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47 results on '"Behrend R"'

1. Scaling slowly rotating asteroids with stellar occultations

Author: Marciniak, A., primary, Ďurech, J., additional, Choukroun, A., additional, Hanuš, J., additional, Ogłoza, W., additional, Szakáts, R., additional, Molnár, L., additional, Pál, A., additional, Monteiro, F., additional, Frappa, E., additional, Beisker, W., additional, Pavlov, H., additional, Moore, J., additional, Adomavičienė, R., additional, Aikawa, R., additional, Andersson, S., additional, Antonini, P., additional, Argentin, Y., additional, Asai, A., additional, Assoignon, P., additional, Barton, J., additional, Baruffetti, P., additional, Bath, K. L., additional, Behrend, R., additional, Benedyktowicz, L., additional, Bernasconi, L., additional, Biguet, G., additional, Billiani, M., additional, Błażewicz, D., additional, Boninsegna, R., additional, Borkowski, M., additional, Bosch, J., additional, Brazill, S., additional, Bronikowska, M., additional, Bruno, A., additional, Butkiewicz-Bąk, M., additional, Caron, J., additional, Casalnuovo, G., additional, Castellani, J. J., additional, Ceravolo, P., additional, Conjat, M., additional, Delincak, P., additional, Delpau, J., additional, Demeautis, C., additional, Demirkol, A., additional, Dróżdż, M., additional, Duffard, R., additional, Durandet, C., additional, Eisfeldt, D., additional, Evangelista, M., additional, Fauvaud, S., additional, Fauvaud, M., additional, Ferrais, M., additional, Filipek, M., additional, Fini, P., additional, Fukui, K., additional, Gährken, B., additional, Geier, S., additional, George, T., additional, Goffin, B., additional, Golonka, J., additional, Goto, T., additional, Grice, J., additional, Guhl, K., additional, Halíř, K., additional, Hanna, W., additional, Harman, M., additional, Hashimoto, A., additional, Hasubick, W., additional, Higgins, D., additional, Higuchi, M., additional, Hirose, T., additional, Hirsch, R., additional, Hofschulz, O., additional, Horaguchi, T., additional, Horbowicz, J., additional, Ida, M., additional, Ignácz, B., additional, Ishida, M., additional, Isobe, K., additional, Jehin, E., additional, Joachimczyk, B., additional, Jones, A., additional, Juan, J., additional, Kamiński, K., additional, Kamińska, M. K., additional, Kankiewicz, P., additional, Kasebe, H., additional, Kattentidt, B., additional, Kim, D.-H., additional, Kim, M.-J., additional, Kitazaki, K., additional, Klotz, A., additional, Komraus, M., additional, Konstanciak, I., additional, Könyves-Tóth, R., additional, Kouno, K., additional, Kowald, E., additional, Krajewski, J., additional, Krannich, G., additional, Kreutzer, A., additional, Kryszczyńska, A., additional, Kubánek, J., additional, Kudak, V., additional, Kugel, F., additional, Kukita, R., additional, Kulczak, P., additional, Lazzaro, D., additional, Licandro, J., additional, Livet, F., additional, Maley, P., additional, Manago, N., additional, Mánek, J., additional, Manna, A., additional, Matsushita, H., additional, Meister, S., additional, Mesquita, W., additional, Messner, S., additional, Michelet, J., additional, Michimani, J., additional, Mieczkowska, I., additional, Morales, N., additional, Motyliński, M., additional, Murawiecka, M., additional, Newman, J., additional, Nikitin, V., additional, Nishimura, M., additional, Oey, J., additional, Oszkiewicz, D., additional, Owada, M., additional, Pakštienė, E., additional, Pawłowski, M., additional, Pereira, W., additional, Perig, V., additional, Perła, J., additional, Pilcher, F., additional, Podlewska-Gaca, E., additional, Polák, J., additional, Polakis, T., additional, Polińska, M., additional, Popowicz, A., additional, Richard, F., additional, Rives, J. J, additional, Rodrigues, T., additional, Rogiński, Ł., additional, Rondón, E., additional, Rottenborn, M., additional, Schäfer, R., additional, Schnabel, C., additional, Schreurs, O., additional, Selva, A., additional, Simon, M., additional, Skiff, B., additional, Skrutskie, M., additional, Skrzypek, J., additional, Sobkowiak, K., additional, Sonbas, E., additional, Sposetti, S., additional, Stuart, P., additional, Szyszka, K., additional, Terakubo, K., additional, Thomas, W., additional, Trela, P., additional, Uchiyama, S., additional, Urbanik, M., additional, Vaudescal, G., additional, Venable, R., additional, Watanabe, Ha., additional, Watanabe, Hi., additional, Winiarski, M., additional, Wróblewski, R., additional, Yamamura, H., additional, Yamashita, M., additional, Yoshihara, H., additional, Zawilski, M., additional, Zelený, P., additional, Żejmo, M., additional, Żukowski, K., additional, and Żywica, S., additional
Published: 2023
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2. Asteroid spin-states of a 4 Gyr collisional family

Author: Athanasopoulos, D., primary, Hanuš, J., additional, Avdellidou, C., additional, Bonamico, R., additional, Delbo, M., additional, Conjat, M., additional, Ferrero, A., additional, Gazeas, K., additional, Rivet, J. P., additional, Sioulas, N., additional, van Belle, G., additional, Antonini, P., additional, Audejean, M., additional, Behrend, R., additional, Bernasconi, L., additional, Brinsfield, J. W., additional, Brouillard, S., additional, Brunetto, L., additional, Fauvaud, M., additional, Fauvaud, S., additional, Gonzalez, R., additional, Higgins, D., additional, Holoien, T. W.-S., additional, Kober, G., additional, Koff, R. A., additional, Kryszczynska, A., additional, Livet, F., additional, Marciniak, A., additional, Oey, J., additional, Pejcha, O., additional, Rives, J. J., additional, and Roy, R., additional
Published: 2022
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3. Constraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observations

