Search Results - "Sobkowiak, K."

Asteroid phase curves using sparse Gaia DR2 data and differential dense light curves by Wilawer, E, Oszkiewicz, D, Kryszczyńska, A, Marciniak, A, Shevchenko, V, Belskaya, I, Kwiatkowski, T, Kankiewicz, P, Horbowicz, J, Kudak, V, Kulczak, P, Perig, V, Sobkowiak, K

“…ABSTRACT The amount of sparse asteroid photometry being gathered by both space- and ground-based surveys is growing exponentially. This large volume of data…”
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Against the biases in spins and shapes of asteroids by Marciniak, A., Pilcher, F., Oszkiewicz, D., Santana-Ros, T., Urakawa, S., Fauvaud, S., Kankiewicz, P., Tychoniec, Ł., Fauvaud, M., Hirsch, R., Horbowicz, J., Kamiński, K., Konstanciak, I., Kosturkiewicz, E., Murawiecka, M., Nadolny, J., Nishiyama, K., Okumura, S., Polińska, M., Richard, F., Sakamoto, T., Sobkowiak, K., Stachowski, G., Trela, P.

“…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…”
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The small binary asteroid (939) Isberga by Carry, B., Matter, A., Scheirich, P., Pravec, P., Molnar, L., Mottola, S., Carbognani, A., Jehin, E., Marciniak, A., Binzel, R.P., DeMeo, F.E., Birlan, M., Delbo, M., Barbotin, E., Behrend, R., Bonnardeau, M., Colas, F., Farissier, P., Fauvaud, M., Fauvaud, S., Gillier, C., Gillon, M., Hellmich, S., Hirsch, R., Leroy, A., Manfroid, J., Montier, J., Morelle, E., Richard, F., Sobkowiak, K., Strajnic, J., Vachier, F.

“…•We study the small main-belt binary asteroid (939) Isberga.•Isberga is a Sq-type asteroid from near-infrared spectroscopy.•Mutual orbit, size ratio, and shape…”
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Asteroid phase curves using sparse Gaia DR2 data and differential dense light curves by Wilawer, E, Oszkiewicz, D, Kryszczyńska, A, Marciniak, A, Shevchenko, V, Belskaya, I, Kwiatkowski, T, Kankiewicz, P, Horbowicz, J, Kudak, V, Kulczak, P, Perig, V, Sobkowiak, K

“…Monthly Notices of the Royal Astronomical Society, Volume 513, Issue 3, July 2022, Pages 3242-3251 The amount of sparse asteroid photometry being gathered by…”
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Scaling slowly rotating asteroids by stellar occultations by Marciniak, A, Ďurech, J, Hanuš, J, Monteiro, F, Frappa, E, Beisker, W, Pavlov, H, Moore, J, Adomavičienė, R, Argentin, Y, Asai, A, Baruffetti, P, Bath, K. L, Behrend, R, Biguet, G, Billiani, M, Błażewicz, D, Boninsegna, R, Borkowski, M, Bosch, J, Brazill, S, Bruno, A, Casalnuovo, G, Castellani, J. J, Delincak, P, Delpau, J, Duffard, R, Durandet, C, Evangelista, M, Fauvaud, S, Fauvaud, M, Ferrais, M, Filipek, M, Fini, P, Fukui, K, Goffin, B, Goto, T, Grice, J, Guhl, K, Halíř, K, Hanna, W, Hasubick, W, Hirose, T, Hirsch, R, Horaguchi, T, Horbowicz, J, Ignácz, B, Jehin, E, Jones, A, Kamiński, K, Kankiewicz, P, Kasebe, H, Kattentidt, B, Kim, M. -J, Kitazaki, K, Klotz, A, Komraus, M, Konstanciak, I, Kouno, K, Krajewski, J, Krannich, G, Kreutzer, A, Kryszczyńska, A, Kubánek, J, Kukita, R, Kulczak, P, Lazzaro, D, Maley, P, Mánek, J, Matsushita, H, Mesquita, W, Messner, S, Michimani, J, Mieczkowska, I, Motyliński, M, Murawiecka, M, Newman, J, Nikitin, V, Owada, M, Pawłowski, M, Perła, J, Pilcher, F, Podlewska-Gaca, E, Polák, J, Polakis, T, Richard, F, Rives, J. J, Rodrigues, T, Rondón, E, Rottenborn, M, Schreurs, O, Simon, M, Skrutskie, M, Sonbas, E, Stuart, P, Thomas, W, Winiarski, M, Yamashita, M, Yoshihara, H, Zelený, P

“…A&A 679, A60 (2023) As evidenced by recent survey results, majority of asteroids are slow rotators (P>12 h), but lack spin and shape models due to selection…”
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Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model by 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, Bąk, M. Butkiewicz, Del Freo, F, Duffard, R, Evangelista-Santana, M, Farroni, G, Fauvaud, S, Fauvaud, M, Ferrais, M, Geier, S, Golonka, J, Grice, J, Hirsch, R, Horbowicz, J, Jehin, E, Julien, P, Kalup, Cs, Kamiński, K, Kamińska, M. K, Kankiewicz, P, Kecskeméthy, V, Kim, D. -H, Kim, M. -J, Konstanciak, I, Krajewski, J, Kudak, V, Kulczak, P, Kundera, T, Lazzaro, D, Manzini, F, Medeiros, H, Michimani-Garcia, J, Morales, N, Nadolny, J, Oszkiewicz, D, Pakštienė, E, Pawłowski, M, Perig, V, Pilcher, F, Pinel, P, Podlewska-Gaca, E, Polakis, T, Richard, F, Rodrigues, T, Rondon, E, Roy, R, Sanabria, J. J, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Stachowski, G, Strajnic, J, Trela, P, Tychoniec, Ł, Urakawa, S, Verebelyi, E, Wagrez, K, Żejmo, M, Żukowski, K

