, J. -P, Sposetti, S, Starkey, D, Stoss, R, Strajnic, J, Teng, J. -P, Tregon, B, Vagnozzi, A, Velichko, F. P, Waelchli, N, Wagrez, K

“…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…”
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