Author: Física aplicada I, Fisika aplikatua I, Marques Oliveira, Joana, Sicardy, Bruno, Gómes Junior, A.R., Ortiz, J.L., Strobel, D.F., Bertrand, T., Forget, F., Lellouch, E., Desmars, J., Bérard, D., Doressoundiram, A., Lecacheux, J., Leiva, R., Meza, E., Roques, F., Souami, D., Widemann, T., Santos Sanz, Pablo, Morales, N., Duffard, Rene, Fernández Valenzuela, Estela, Castro Tirado, A.J., Braga Ribas, Felipe, Morgado, Bruno, Assafin, Marcelo, Bueno de Camargo, Julio Ignacio, Vieira Martins, Roberto, Benedetti Rossi, Gustavo, Santos Filho, S., Banda Huarca, M.V., Quispe Huaynasi, F., Pereira, Chrystian Luciano, Rommel, Flavia Luane, Margoti, Giuliano, Dias Oliveira, A., Colas, F., Berthier, J., Renner, S., Hueso, Ricardo, Pérez Hoyos, Santiago, Sánchez Lavega, Agustín María, Rojas Palenzuela, José Félix, Beisker, W., Kretlow, Mike, Herald, D., Gault, D., Bath, K.-L., Bode, H.-J., Bredner, E., Guhl, K., Haymes, T.V., Hummel, E., Kattentidt, B., Klös, O., Pratt, A., Thome, B., Avdellidou, Chrysa, Gazeas, K., Karampotsiou, E., Tzouganatos, L., Kardasis, E., Christou, A.A., Xilouris, Emmanuel, Alikakos, I., Gourzelas, A., Liakos, Alexios, Charmandaris, Vassilis, Jelínek, Martin, Štrobl, Jan, Eberle, A., Rapp, K., Gährken, B., Klemt, B., Kowollik, S., Bitzer, R., Miller, M., Herzogenrath, G., Frangenberg, Dirk, Brandis, L., Pütz, I., Perdelwitz, Volker, Piehler, G. M., Riepe, P., von Poschinger, K., Baruffetti, P., Cenadelli, D., Christille, J.-M., Ciabattari, F., Di Luca, R., Alboresi, D., Leto, Giuseppe, Zanmar Sánchez, R., Bruno, P., Occhipinti, G., Morrone, L., Cupolino, L., Noschese, A., Vecchione, A., Scalia, Cesare, Lo Savio, R., Giardina, G., Kamoun, S., Barbosa, R., Behrend, R., Spano, M., Bouchet, E., Cottier, M., Falco, L., G. Gallego, Sofía, Tortorelli, Luca, Sposetti, S., Sussenbach, J., Van Den Abbeel, F., André, P., Llibre, M., Pailler, Frédéric, Ardissone, J., Boutet, Michel, Sánchez, J., Bretton, M., Cailleau, A., Pic, V., Granier, L., Chauvet, R., Conjat, M., Dauvergne, J.L., Dechambre, O., Delay, P., Delcroix, Marc, Rousselot, Lionel, Ferreira, João, Machado, Pedro, Tanga, P., Rivet, J.-P., Frappa, Eric, Irzyk, M., Jabet, F., Kaschinski, M., Klotz, A., Rieugnie, Y., Klotz, A.N., Labrevoir, O., Lavandier, D., Walliang, D., Leroy, A., Bouley, S., Lisciandra, S., Coliac, Jean-François, Metz, F., Erpelding, D., Nougayrede, Jean-Philippe, Midavaine, T., Miniou, M., Moindrot, S., Morel, P., Reginato, B., Reginato, E., Rudelle, J., Tregon, B., Tanguy, R., David, J., Thuillot, W., Hestroffer, D., Vaudescal, G., Baba Aissa, D., Grigahcene, Z., Briggs, D., Broadbent, Stephen, Denyer, P., Haigh, Nicholas, Quinn, N., Thurston, G., Fossey, S. J., Arena, C., Jennings, M., talbot, J., Alonso Burgos, Sergio, Román Reche, A., Casanova, V., Briggs, E., Iglesias Marzoa, Ramón, Abril Ibáñez, J., Díaz Martín, M.C., González, H., Maestre García, J.L., Marchant, Jonathan, Ordoñez Etxeberria, Iñaki, Martorell, P., Salamero, J., Organero, F., Ana, L., Fonseca, F., Peris, V., Brevia, O., Selva, A., Perelló Pérez, Carlos, Cabedo, V., Gonçalves, Rui M. D., Ferreira, M., Marques Dias, Filipe, Daassou, A., Barkaoui, Khalid, Benkhaldoun, Z., Guennoun, M., Chouqar, J., Jehin, E., Rinner, C., Lloyd, J., El Moutamid, Maryame, Lamarche, C., Pollock, J.T., caton, D.B., Kouprianov, Vladimir, Timerson, B.W., Blanchard, G., Payet, B., Peyrot, A., Teng-Chuen-Yu, J.-P., Françoise, J., Mondon, Bernard, Payet, Thierry, Boissel, C., Castets, M., Hubbard, William, Hill, R., Reitsema, H. J., Mousis, Olivier, Ball, L., Neilsen, G., Hutcheon, S., lay, K., Anderson, P., Moy, M., Jonsen, M., Pink, I., Walters, R., Downs, B., Física aplicada I, Fisika aplikatua I, Marques Oliveira, Joana, Sicardy, Bruno, Gómes Junior, A.R., Ortiz, J.L., Strobel, D.F., Bertrand, T., Forget, F., Lellouch, E., Desmars, J., Bérard, D., Doressoundiram, A., Lecacheux, J., Leiva, R., Meza, E., Roques, F., Souami, D., Widemann, T., Santos Sanz, Pablo, Morales, N., Duffard, Rene, Fernández Valenzuela, Estela, Castro Tirado, A.J., Braga Ribas, Felipe, Morgado, Bruno, Assafin, Marcelo, Bueno de Camargo, Julio Ignacio, Vieira Martins, Roberto, Benedetti Rossi, Gustavo, Santos Filho, S., Banda Huarca, M.V., Quispe Huaynasi, F., Pereira, Chrystian Luciano, Rommel, Flavia Luane, Margoti, Giuliano, Dias Oliveira, A., Colas, F., Berthier, J., Renner, S., Hueso, Ricardo, Pérez Hoyos, Santiago, Sánchez Lavega, Agustín María, Rojas Palenzuela, José Félix, Beisker, W., Kretlow, Mike, Herald, D., Gault, D., Bath, K.-L., Bode, H.-J., Bredner, E., Guhl, K., Haymes, T.V., Hummel, E., Kattentidt, B., Klös, O., Pratt, A., Thome, B., Avdellidou, Chrysa, Gazeas, K., Karampotsiou, E., Tzouganatos, L., Kardasis, E., Christou, A.A., Xilouris, Emmanuel, Alikakos, I., Gourzelas, A., Liakos, Alexios, Charmandaris, Vassilis, Jelínek, Martin, Štrobl, Jan, Eberle, A., Rapp, K., Gährken, B., Klemt, B., Kowollik, S., Bitzer, R., Miller, M., Herzogenrath, G., Frangenberg, Dirk, Brandis, L., Pütz, I., Perdelwitz, Volker, Piehler, G. M., Riepe, P., von Poschinger, K., Baruffetti, P., Cenadelli, D., Christille, J.-M., Ciabattari, F., Di Luca, R., Alboresi, D., Leto, Giuseppe, Zanmar Sánchez, R., Bruno, P., Occhipinti, G., Morrone, L., Cupolino, L., Noschese, A., Vecchione, A., Scalia, Cesare, Lo Savio, R., Giardina, G., Kamoun, S., Barbosa, R., Behrend, R., Spano, M., Bouchet, E., Cottier, M., Falco, L., G. Gallego, Sofía, Tortorelli, Luca, Sposetti, S., Sussenbach, J., Van Den Abbeel, F., André, P., Llibre, M., Pailler, Frédéric, Ardissone, J., Boutet, Michel, Sánchez, J., Bretton, M., Cailleau, A., Pic, V., Granier, L., Chauvet, R., Conjat, M., Dauvergne, J.L., Dechambre, O., Delay, P., Delcroix, Marc, Rousselot, Lionel, Ferreira, João, Machado, Pedro, Tanga, P., Rivet, J.-P., Frappa, Eric, Irzyk, M., Jabet, F., Kaschinski, M., Klotz, A., Rieugnie, Y., Klotz, A.N., Labrevoir, O., Lavandier, D., Walliang, D., Leroy, A., Bouley, S., Lisciandra, S., Coliac, Jean-François, Metz, F., Erpelding, D., Nougayrede, Jean-Philippe, Midavaine, T., Miniou, M., Moindrot, S., Morel, P., Reginato, B., Reginato, E., Rudelle, J., Tregon, B., Tanguy, R., David, J., Thuillot, W., Hestroffer, D., Vaudescal, G., Baba Aissa, D., Grigahcene, Z., Briggs, D., Broadbent, Stephen, Denyer, P., Haigh, Nicholas, Quinn, N., Thurston, G., Fossey, S. J., Arena, C., Jennings, M., talbot, J., Alonso Burgos, Sergio, Román Reche, A., Casanova, V., Briggs, E., Iglesias Marzoa, Ramón, Abril Ibáñez, J., Díaz Martín, M.C., González, H., Maestre García, J.L., Marchant, Jonathan, Ordoñez Etxeberria, Iñaki, Martorell, P., Salamero, J., Organero, F., Ana, L., Fonseca, F., Peris, V., Brevia, O., Selva, A., Perelló Pérez, Carlos, Cabedo, V., Gonçalves, Rui M. D., Ferreira, M., Marques Dias, Filipe, Daassou, A., Barkaoui, Khalid, Benkhaldoun, Z., Guennoun, M., Chouqar, J., Jehin, E., Rinner, C., Lloyd, J., El Moutamid, Maryame, Lamarche, C., Pollock, J.T., caton, D.B., Kouprianov, Vladimir, Timerson, B.W., Blanchard, G., Payet, B., Peyrot, A., Teng-Chuen-Yu, J.-P., Françoise, J., Mondon, Bernard, Payet, Thierry, Boissel, C., Castets, M., Hubbard, William, Hill, R., Reitsema, H. J., Mousis, Olivier, Ball, L., Neilsen, G., Hutcheon, S., lay, K., Anderson, P., Moy, M., Jonsen, M., Pink, I., Walters, R., and Downs, B.
Abstract: Context. A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. Aims. We aimed at constraining Triton's atmospheric structure and the seasonal variations of its atmospheric pressure since the Voyager 2 epoch (1989). We also derived the shape of the lower atmosphere from central flash analysis. Methods. We used Abel inversions and direct ray-tracing code to provide the density, pressure, and temperature profiles in the altitude range similar to 8 km to similar to 190 km, corresponding to pressure levels from 9 mu bar down to a few nanobars. Results. (i) A pressure of 1.18 +/- 0.03 mu bar is found at a reference radius of 1400 km (47 km altitude). (ii) A new analysis of the Voyager 2 radio science occultation shows that this is consistent with an extrapolation of pressure down to the surface pressure obtained in 1989. (iii) A survey of occultations obtained between 1989 and 2017 suggests that an enhancement in surface pressure as reported during the 1990s might be real, but debatable, due to very few high S/N light curves and data accessible for reanalysis. The volatile transport model analysed supports a moderate increase in surface pressure, with a maximum value around 2005-2015 no higher than 23 mu bar. The pressures observed in 1995-1997 and 2017 appear mutually inconsistent with the volatile transport model presented here. (iv) The central flash structure does not show evidence of an atmospheric distortion. We find an upper limit of 0.0011 for the apparent oblateness of the atmosphere near the 8 km altitude.
Published: 2022

4. Constraints on the structure and seasonal variations of Triton’s atmosphere from the 5 October 2017 stellar occultation and previous observations