“…A&A 654, A87 (2021) Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of…”
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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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(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body by Hanuš, J, Vernazza, P, Viikinkoski, M, Ferrais, M, Rambaux, N, Podlewska-Gaca, E, Drouard, A, Jorda, L, Jehin, E, Carry, B, Marsset, M, Marchis, F, Warner, B, Behrend, R, Asenjo, V, Berger, N, Bronikowska, M, Brothers, T, Charbonnel, S, Colazo, C, Coliac, J-F, Duffard, R, Jones, A, Leroy, A, Marciniak, A, Melia, R, Molina, D, Nadolny, J, Person, M, Pejcha, O, Riemis, H, Shappee, B, Sobkowiak, K, Soldán, F, Suys, D, Szakats, R, Vantomme, J, Birlan, M, Berthier, J, Bartczak, P, Dumas, C, Dudziński, G, Ďurech, J, Castillo-Rogez, J, Cipriani, F, Fetick, R, Fusco, T, Grice, J, Kaasalainen, M, Kryszczynska, A, Lamy, P, Michalowski, T, Michel, P, Santana-Ros, T, Tanga, P, Vachier, F, Vigan, A, Witasse, O, Yang, B

“…A&A 633, A65 (2020) With an estimated diameter in the 320 to 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies…”
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Thermal properties of slowly rotating asteroids: Results from a targeted survey by Marciniak, A, Alí-Lagoa, V, Müller, T. G, Szakáts, R, Molnár, L, Pál, A, Gaca, E. Podlewska, Parley, N, Antonini, P, Barbotin, E, Behrend, R, Bernasconi, L, Bąk, M. Butkiewicz, Crippa, R, Duffard, R, Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S, Goncalves, R, Grice, J, Grześkowiak, I, Hirsch, R, Horbowicz, J, Kamiński, K, Kamińska, M. K, Kim, D. -H, Kim, M. -J, Konstanciak, I, Kudak, V, Kulczak, P, Maestre, J. L, Manzini, F, Marks, S, Monteiro, F, Ogłoza, W, Oszkiewicz, D, Pilcher, F, Perig, V, Polakis, T, Polińska, M, Roy, R, Sanabria, J. J, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Żejmo, M, Żukowski, K

“…A&A 625, A139 (2019) Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat…”
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Against the biases in spins and shapes of asteroids by Marciniak, A, Pilcher, F, Oszkiewicz, D, Santana-Ros, T, Urakawa, S, Fauvaud, S, Kankiewicz, P, Tychoniec, Ł, Fauvaud, M, Hirsch, R, Horbowicz, J, Kamiński, K, Konstanciak, I, Kosturkiewicz, E, Murawiecka, M, Nadolny, J, Nishiyama, K, Okumura, S, Polińska, M, Richard, F, Sakamoto, T, Sobkowiak, K, Stachowski, G, Trela, P

“…Marciniak et al. 2015, PSS, 118, 256 Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse…”
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Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids by Marciniak, A, Bartczak, P, Müller, T, Sanabria, J. J, Alí-Lagoa, V, Antonini, P, Behrend, R, Bernasconi, L, Bronikowska, M, Bąk, M. Butkiewicz, Cikota, A, Crippa, R, Ditteon, R, Dudziński, G, Duffard, R, Dziadura, K, Fauvaud, S, Geier, S, Hirsch, R, Horbowicz, J, Hren, M, Jerosimic, L, Kamiński, K, Kankiewicz, P, Konstanciak, I, Korlevic, P, Kosturkiewicz, E, Kudak, V, Manzini, F, Morales, N, Murawiecka, M, Ogłoza, W, Oszkiewicz, D, Pilcher, F, Polakis, T, Poncy, R, Santana-Ros, T, Siwak, M, Skiff, B, Sobkowiak, K, Stoss, R, Żejmo, M, Żukowski, K

“…The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a…”
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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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The small binary asteroid (939) Isberga by Carry, B, Matter, A, Scheirich, P, Pravec, P, Molnar, L, Mottola, S, Carbognani, A, Jehin, E, Marciniak, A, Binzel, R. P, DeMeo, F. E, Birlan, M, Delbo, M, Barbotin, E, Behrend, R, Bonnardeau, M, Colas, F, Farissier, P, Fauvaud, M, Fauvaud, S, Gillier, C, Gillon, M, Hellmich, S, Hirsch, R, Leroy, A, Manfroid, J, Montier, J, Morelle, E, Richard, F, Sobkowiak, K, Strajnic, J, Vachier, F

“…In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here to characterize the…”
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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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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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