Author: Marques Oliveira, J., primary, Sicardy, B., additional, Gomes-Júnior, A. R., additional, Ortiz, J. L., additional, Strobel, D. F., additional, Bertrand, T., additional, Forget, F., additional, Lellouch, E., additional, Desmars, J., additional, Bérard, D., additional, Doressoundiram, A., additional, Lecacheux, J., additional, Leiva, R., additional, Meza, E., additional, Roques, F., additional, Souami, D., additional, Widemann, T., additional, Santos-Sanz, P., additional, Morales, N., additional, Duffard, R., additional, Fernández-Valenzuela, E., additional, Castro-Tirado, A. J., additional, Braga-Ribas, F., additional, Morgado, B. E., additional, Assafin, M., additional, Camargo, J. I. B., additional, Vieira-Martins, R., additional, Benedetti-Rossi, G., additional, Santos-Filho, S., additional, Banda-Huarca, M. V., additional, Quispe-Huaynasi, F., additional, Pereira, C. L., additional, Rommel, F. L., additional, Margoti, G., additional, Dias-Oliveira, A., additional, Colas, F., additional, Berthier, J., additional, Renner, S., additional, Hueso, R., additional, Pérez-Hoyos, S., additional, Sánchez-Lavega, A., additional, Rojas, J. F., additional, Beisker, W., additional, Kretlow, M., additional, Herald, D., additional, Gault, D., additional, Bath, K.-L., additional, Bode, H.-J., additional, Bredner, E., additional, Guhl, K., additional, Haymes, T. V., additional, Hummel, E., additional, Kattentidt, B., additional, Klös, O., additional, Pratt, A., additional, Thome, B., additional, Avdellidou, C., additional, Gazeas, K., additional, Karampotsiou, E., additional, Tzouganatos, L., additional, Kardasis, E., additional, Christou, A. A., additional, Xilouris, E. M., additional, Alikakos, I., additional, Gourzelas, A., additional, Liakos, A., additional, Charmandaris, V., additional, Jelínek, M., additional, Štrobl, J., additional, Eberle, A., additional, Rapp, K., additional, Gährken, B., additional, Klemt, B., additional, Kowollik, S., additional, Bitzer, R., additional, Miller, M., additional, Herzogenrath, G., additional, Frangenberg, D., additional, Brandis, L., additional, Pütz, I., additional, Perdelwitz, V., additional, Piehler, G. M., additional, Riepe, P., additional, von Poschinger, K., additional, Baruffetti, P., additional, Cenadelli, D., additional, Christille, J.-M., additional, Ciabattari, F., additional, Di Luca, R., additional, Alboresi, D., additional, Leto, G., additional, Zanmar Sanchez, R., additional, Bruno, P., additional, Occhipinti, G., additional, Morrone, L., additional, Cupolino, L., additional, Noschese, A., additional, Vecchione, A., additional, Scalia, C., additional, Lo Savio, R., additional, Giardina, G., additional, Kamoun, S., additional, Barbosa, R., additional, Behrend, R., additional, Spano, M., additional, Bouchet, E., additional, Cottier, M., additional, Falco, L., additional, Gallego, S., additional, Tortorelli, L., additional, Sposetti, S., additional, Sussenbach, J., additional, Van Den Abbeel, F., additional, André, P., additional, Llibre, M., additional, Pailler, F., additional, Ardissone, J., additional, Boutet, M., additional, Sanchez, J., additional, Bretton, M., additional, Cailleau, A., additional, Pic, V., additional, Granier, L., additional, Chauvet, R., additional, Conjat, M., additional, Dauvergne, J. L., additional, Dechambre, O., additional, Delay, P., additional, Delcroix, M., additional, Rousselot, L., additional, Ferreira, J., additional, Machado, P., additional, Tanga, P., additional, Rivet, J.-P., additional, Frappa, E., additional, Irzyk, M., additional, Jabet, F., additional, Kaschinski, M., additional, Klotz, A., additional, Rieugnie, Y., additional, Klotz, A. N., additional, Labrevoir, O., additional, Lavandier, D., additional, Walliang, D., additional, Leroy, A., additional, Bouley, S., additional, Lisciandra, S., additional, Coliac, J.-F., additional, Metz, F., additional, Erpelding, D., additional, Nougayrède, P., additional, Midavaine, T., additional, Miniou, M., additional, Moindrot, S., additional, Morel, P., additional, Reginato, B., additional, Reginato, E., additional, Rudelle, J., additional, Tregon, B., additional, Tanguy, R., additional, David, J., additional, Thuillot, W., additional, Hestroffer, D., additional, Vaudescal, G., additional, Baba Aissa, D., additional, Grigahcene, Z., additional, Briggs, D., additional, Broadbent, S., additional, Denyer, P., additional, Haigh, N. J., additional, Quinn, N., additional, Thurston, G., additional, Fossey, S. J., additional, Arena, C., additional, Jennings, M., additional, Talbot, J., additional, Alonso, S., additional, Román Reche, A., additional, Casanova, V., additional, Briggs, E., additional, Iglesias-Marzoa, R., additional, Abril Ibáñez, J., additional, Díaz Martín, M. C., additional, González, H., additional, Maestre García, J. L., additional, Marchant, J., additional, Ordonez-Etxeberria, I., additional, Martorell, P., additional, Salamero, J., additional, Organero, F., additional, Ana, L., additional, Fonseca, F., additional, Peris, V., additional, Brevia, O., additional, Selva, A., additional, Perello, C., additional, Cabedo, V., additional, Gonçalves, R., additional, Ferreira, M., additional, Marques Dias, F., additional, Daassou, A., additional, Barkaoui, K., additional, Benkhaldoun, Z., additional, Guennoun, M., additional, Chouqar, J., additional, Jehin, E., additional, Rinner, C., additional, Lloyd, J., additional, El Moutamid, M., additional, Lamarche, C., additional, Pollock, J. T., additional, Caton, D. B., additional, Kouprianov, V., additional, Timerson, B. W., additional, Blanchard, G., additional, Payet, B., additional, Peyrot, A., additional, Teng-Chuen-Yu, J.-P., additional, Françoise, J., additional, Mondon, B., additional, Payet, T., additional, Boissel, C., additional, Castets, M., additional, Hubbard, W. B., additional, Hill, R., additional, Reitsema, H. J., additional, Mousis, O., additional, Ball, L., additional, Neilsen, G., additional, Hutcheon, S., additional, Lay, K., additional, Anderson, P., additional, Moy, M., additional, Jonsen, M., additional, Pink, I., additional, Walters, R., additional, and Downs, B., additional
Published: 2022
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5. Observed tidal evolution of Kleopatra’s outer satellite

Author: Brož, M., primary, Ďurech, J., additional, Carry, B., additional, Vachier, F., additional, Marchis, F., additional, Hanuš, J., additional, Jorda, L., additional, Vernazza, P., additional, Vokrouhlický, D., additional, Walterová, M., additional, and Behrend, R., additional
Published: 2022
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6. Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Author: Marciniak, A., primary, Ďurech, J., additional, Alí-Lagoa, V., additional, Ogłoza, W., additional, Szakáts, R., additional, Müller, T. G., additional, Molnár, L., additional, Pál, A., additional, Monteiro, F., additional, Arcoverde, P., additional, Behrend, R., additional, Benkhaldoun, Z., additional, Bernasconi, L., additional, Bosch, J., additional, Brincat, S., additional, Brunetto, L., additional, Butkiewicz - Bąk, M., additional, Del Freo, F., additional, Duffard, R., additional, Evangelista-Santana, M., additional, Farroni, G., additional, Fauvaud, S., additional, Fauvaud, M., additional, Ferrais, M., additional, Geier, S., additional, Golonka, J., additional, Grice, J., additional, Hirsch, R., additional, Horbowicz, J., additional, Jehin, E., additional, Julien, P., additional, Kalup, Cs., additional, Kamiński, K., additional, Kamińska, M. K., additional, Kankiewicz, P., additional, Kecskeméthy, V., additional, Kim, D.-H., additional, Kim, M.-J., additional, Konstanciak, I., additional, Krajewski, J., additional, Kudak, V., additional, Kulczak, P., additional, Kundera, T., additional, Lazzaro, D., additional, Manzini, F., additional, Medeiros, H., additional, Michimani-Garcia, J., additional, Morales, N., additional, Nadolny, J., additional, Oszkiewicz, D., additional, Pakštienė, E., additional, Pawłowski, M., additional, Perig, V., additional, Pilcher, F., additional, Pinel, P., additional, Podlewska-Gaca, E., additional, Polakis, T., additional, Richard, F., additional, Rodrigues, T., additional, Rondón, E., additional, Roy, R., additional, Sanabria, J. J., additional, Santana-Ros, T., additional, Skiff, B., additional, Skrzypek, J., additional, Sobkowiak, K., additional, Sonbas, E., additional, Stachowski, G., additional, Strajnic, J., additional, Trela, P., additional, Tychoniec, Ł., additional, Urakawa, S., additional, Verebelyi, E., additional, Wagrez, K., additional, Żejmo, M., additional, and Żukowski, K., additional
Published: 2021
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7. VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis

Author: Vernazza, P., primary, Ferrais, M., additional, Jorda, L., additional, Hanuš, J., additional, Carry, B., additional, Marsset, M., additional, Brož, M., additional, Fetick, R., additional, Viikinkoski, M., additional, Marchis, F., additional, Vachier, F., additional, Drouard, A., additional, Fusco, T., additional, Birlan, M., additional, Podlewska-Gaca, E., additional, Rambaux, N., additional, Neveu, M., additional, Bartczak, P., additional, Dudziński, G., additional, Jehin, E., additional, Beck, P., additional, Berthier, J., additional, Castillo-Rogez, J., additional, Cipriani, F., additional, Colas, F., additional, Dumas, C., additional, Ďurech, J., additional, Grice, J., additional, Kaasalainen, M., additional, Kryszczynska, A., additional, Lamy, P., additional, Le Coroller, H., additional, Marciniak, A., additional, Michalowski, T., additional, Michel, P., additional, Santana-Ros, T., additional, Tanga, P., additional, Vigan, A., additional, Witasse, O., additional, Yang, B., additional, Antonini, P., additional, Audejean, M., additional, Aurard, P., additional, Behrend, R., additional, Benkhaldoun, Z., additional, Bosch, J. M., additional, Chapman, A., additional, Dalmon, L., additional, Fauvaud, S., additional, Hamanowa, Hiroko, additional, Hamanowa, Hiromi, additional, His, J., additional, Jones, A., additional, Kim, D.-H., additional, Kim, M.-J., additional, Krajewski, J., additional, Labrevoir, O., additional, Leroy, A., additional, Livet, F., additional, Molina, D., additional, Montaigut, R., additional, Oey, J., additional, Payre, N., additional, Reddy, V., additional, Sabin, P., additional, Sanchez, A. G., additional, and Socha, L., additional
Published: 2021
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8. Evidence for differentiation of the most primitive small bodies

Author: Carry, B., primary, Vernazza, P., additional, Vachier, F., additional, Neveu, M., additional, Berthier, J., additional, Hanuš, J., additional, Ferrais, M., additional, Jorda, L., additional, Marsset, M., additional, Viikinkoski, M., additional, Bartczak, P., additional, Behrend, R., additional, Benkhaldoun, Z., additional, Birlan, M., additional, Castillo-Rogez, J., additional, Cipriani, F., additional, Colas, F., additional, Drouard, A., additional, Dudziński, G. P., additional, Desmars, J., additional, Dumas, C., additional, Ďurech, J., additional, Fetick, R., additional, Fusco, T., additional, Grice, J., additional, Jehin, E., additional, Kaasalainen, M., additional, Kryszczynska, A., additional, Lamy, P., additional, Marchis, F., additional, Marciniak, A., additional, Michalowski, T., additional, Michel, P., additional, Pajuelo, M., additional, Podlewska-Gaca, E., additional, Rambaux, N., additional, Santana-Ros, T., additional, Storrs, A., additional, Tanga, P., additional, Vigan, A., additional, Warner, B., additional, Wieczorek, M., additional, Witasse, O., additional, and Yang, B., additional
Published: 2021
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9. (704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body

Author: Dudziński, G., Podlewska-Gaca, E., Bartczak, P., Benseguane, S, Ferrais, M., Jorda, L., Hanuš, J., Vernazza, P., Rambaux, N., Carry, B., Marchis, F., Marsset, M., Viikinkoski, M., Brož, M., Fetick, R., Drouard, A., Fusco, T., Birlan, M., Jehin, E., Berthier, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Dumas, C., Kryszczynska, A., Lamy, P., Le Coroller, H, Marciniak, A., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vachier, F., Vigan, A., Witasse, O., Yang, Bin, Ďurech, J., Kaasalainen, M., Le Coroller, H., Ševeček, P., Dudzinski, G., DeMeo, F., Durech, J., Grice, J., Gillon, M., Benkhaldoun, Z., Szakats, R., Hirsch, R., Duffard, R., Chapman, A., Maestre, J., Carbognani, Albino, Barghini, D., Gardiol, D., Martino, M. Di, Valsecchi, G., Trivero, P., Buzzoni, A., Rasetti, S., Selvestrel, D., Knapic, C., Londero, E., Zorba, S., Volpicelli, C., Carlo, M. Di, Vaubaillon, J., Marmo, C., Valeri, D., Zanotti, F., Morini, M., Demaria, P., Zanda, B., Bouley, S., Rault, J., Maquet, L., Warner, B., Behrend, R., Asenjo, V., Berger, N., Bronikowska, M., Brothers, T., Charbonnel, S., Colazo, C., Coliac, J.-F., Jones, A., Leroy, A., Melia, R., Molina, D., Nadolny, J., Person, M., Pejcha, O., Riemis, H., Shappee, B., Sobkowiak, K., Soldán, F., Suys, D., Vantomme, J., Ministry of Education, Youth and Sports (Czech Republic), European Commission, National Aeronautics and Space Administration (US), National Centre for Research and Development (Poland), National Research, Development and Innovation Office (Hungary), Hungarian Academy of Sciences, Université de Liège, Centre National de la Recherche Scientifique (France), Gordon and Betty Moore Foundation, National Science Foundation (US), The Ohio State University, Chinese Academy of Sciences, Villum Fonden, Astronomical Institute of Charles University, Charles University [Prague], Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Tampere University of Technology [Tampere] (TUT), Space Sciences, Technologies and Astrophysics Research Institute (STAR), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Adam Mickiewicz University in Poznań (UAM), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), European Southern Observatory (ESO), European Space Astronomy Centre (ESAC), European Space Agency (ESA), Astrophysics Research Centre [Belfast] (ARC), Queen's University [Belfast] (QUB), Geneva Observatory, University of Geneva [Switzerland], Asociación Astronómica Astro Henares, Centro de Recursos Asociativos El Cerro, Institute of Geology [Poznan], Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS), Massachusetts Institute of Technology (MIT), Association T60, Observatoire Midi-Pyrénées, Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées, Observatorio Astronómico de Córdoba (OAC), Universidad Nacional de Córdoba [Argentina], Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Spain] (CSIC), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Departamento de Astrofísica [La laguna], Universidad de La Laguna [Tenerife - SP] (ULL), Department of Geological Sciences [Bloomington], Indiana University [Bloomington], Indiana University System-Indiana University System, Institute for Astronomy [Honolulu], University of Hawai‘i [Mānoa] (UHM), Astronomical Observatory [Poznan], Observatorio Amanecer de Arrakis, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences [Budapest], Hungarian Academy of Sciences (MTA)-Hungarian Academy of Sciences (MTA), Laboratoire associé de Reconnaissance cellulaire et amélioration des plantes, Institut National de la Recherche Agronomique (INRA), Jet Propulsion Laboratory (JPL), California Institute of Technology (CALTECH)-NASA, European Space Research and Technology Centre (ESTEC), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA), Department of Mathematics [Tampere], Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Northeastern University [Shenyang], Charles University [Prague] (CU), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), SETI Institute, Center for Solar System Studies (CS3), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), Observatoire de Durtal, Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), L'Uranoscope de l'Ile de France, Observatoire de Gretz-Armainvilliers, Anunaki Observatory, Thirty Meter Telescope Observatory, NASA-California Institute of Technology (CALTECH), Agence Spatiale Européenne = European Space Agency (ESA), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA), Departamento de Fisica, Ingenieria de Sistemas y Teoria de la Señal [Alicante] (DFESTS), Universidad de Alicante, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), European Southern Observatory [Santiago] (ESO), Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Genève (UNIGE), and Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: asteroids, 010504 meteorology & atmospheric sciences, Dwarf planet, Irregular shape, Minor (linear algebra), FOS: Physical sciences, Astrophysics, 01 natural sciences, 7. Clean energy, law.invention, Techniques: high angular resolution, photometric, Impact crater, Methods: observational, law, Física Aplicada, 0103 physical sciences, high angular resolutiontechniques, observational [Methods], individual, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences, (704) Interamnia -methods, Earth and Planetary Astrophysics (astro-ph.EP), Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Interamnia, photometric [Techniques], observational -techniques, Minor planets, Astronomy and Astrophysics, individual: (704) [Asteroids], Ellipsoid, high angular resolution [Techniques], Space and Planetary Science, Asteroid, [SDU]Sciences of the Universe [physics], individual: (704) Interamnia [Minor planets, asteroids], Stellar occultation, Asteroids: individual: (704), Hydrostatic equilibrium, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Techniques: photometric, Astrophysics - Earth and Planetary Astrophysics
Abstract: Full list of authors: 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., With an estimated diameter in the 320 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largest bodies with D >400 km (Ceres, Vesta, Pallas and Hygiea) and the numerous smaller bodies with diameter 200 km. However, despite its large size, little is known about the shape and spin state of Interamnia and, therefore, about its bulk composition and past collisional evolution. Aims. We aimed to test at what size and mass the shape of a small body departs from a nearly ellipsoidal equilibrium shape (as observed in the case of the four largest asteroids) to an irregular shape as routinely observed in the case of smaller (D 200 km) bodies. Methods. We observed Interamnia as part of our ESO VLT/SPHERE large program (ID: 199.C-0074) at thirteen different epochs. In addition, several new optical lightcurves were recorded. These data, along with stellar occultation data from the literature, were fed to the All-Data Asteroid Modeling algorithm to reconstruct the 3D-shape model of Interamnia and to determine its spin state. Results. Interamnia s volume-equivalent diameter of 332 6 km implies a bulk density of = 1.98 0.68 g cm3, which suggests that Interamnia like Ceres and Hygiea contains a high fraction of water ice, consistent with the paucity of apparent craters. Our observations reveal a shape that can be well approximated by an ellipsoid, and that is compatible with a fluid hydrostatic equilibrium at the 2 level. Conclusions. The rather regular shape of Interamnia implies that the size and mass limit, under which the shapes of minor bodies with a high amount of water ice in the subsurface become irregular, has to be searched among smaller (D 300 km) less massive (m 3 1019 kg) bodies. © 2020 EDP Sciences. All rights reserved., This work has been supported by the Czech Science Foundation through grant 18-09470S (J.H., J.D.) and by the Charles University Research program No. UNCE/SCI/023. This research was supported by INTER-EXCELLENCE grant LTAUSA18093 from the Czech Ministry of Education, Youth, and Sports (J.H. and O.P.). The research of O.P. is additionally supported by Horizon 2020 ERC Starting Grant "Cat-In-hAT" (grant agreement #803158) and award PRIMUS/SCI/17 from Charles University. P.V., A.D., and B.C. were supported by CNRS/INSU/PNP. M.M. was supported by the National Aeronautics and Space Administration under Grant No. 80NSSC18K0849 issued through the Planetary Astronomy Program. This work was supported by the National Science Centre, Poland, through grant no. 2014/13/D/ST9/01818 (A.M.). The research leading to these results has received funding from the European Union's Horizon 2020 Research and Innovation Programme, under Grant Agreement no 687378 (SBNAF). This project has been supported by the GINOP-2.3.2-15-2016-00003 and NKFIH K125015 grants of the Hungarian National Research, Development and Innovation Office (NKFIH) and by the Lendulet grant LP2012-31 of the Hungarian Academy of Sciences. TRAPPIST-North is a project funded by the University of Liege, in collaboration with Cadi Ayyad University of Marrakech (Morocco). TRAPPIST-South is a project funded by the Belgian FNRS under grant FRFC 2.5.594.09. F.E.J. is a FNRS Senior Research Associate. ASAS-SN thanks the Las Cumbres Observatory and its staff for its continuing support of the ASAS-SN project. ASAS-SN is supported by the Gordon and Betty Moore Foundation through grant GBMF5490 to the Ohio State University and NSF grant AST-1515927. Development of ASAS-SN has been supported by NSF grant AST-0908816, the Mt. Cuba Astronomical Foundation, the Center for Cosmology and AstroParticle Physics at the Ohio State University, the Chinese Academy of Sciences South America Center for Astronomy (CASSACA), the Villum Foundation, and George Skestos.
Published: 2020

10. Physical parameters of selected Gaia mass asteroids

Author: European Commission, National Aeronautics and Space Administration (US), Hungarian Academy of Sciences, Hungarian Scientific Research Fund, Fonds de la Recherche Scientifique (Fédération Wallonie-Bruxelles), Université de Liège, Generalitat Valenciana, Université Cadi Ayyad, Podlewska-Gaca, E., Marciniak, A., Ali-Lagoa, Victor, Bartczak, P., Müller, T.G., Szakáts, R., Duffard, René D., 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, Nicolás, Parley, N., Poncy, R., Roy, R., Santana-Ros, Toni, Seli, B., Sobkowiak, K., Verebélyi, E., Żukowski, K., European Commission, National Aeronautics and Space Administration (US), Hungarian Academy of Sciences, Hungarian Scientific Research Fund, Fonds de la Recherche Scientifique (Fédération Wallonie-Bruxelles), Université de Liège, Generalitat Valenciana, Université Cadi Ayyad, Podlewska-Gaca, E., Marciniak, A., Ali-Lagoa, Victor, Bartczak, P., Müller, T.G., Szakáts, R., Duffard, René D., 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, Nicolás, Parley, N., Poncy, R., Roy, R., Santana-Ros, Toni, Seli, B., Sobkowiak, K., Verebélyi, E., and Żukowski, K.
Abstract: 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 volume and hence their density. However, some of those diameters are still based on simple thermal models, which can occasionally lead to volume uncertainties as high as 20-30%. Aims. The aim of this paper is to determine the 3D shape models and compute the volumes for 13 main belt asteroids that were selected from those targets for which Gaia will provide the mass with an accuracy of better than 10%. Methods. We used the genetic Shaping Asteroids with Genetic Evolution (SAGE) algorithm to fit disk-integrated, dense photometric lightcurves and obtain detailed asteroid shape models. These models were scaled by fitting them to available stellar occultation and/or thermal infrared observations. Results. We determine the spin and shape models for 13 main belt asteroids using the SAGE algorithm. Occultation fitting enables us to confirm main shape features and the spin state, while thermophysical modeling leads to more precise diameters as well as estimates of thermal inertia values. Conclusions. We calculated the volume of our sample of main-belt asteroids for which the Gaia satellite will provide precise mass determinations. From our volumes, it will then be possible to more accurately compute the bulk density, which is a fundamental physical property needed to understand the formation and evolution processes of small Solar System bodies. © ESO 2020.
Published: 2020

11. FRIPON: a worldwide network to track incoming meteoroids

Author: Colas, F., primary, Zanda, B., additional, Bouley, S., additional, Jeanne, S., additional, Malgoyre, A., additional, Birlan, M., additional, Blanpain, C., additional, Gattacceca, J., additional, Jorda, L., additional, Lecubin, J., additional, Marmo, C., additional, Rault, J. L., additional, Vaubaillon, J., additional, Vernazza, P., additional, Yohia, C., additional, Gardiol, D., additional, Nedelcu, A., additional, Poppe, B., additional, Rowe, J., additional, Forcier, M., additional, Koschny, D., additional, Trigo-Rodriguez, J. M., additional, Lamy, H., additional, Behrend, R., additional, Ferrière, L., additional, Barghini, D., additional, Buzzoni, A., additional, Carbognani, A., additional, Di Carlo, M., additional, Di Martino, M., additional, Knapic, C., additional, Londero, E., additional, Pratesi, G., additional, Rasetti, S., additional, Riva, W., additional, Stirpe, G. M., additional, Valsecchi, G. B., additional, Volpicelli, C. A., additional, Zorba, S., additional, Coward, D., additional, Drolshagen, E., additional, Drolshagen, G., additional, Hernandez, O., additional, Jehin, E., additional, Jobin, M., additional, King, A., additional, Nitschelm, C., additional, Ott, T., additional, Sanchez-Lavega, A., additional, Toni, A., additional, Abraham, P., additional, Affaticati, F., additional, Albani, M., additional, Andreis, A., additional, Andrieu, T., additional, Anghel, S., additional, Antaluca, E., additional, Antier, K., additional, Appéré, T., additional, Armand, A., additional, Ascione, G., additional, Audureau, Y., additional, Auxepaules, G., additional, Avoscan, T., additional, Baba Aissa, D., additional, Bacci, P., additional, Bǎdescu, O., additional, Baldini, R., additional, Baldo, R., additional, Balestrero, A., additional, Baratoux, D., additional, Barbotin, E., additional, Bardy, M., additional, Basso, S., additional, Bautista, O., additional, Bayle, L. D., additional, Beck, P., additional, Bellitto, R., additional, Belluso, R., additional, Benna, C., additional, Benammi, M., additional, Beneteau, E., additional, Benkhaldoun, Z., additional, Bergamini, P., additional, Bernardi, F., additional, Bertaina, M. E., additional, Bessin, P., additional, Betti, L., additional, Bettonvil, F., additional, Bihel, D., additional, Birnbaum, C., additional, Blagoi, O., additional, Blouri, E., additional, Boacă, I., additional, Boatǎ, R., additional, Bobiet, B., additional, Bonino, R., additional, Boros, K., additional, Bouchet, E., additional, Borgeot, V., additional, Bouchez, E., additional, Boust, D., additional, Boudon, V., additional, Bouman, T., additional, Bourget, P., additional, Brandenburg, S., additional, Bramond, Ph., additional, Braun, E., additional, Bussi, A., additional, Cacault, P., additional, Caillier, B., additional, Calegaro, A., additional, Camargo, J., additional, Caminade, S., additional, Campana, A. P. C., additional, Campbell-Burns, P., additional, Canal-Domingo, R., additional, Carell, O., additional, Carreau, S., additional, Cascone, E., additional, Cattaneo, C., additional, Cauhape, P., additional, Cavier, P., additional, Celestin, S., additional, Cellino, A., additional, Champenois, M., additional, Chennaoui Aoudjehane, H., additional, Chevrier, S., additional, Cholvy, P., additional, Chomier, L., additional, Christou, A., additional, Cricchio, D., additional, Coadou, P., additional, Cocaign, J. Y., additional, Cochard, F., additional, Cointin, S., additional, Colombi, E., additional, Colque Saavedra, J. P., additional, Corp, L., additional, Costa, M., additional, Costard, F., additional, Cottier, M., additional, Cournoyer, P., additional, Coustal, E., additional, Cremonese, G., additional, Cristea, O., additional, Cuzon, J. C., additional, D’Agostino, G., additional, Daiffallah, K., additional, Dǎnescu, C., additional, Dardon, A., additional, Dasse, T., additional, Davadan, C., additional, Debs, V., additional, Defaix, J. P., additional, Deleflie, F., additional, D’Elia, M., additional, De Luca, P., additional, De Maria, P., additional, Deverchère, P., additional, Devillepoix, H., additional, Dias, A., additional, Di Dato, A., additional, Di Luca, R., additional, Dominici, F. M., additional, Drouard, A., additional, Dumont, J. L., additional, Dupouy, P., additional, Duvignac, L., additional, Egal, A., additional, Erasmus, N., additional, Esseiva, N., additional, Ebel, A., additional, Eisengarten, B., additional, Federici, F., additional, Feral, S., additional, Ferrant, G., additional, Ferreol, E., additional, Finitzer, P., additional, Foucault, A., additional, Francois, P., additional, Frîncu, M., additional, Froger, J. L., additional, Gaborit, F., additional, Gagliarducci, V., additional, Galard, J., additional, Gardavot, A., additional, Garmier, M., additional, Garnung, M., additional, Gautier, B., additional, Gendre, B., additional, Gerard, D., additional, Gerardi, A., additional, Godet, J. P., additional, Grandchamps, A., additional, Grouiez, B., additional, Groult, S., additional, Guidetti, D., additional, Giuli, G., additional, Hello, Y., additional, Henry, X., additional, Herbreteau, G., additional, Herpin, M., additional, Hewins, P., additional, Hillairet, J. J., additional, Horak, J., additional, Hueso, R., additional, Huet, E., additional, Huet, S., additional, Hyaumé, F., additional, Interrante, G., additional, Isselin, Y., additional, Jeangeorges, Y., additional, Janeux, P., additional, Jeanneret, P., additional, Jobse, K., additional, Jouin, S., additional, Jouvard, J. M., additional, Joy, K., additional, Julien, J. F., additional, Kacerek, R., additional, Kaire, M., additional, Kempf, M., additional, Krier, C., additional, Kwon, M. K., additional, Lacassagne, L., additional, Lachat, D., additional, Lagain, A., additional, Laisné, E., additional, Lanchares, V., additional, Laskar, J., additional, Lazzarin, M., additional, Leblanc, M., additional, Lebreton, J. P., additional, Lecomte, J., additional, Le Dû, P., additional, Lelong, F., additional, Lera, S., additional, Leoni, J. F., additional, Le-Pichon, A., additional, Le-Poupon, P., additional, Leroy, A., additional, Leto, G., additional, Levansuu, A., additional, Lewin, E., additional, Lienard, A., additional, Licchelli, D., additional, Locatelli, H., additional, Loehle, S., additional, Loizeau, D., additional, Luciani, L., additional, Maignan, M., additional, Manca, F., additional, Mancuso, S., additional, Mandon, E., additional, Mangold, N., additional, Mannucci, F., additional, Maquet, L., additional, Marant, D., additional, Marchal, Y., additional, Marin, J. L., additional, Martin-Brisset, J. C., additional, Martin, D., additional, Mathieu, D., additional, Maury, A., additional, Mespoulet, N., additional, Meyer, F., additional, Meyer, J. Y., additional, Meza, E., additional, Moggi Cecchi, V., additional, Moiroud, J. J., additional, Millan, M., additional, Montesarchio, M., additional, Misiano, A., additional, Molinari, E., additional, Molau, S., additional, Monari, J., additional, Monflier, B., additional, Monkos, A., additional, Montemaggi, M., additional, Monti, G., additional, Moreau, R., additional, Morin, J., additional, Mourgues, R., additional, Mousis, O., additional, Nablanc, C., additional, Nastasi, A., additional, Niacşu, L., additional, Notez, P., additional, Ory, M., additional, Pace, E., additional, Paganelli, M. A., additional, Pagola, A., additional, Pajuelo, M., additional, Palacián, J. F., additional, Pallier, G., additional, Paraschiv, P., additional, Pardini, R., additional, Pavone, M., additional, Pavy, G., additional, Payen, G., additional, Pegoraro, A., additional, Peña-Asensio, E., additional, Perez, L., additional, Pérez-Hoyos, S., additional, Perlerin, V., additional, Peyrot, A., additional, Peth, F., additional, Pic, V., additional, Pietronave, S., additional, Pilger, C., additional, Piquel, M., additional, Pisanu, T., additional, Poppe, M., additional, Portois, L., additional, Prezeau, J. F., additional, Pugno, N., additional, Quantin, C., additional, Quitté, G., additional, Rambaux, N., additional, Ravier, E., additional, Repetti, U., additional, Ribas, S., additional, Richard, C., additional, Richard, D., additional, Rigoni, M., additional, Rivet, J. P., additional, Rizzi, N., additional, Rochain, S., additional, Rojas, J.F., additional, Romeo, M., additional, Rotaru, M., additional, Rotger, M., additional, Rougier, P., additional, Rousselot, P., additional, Rousset, J., additional, Rousseu, D., additional, Rubiera, O., additional, Rudawska, R., additional, Rudelle, J., additional, Ruguet, J.P., additional, Russo, P., additional, Sales, S., additional, Sauzereau, O., additional, Salvati, F., additional, Schieffer, M., additional, Schreiner, D., additional, Scribano, Y., additional, Selvestrel, D., additional, Serra, R., additional, Shengold, L., additional, Shuttleworth, A., additional, Smareglia, R., additional, Sohy, S., additional, Soldi, M., additional, Stanga, R., additional, Steinhausser, A., additional, Strafella, F., additional, Sylla Mbaye, S., additional, Smedley, A. R. D., additional, Tagger, M., additional, Tanga, P., additional, Taricco, C., additional, Teng, J. P., additional, Tercu, J. O., additional, Thizy, O., additional, Thomas, J. P., additional, Tombelli, M., additional, Trangosi, R., additional, Tregon, B., additional, Trivero, P., additional, Tukkers, A., additional, Turcu, V., additional, Umbriaco, G., additional, Unda-Sanzana, E., additional, Vairetti, R., additional, Valenzuela, M., additional, Valente, G., additional, Varennes, G., additional, Vauclair, S., additional, Vergne, J., additional, Verlinden, M., additional, Vidal-Alaiz, M., additional, Vieira-Martins, R., additional, Viel, A., additional, Vîntdevarǎ, D. C., additional, Vinogradoff, V., additional, Volpini, P., additional, Wendling, M., additional, Wilhelm, P., additional, Wohlgemuth, K., additional, Yanguas, P., additional, Zagarella, R., additional, and Zollo, A., additional
Published: 2020
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12. The large trans-Neptunian object 2002 TC302from combined stellar occultation, photometry, and astrometry data

Author: Ortiz, J. L., primary, Santos-Sanz, P., additional, Sicardy, B., additional, Benedetti-Rossi, G., additional, Duffard, R., additional, Morales, N., additional, Braga-Ribas, F., additional, Fernández-Valenzuela, E., additional, Nascimbeni, V., additional, Nardiello, D., additional, Carbognani, A., additional, Buzzi, L., additional, Aletti, A., additional, Bacci, P., additional, Maestripieri, M., additional, Mazzei, L., additional, Mikuz, H., additional, Skvarc, J., additional, Ciabattari, F., additional, Lavalade, F., additional, Scarfi, G., additional, Mari, J. M., additional, Conjat, M., additional, Sposetti, S., additional, Bachini, M., additional, Succi, G., additional, Mancini, F., additional, Alighieri, M., additional, Dal Canto, E., additional, Masucci, M., additional, Vara-Lubiano, M., additional, Gutiérrez, P. J., additional, Desmars, J., additional, Lecacheux, J., additional, Vieira-Martins, R., additional, Camargo, J. I. B., additional, Assafin, M., additional, Colas, F., additional, Beisker, W., additional, Behrend, R., additional, Mueller, T. G., additional, Meza, E., additional, Gomes-Junior, A. R., additional, Roques, F., additional, Vachier, F., additional, Mottola, S., additional, Hellmich, S., additional, Campo Bagatin, A., additional, Alvarez-Candal, A., additional, Cikota, S., additional, Cikota, A., additional, Christille, J. M., additional, Pál, A., additional, Kiss, C., additional, Pribulla, T., additional, Komžík, R., additional, Madiedo, J. M., additional, Charmandaris, V., additional, Alikakos, J., additional, Szakáts, R., additional, Farkas-Takács, A., additional, Varga-Verebélyi, E., additional, Marton, G., additional, Marciniak, A., additional, Bartczak, P., additional, Butkiewicz-Ba̧k, M., additional, Dudziński, G., additional, Alí-Lagoa, V., additional, Gazeas, K., additional, Paschalis, N., additional, Tsamis, V., additional, Guirado, J. C., additional, Peris, V., additional, Iglesias-Marzoa, R., additional, Schnabel, C., additional, Manzano, F., additional, Navarro, A., additional, Perelló, C., additional, Vecchione, A., additional, Noschese, A., additional, and Morrone, L., additional
Published: 2020
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13. Physical parameters of selected Gaia mass asteroids

Author: Podlewska-Gaca, E., primary, Marciniak, A., additional, Alí-Lagoa, V., additional, Bartczak, P., additional, Müller, T. G., additional, Szakáts, R., additional, Duffard, R., additional, Molnár, L., additional, Pál, A., additional, Butkiewicz-Bąk, M., additional, Dudziński, G., additional, Dziadura, K., additional, Antonini, P., additional, Asenjo, V., additional, Audejean, M., additional, Benkhaldoun, Z., additional, Behrend, R., additional, Bernasconi, L., additional, Bosch, J. M., additional, Chapman, A., additional, Dintinjana, B., additional, Farkas, A., additional, Ferrais, M., additional, Geier, S., additional, Grice, J., additional, Hirsh, R., additional, Jacquinot, H., additional, Jehin, E., additional, Jones, A., additional, Molina, D., additional, Morales, N., additional, Parley, N., additional, Poncy, R., additional, Roy, R., additional, Santana-Ros, T., additional, Seli, B., additional, Sobkowiak, K., additional, Verebélyi, E., additional, and Żukowski, K., additional
Published: 2020
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14. (704) Interamnia: a transitional object between a dwarf planet and a typical irregular-shaped minor body

Author: Hanuš, J., primary, Vernazza, P., additional, Viikinkoski, M., additional, Ferrais, M., additional, Rambaux, N., additional, Podlewska-Gaca, E., additional, Drouard, A., additional, Jorda, L., additional, Jehin, E., additional, Carry, B., additional, Marsset, M., additional, Marchis, F., additional, Warner, B., additional, Behrend, R., additional, Asenjo, V., additional, Berger, N., additional, Bronikowska, M., additional, Brothers, T., additional, Charbonnel, S., additional, Colazo, C., additional, Coliac, J.-F., additional, Duffard, R., additional, Jones, A., additional, Leroy, A., additional, Marciniak, A., additional, Melia, R., additional, Molina, D., additional, Nadolny, J., additional, Person, M., additional, Pejcha, O., additional, Riemis, H., additional, Shappee, B., additional, Sobkowiak, K., additional, Soldán, F., additional, Suys, D., additional, Szakats, R., additional, Vantomme, J., additional, Birlan, M., additional, Berthier, J., additional, Bartczak, P., additional, Dumas, C., additional, Dudziński, G., additional, Ďurech, J., additional, Castillo-Rogez, J., additional, Cipriani, F., additional, Fetick, R., additional, Fusco, T., additional, Grice, J., additional, Kaasalainen, M., additional, Kryszczynska, A., additional, Lamy, P., additional, Michalowski, T., additional, Michel, P., additional, Santana-Ros, T., additional, Tanga, P., additional, Vachier, F., additional, Vigan, A., additional, Witasse, O., additional, and Yang, B., additional
Published: 2020
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15. Thermal properties of slowly rotating asteroids: results from a targeted survey

Author: National Science Centre (Poland), European Commission, Ministry of Education (Slovak Republic), Ministerio de Ciencia, Innovación y Universidades (España), Hungarian Academy of Sciences, Marciniak, A., Ali-Lagoa, Victor, Mueller, T.G., Szakáts, R., Molnár, L., Pal, A., Podlewska-Gaca, E., Parley, N., Antonini, P., Barbotin, E., Behrend, R., Bernasconi, L., Butkiewicz-Bąk, M., Crippa, R., Duffard, René D., Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S., Goncalves, R, Grice, J., Grzeskowiak, I, Hirsch, R., Horbowicz, J, Kaminski, 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, Ogloza, W, Oszkiewicz, D., Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R., Sanabria, JJ, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Zejmo, M, Zukowski, K, National Science Centre (Poland), European Commission, Ministry of Education (Slovak Republic), Ministerio de Ciencia, Innovación y Universidades (España), Hungarian Academy of Sciences, Marciniak, A., Ali-Lagoa, Victor, Mueller, T.G., Szakáts, R., Molnár, L., Pal, A., Podlewska-Gaca, E., Parley, N., Antonini, P., Barbotin, E., Behrend, R., Bernasconi, L., Butkiewicz-Bąk, M., Crippa, R., Duffard, René D., Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S., Goncalves, R, Grice, J., Grzeskowiak, I, Hirsch, R., Horbowicz, J, Kaminski, 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, Ogloza, W, Oszkiewicz, D., Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R., Sanabria, JJ, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Zejmo, M, and Zukowski, K
Abstract: Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the subsurface. However, thermal inertias have been determined mainly for fast rotators due to selection effects in the available photometry used to obtain shape models required for thermophysical modelling (TPM). Aims. Our aims are to mitigate these selection effects by producing shape models of slow rotators, to scale them and compute their thermal inertia with TPM, and to verify whether thermal inertia increases with the rotation period. Methods. To decrease the bias against slow rotators, we conducted a photometric observing campaign of main-belt asteroids with periods longer than 12 h, from multiple stations worldwide, adding in some cases data from WISE and Kepler space telescopes. For spin and shape reconstruction we used the lightcurve inversion method, and to derive thermal inertias we applied a thermophysical model to fit available infrared data from IRAS, AKARI, and WISE. Results. We present new models of 11 slow rotators that provide a good fit to the thermal data. In two cases, the TPM analysis showed a clear preference for one of the two possible mirror solutions. We derived the diameters and albedos of our targets in addition to their thermal inertias, which ranged between 3(-3)(+33) and 45(-30)(+60) Jm(-2) s(-1/2) K-1. Conclusions. Together with our previous work, we have analysed 16 slow rotators from our dense survey with sizes between 30 and 150 km. The current sample thermal inertias vary widely, which does not confirm the earlier suggestion that slower rotators have higher thermal inertias.© ESO 2019
Published: 2019

16. Pluto's ephemeris from ground-based stellar occultations (1988-2016)

Author: Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), Fundação de Amparo à Pesquisa do Estado do Rio Grande do Sul, Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (Brasil), European Research Council, Desmars, J., Meza, E., Sicardy, B., Assafin, M., Camargo, J.I.B., Braga-Ribas, F., Benedetti-Rossi, G., Dias-Oliveira, A., Morgado, B., Gomes-Júnior, A.R., Vieira-Martins, Roberto, Behrend, R., Ortiz, José Luis, Duffard, René D., Morales, Nicolás, Santos Sanz, Pablo, Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), Fundação de Amparo à Pesquisa do Estado do Rio Grande do Sul, Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (Brasil), European Research Council, Desmars, J., Meza, E., Sicardy, B., Assafin, M., Camargo, J.I.B., Braga-Ribas, F., Benedetti-Rossi, G., Dias-Oliveira, A., Morgado, B., Gomes-Júnior, A.R., Vieira-Martins, Roberto, Behrend, R., Ortiz, José Luis, Duffard, René D., Morales, Nicolás, and Santos Sanz, Pablo
Abstract: Context. From 1988 to 2016, several stellar occultations have been observed to characterise Pluto's atmosphere and its evolution. From each stellar occultation, an accurate astrometric position of Pluto at the observation epoch is derived. These positions mainly depend on the position of the occulted star and the precision of the timing. Aims. We present 19 Pluto's astrometric positions derived from occultations from 1988 to 2016. Using Gaia DR2 for the positions of the occulted stars, the accuracy of these positions is estimated at 2-10 mas, depending on the observation circumstances. From these astrometric positions, we derive an updated ephemeris of Pluto's system barycentre using the NIMA code. Methods. The astrometric positions were derived by fitting the light curves of the occultation by a model of Pluto's atmosphere. The fits provide the observed position of the centre for a reference star position. In most cases other publications provided the circumstances of the occultation such as the coordinates of the stations, timing, and impact parameter, i.e. the closest distance between the station and centre of the shadow. From these parameters, we used a procedure based on the Bessel method to derive an astrometric position. Results. We derive accurate Pluto's astrometric positions from 1988 to 2016. These positions are used to refine the orbit of Pluto'system barycentre providing an ephemeris, accurate to the milliarcsecond level, over the period 2000-2020, allowing for better predictions for future stellar occultations.© J. Desmars et al. 2019.
Published: 2019

17. Physical model of near-Earth asteroid (1917) Cuyo from ground-based optical and thermal-IR observations

Author: Rożek, A., primary, Lowry, S. C., additional, Rozitis, B., additional, Green, S. F., additional, Snodgrass, C., additional, Weissman, P. R., additional, Fitzsimmons, A., additional, Hicks, M. D., additional, Lawrence, K. J., additional, Duddy, S. R., additional, Wolters, S. D., additional, Roberts-Borsani, G., additional, Behrend, R., additional, and Manzini, F., additional
Published: 2019
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18. Thermal properties of slowly rotating asteroids: results from a targeted survey

Author: Marciniak, A., primary, Alí-Lagoa, V., additional, Müller, T. G., additional, Szakáts, R., additional, Molnár, L., additional, Pál, A., additional, Podlewska-Gaca, E., additional, Parley, N., additional, Antonini, P., additional, Barbotin, E., additional, Behrend, R., additional, Bernasconi, L., additional, Butkiewicz-Bąk, M., additional, Crippa, R., additional, Duffard, R., additional, Ditteon, R., additional, Feuerbach, M., additional, Fauvaud, S., additional, Garlitz, J., additional, Geier, S., additional, Goncalves, R., additional, Grice, J., additional, Grześkowiak, I., additional, Hirsch, R., additional, Horbowicz, J., additional, Kamiński, K., additional, Kamińska, M. K., additional, Kim, D.-H., additional, Kim, M.-J., additional, Konstanciak, I., additional, Kudak, V., additional, Kulczak, P., additional, Maestre, J. L., additional, Manzini, F., additional, Marks, S., additional, Monteiro, F., additional, Ogłoza, W., additional, Oszkiewicz, D., additional, Pilcher, F., additional, Perig, V., additional, Polakis, T., additional, Polińska, M., additional, Roy, R., additional, Sanabria, J. J., additional, Santana-Ros, T., additional, Skiff, B., additional, Skrzypek, J., additional, Sobkowiak, K., additional, Sonbas, E., additional, Thizy, O., additional, Trela, P., additional, Urakawa, S., additional, Żejmo, M., additional, and Żukowski, K., additional
Published: 2019
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19. Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988–2016

Author: Meza, E., primary, Sicardy, B., additional, Assafin, M., additional, Ortiz, J. L., additional, Bertrand, T., additional, Lellouch, E., additional, Desmars, J., additional, Forget, F., additional, Bérard, D., additional, Doressoundiram, A., additional, Lecacheux, J., additional, Oliveira, J. Marques, additional, Roques, F., additional, Widemann, T., additional, Colas, F., additional, Vachier, F., additional, Renner, S., additional, Leiva, R., additional, Braga-Ribas, F., additional, Benedetti-Rossi, G., additional, Camargo, J. I. B., additional, Dias-Oliveira, A., additional, Morgado, B., additional, Gomes-Júnior, A. R., additional, Vieira-Martins, R., additional, Behrend, R., additional, Tirado, A. Castro, additional, Duffard, R., additional, Morales, N., additional, Santos-Sanz, P., additional, Jelínek, M., additional, Cunniffe, R., additional, Querel, R., additional, Harnisch, M., additional, Jansen, R., additional, Pennell, A., additional, Todd, S., additional, Ivanov, V. D., additional, Opitom, C., additional, Gillon, M., additional, Jehin, E., additional, Manfroid, J., additional, Pollock, J., additional, Reichart, D. E., additional, Haislip, J. B., additional, Ivarsen, K. M., additional, LaCluyze, A. P., additional, Maury, A., additional, Gil-Hutton, R., additional, Dhillon, V., additional, Littlefair, S., additional, Marsh, T., additional, Veillet, C., additional, Bath, K.-L., additional, Beisker, W., additional, Bode, H.-J., additional, Kretlow, M., additional, Herald, D., additional, Gault, D., additional, Kerr, S., additional, Pavlov, H., additional, Faragó, O., additional, Klös, O., additional, Frappa, E., additional, Lavayssière, M., additional, Cole, A. A., additional, Giles, A. B., additional, Greenhill, J. G., additional, Hill, K. M., additional, Buie, M. W., additional, Olkin, C. B., additional, Young, E. F., additional, Young, L. A., additional, Wasserman, L. H., additional, Devogèle, M., additional, French, R. G., additional, Bianco, F. B., additional, Marchis, F., additional, Brosch, N., additional, Kaspi, S., additional, Polishook, D., additional, Manulis, I., additional, Ait Moulay Larbi, M., additional, Benkhaldoun, Z., additional, Daassou, A., additional, El Azhari, Y., additional, Moulane, Y., additional, Broughton, J., additional, Milner, J., additional, Dobosz, T., additional, Bolt, G., additional, Lade, B., additional, Gilmore, A., additional, Kilmartin, P., additional, Allen, W. H., additional, Graham, P. B., additional, Loader, B., additional, McKay, G., additional, Talbot, J., additional, Parker, S., additional, Abe, L., additional, Bendjoya, Ph., additional, Rivet, J.-P., additional, Vernet, D., additional, Di Fabrizio, L., additional, Lorenzi, V., additional, Magazzú, A., additional, Molinari, E., additional, Gazeas, K., additional, Tzouganatos, L., additional, Carbognani, A., additional, Bonnoli, G., additional, Marchini, A., additional, Leto, G., additional, Sanchez, R. Zanmar, additional, Mancini, L., additional, Kattentidt, B., additional, Dohrmann, M., additional, Guhl, K., additional, Rothe, W., additional, Walzel, K., additional, Wortmann, G., additional, Eberle, A., additional, Hampf, D., additional, Ohlert, J., additional, Krannich, G., additional, Murawsky, G., additional, Gährken, B., additional, Gloistein, D., additional, Alonso, S., additional, Román, A., additional, Communal, J.-E., additional, Jabet, F., additional, deVisscher, S., additional, Sérot, J., additional, Janik, T., additional, Moravec, Z., additional, Machado, P., additional, Selva, A., additional, Perelló, C., additional, Rovira, J., additional, Conti, M., additional, Papini, R., additional, Salvaggio, F., additional, Noschese, A., additional, Tsamis, V., additional, Tigani, K., additional, Barroy, P., additional, Irzyk, M., additional, Neel, D., additional, Godard, J. P., additional, Lanoiselée, D., additional, Sogorb, P., additional, Vérilhac, D., additional, Bretton, M., additional, Signoret, F., additional, Ciabattari, F., additional, Naves, R., additional, Boutet, M., additional, De Queiroz, J., additional, Lindner, P., additional, Lindner, K., additional, Enskonatus, P., additional, Dangl, G., additional, Tordai, T., additional, Eichler, H., additional, Hattenbach, J., additional, Peterson, C., additional, Molnar, L. A., additional, and Howell, R. R., additional
Published: 2019
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20. Pluto’s ephemeris from ground-based stellar occultations (1988–2016)

Author: Desmars, J., primary, Meza, E., additional, Sicardy, B., additional, Assafin, M., additional, Camargo, J. I. B., additional, Braga-Ribas, F., additional, Benedetti-Rossi, G., additional, Dias-Oliveira, A., additional, Morgado, B., additional, Gomes-Júnior, A. R., additional, Vieira-Martins, R., additional, Behrend, R., additional, Ortiz, J. L., additional, Duffard, R., additional, Morales, N., additional, and Santos Sanz, P., additional
Published: 2019
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21. Homogeneous internal structure of CM-like asteroid (41) Daphne

Author: Carry, B., primary, Vachier, F., additional, Berthier, J., additional, Marsset, M., additional, Vernazza, P., additional, Grice, J., additional, Merline, W. J., additional, Lagadec, E., additional, Fienga, A., additional, Conrad, A., additional, Podlewska-Gaca, E., additional, Santana-Ros, T., additional, Viikinkoski, M., additional, Hanuš, J., additional, Dumas, C., additional, Drummond, J. D., additional, Tamblyn, P. M., additional, Chapman, C. R., additional, Behrend, R., additional, Bernasconi, L., additional, Bartczak, P., additional, Benkhaldoun, Z., additional, Birlan, M., additional, Castillo-Rogez, J., additional, Cipriani, F., additional, Colas, F., additional, Drouard, A., additional, Ďurech, J., additional, Enke, B. L., additional, Fauvaud, S., additional, Ferrais, M., additional, Fetick, R., additional, Fusco, T., additional, Gillon, M., additional, Jehin, E., additional, Jorda, L., additional, Kaasalainen, M., additional, Keppler, M., additional, Kryszczynska, A., additional, Lamy, P., additional, Marchis, F., additional, Marciniak, A., additional, Michalowski, T., additional, Michel, P., additional, Pajuelo, M., additional, Tanga, P., additional, Vigan, A., additional, Warner, B., additional, Witasse, O., additional, Yang, B., additional, and Zurlo, A., additional
Published: 2019
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22. Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

Author: Marciniak, A., primary, Bartczak, P., additional, Müller, T., additional, Sanabria, J. J., additional, Alí-Lagoa, V., additional, Antonini, P., additional, Behrend, R., additional, Bernasconi, L., additional, Bronikowska, M., additional, Butkiewicz-Bąk, M., additional, Cikota, A., additional, Crippa, R., additional, Ditteon, R., additional, Dudziński, G., additional, Duffard, R., additional, Dziadura, K., additional, Fauvaud, S., additional, Geier, S., additional, Hirsch, R., additional, Horbowicz, J., additional, Hren, M., additional, Jerosimic, L., additional, Kamiński, K., additional, Kankiewicz, P., additional, Konstanciak, I., additional, Korlevic, P., additional, Kosturkiewicz, E., additional, Kudak, V., additional, Manzini, F., additional, Morales, N., additional, Murawiecka, M., additional, Ogłoza, W., additional, Oszkiewicz, D., additional, Pilcher, F., additional, Polakis, T., additional, Poncy, R., additional, Santana-Ros, T., additional, Siwak, M., additional, Skiff, B., additional, Sobkowiak, K., additional, Stoss, R., additional, Żejmo, M., additional, and Żukowski, K., additional
Published: 2018
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23. Shape and spin determination of Barbarian asteroids

Author: Devogèle, M., primary, Tanga, P., additional, Bendjoya, P., additional, Rivet, J. P., additional, Surdej, J., additional, Hanuš, J., additional, Abe, L., additional, Antonini, P., additional, Artola, R. A., additional, Audejean, M., additional, Behrend, R., additional, Berski, F., additional, Bosch, J. G., additional, Bronikowska, M., additional, Carbognani, A., additional, Char, F., additional, Kim, M.-J., additional, Choi, Y.-J., additional, Colazo, C. A., additional, Coloma, J., additional, Coward, D., additional, Durkee, R., additional, Erece, O., additional, Forne, E., additional, Hickson, P., additional, Hirsch, R., additional, Horbowicz, J., additional, Kamiński, K., additional, Kankiewicz, P., additional, Kaplan, M., additional, Kwiatkowski, T., additional, Konstanciak, I., additional, Kruszewki, A., additional, Kudak, V., additional, Manzini, F., additional, Moon, H.-K., additional, Marciniak, A., additional, Murawiecka, M., additional, Nadolny, J., additional, Ogłoza, W., additional, Ortiz, J. L., additional, Oszkiewicz, D., additional, Pallares, H., additional, Peixinho, N., additional, Poncy, R., additional, Reyes, F., additional, de los Reyes, J. A., additional, Santana-Ros, T., additional, Sobkowiak, K., additional, Pastor, S., additional, Pilcher, F., additional, Quiñones, M. C., additional, Trela, P., additional, and Vernet, D., additional
Published: 2017
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24. Shape and spin determination of Barbarian asteroids

Author: Natural Sciences and Engineering Research Council of Canada, European Commission, Fundação para a Ciência e a Tecnologia (Portugal), National Science Centre (Poland), Devogèle, M., Tanga, P., Bendjoya, P., Rivet, J.P., Surdej, J., Hanuš, 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, José Luis, Oszkiewicz, D., Pallares, H., Peixinho, N., Poncy, R., Reyes, F., de los Reyes, J.A., Santana-Ros, Toni, Sobkowiak, K., Pastor, S., Natural Sciences and Engineering Research Council of Canada, European Commission, Fundação para a Ciência e a Tecnologia (Portugal), National Science Centre (Poland), Devogèle, M., Tanga, P., Bendjoya, P., Rivet, J.P., Surdej, J., Hanuš, 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, José Luis, Oszkiewicz, D., Pallares, H., Peixinho, N., Poncy, R., Reyes, F., de los Reyes, J.A., Santana-Ros, Toni, Sobkowiak, K., and Pastor, S.
Abstract: 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 suggested, large scale topographic features could play a role in the polarimetric response, if the shapes of Barbarians are particularly irregular and present a variety of scattering/incidence angles. This idea is supported by the shape of (234) Barbara, that appears to be deeply excavated by wide concave areas revealed by photometry and stellar occultations. Aims. With these motivations, we started an observation campaign to characterise the shape and rotation properties of Small Main-Belt Asteroid Spectroscopic Survey (SMASS) type L and Ld asteroids. As many of them show long rotation periods, we activated a worldwide network of observers to obtain a dense temporal coverage. Methods. We used light-curve inversion technique in order to determine the sidereal rotation periods of 15 asteroids and the convergence to a stable shape and pole coordinates for 8 of them. By using available data from occultations, we are able to scale some shapes to an absolute size. We also study the rotation periods of our sample looking for confirmation of the suspected abundance of asteroids with long rotation periods. Results. Our results show that the shape models of our sample do not seem to have peculiar properties with respect to asteroids with similar size, while an excess of slow rotators is most probably confirmed.© 2017 ESO.
Published: 2017

25. 3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites

Author: Marsset, M., primary, Carry, B., additional, Dumas, C., additional, Hanuš, J., additional, Viikinkoski, M., additional, Vernazza, P., additional, Müller, T. G., additional, Delbo, M., additional, Jehin, E., additional, Gillon, M., additional, Grice, J., additional, Yang, B., additional, Fusco, T., additional, Berthier, J., additional, Sonnett, S., additional, Kugel, F., additional, Caron, J., additional, and Behrend, R., additional
Published: 2017
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26. New and updated convex shape models of asteroids based on optical data from a large collaboration network

Author: Hanuš, J., primary, Ďurech, J., additional, Oszkiewicz, D. A., additional, Behrend, R., additional, Carry, B., additional, Delbo, M., additional, Adam, O., additional, Afonina, V., additional, Anquetin, R., additional, Antonini, P., additional, Arnold, L., additional, Audejean, M., additional, Aurard, P., additional, Bachschmidt, M., additional, Baduel, B., additional, Barbotin, E., additional, Barroy, P., additional, Baudouin, P., additional, Berard, L., additional, Berger, N., additional, Bernasconi, L., additional, Bosch, J-G., additional, Bouley, S., additional, Bozhinova, I., additional, Brinsfield, J., additional, Brunetto, L., additional, Canaud, G., additional, Caron, J., additional, Carrier, F., additional, Casalnuovo, G., additional, Casulli, S., additional, Cerda, M., additional, Chalamet, L., additional, Charbonnel, S., additional, Chinaglia, B., additional, Cikota, A., additional, Colas, F., additional, Coliac, J.-F., additional, Collet, A., additional, Coloma, J., additional, Conjat, M., additional, Conseil, E., additional, Costa, R., additional, Crippa, R., additional, Cristofanelli, M., additional, Damerdji, Y., additional, Debackère, A., additional, Decock, A., additional, Déhais, Q., additional, Déléage, T., additional, Delmelle, S., additional, Demeautis, C., additional, Dróżdż, M., additional, Dubos, G., additional, Dulcamara, T., additional, Dumont, M., additional, Durkee, R., additional, Dymock, R., additional, Escalante del Valle, A., additional, Esseiva, N., additional, Esseiva, R., additional, Esteban, M., additional, Fauchez, T., additional, Fauerbach, M., additional, Fauvaud, M., additional, Fauvaud, S., additional, Forné, E., additional, Fournel, C., additional, Fradet, D., additional, Garlitz, J., additional, Gerteis, O., additional, Gillier, C., additional, Gillon, M., additional, Giraud, R., additional, Godard, J.-P., additional, Goncalves, R., additional, Hamanowa, Hiroko, additional, Hamanowa, Hiromi, additional, Hay, K., additional, Hellmich, S., additional, Heterier, S., additional, Higgins, D., additional, Hirsch, R., additional, Hodosan, G., additional, Hren, M., additional, Hygate, A., additional, Innocent, N., additional, Jacquinot, H., additional, Jawahar, S., additional, Jehin, E., additional, Jerosimic, L., additional, Klotz, A., additional, Koff, W., additional, Korlevic, P., additional, Kosturkiewicz, E., additional, Krafft, P., additional, Krugly, Y., additional, Kugel, F., additional, Labrevoir, O., additional, Lecacheux, J., additional, Lehký, M., additional, Leroy, A., additional, Lesquerbault, B., additional, Lopez-Gonzales, M. J., additional, Lutz, M., additional, Mallecot, B., additional, Manfroid, J., additional, Manzini, F., additional, Marciniak, A., additional, Martin, A., additional, Modave, B., additional, Montaigut, R., additional, Montier, J., additional, Morelle, E., additional, Morton, B., additional, Mottola, S., additional, Naves, R., additional, Nomen, J., additional, Oey, J., additional, Ogłoza, W., additional, Paiella, M., additional, Pallares, H., additional, Peyrot, A., additional, Pilcher, F., additional, Pirenne, J.-F., additional, Piron, P., additional, Polińska, M., additional, Polotto, M., additional, Poncy, R., additional, Previt, J. P., additional, Reignier, F., additional, Renauld, D., additional, Ricci, D., additional, Richard, F., additional, Rinner, C., additional, Risoldi, V., additional, Robilliard, D., additional, Romeuf, D., additional, Rousseau, G., additional, Roy, R., additional, Ruthroff, J., additional, Salom, P. A., additional, Salvador, L., additional, Sanchez, S., additional, Santana-Ros, T., additional, Scholz, A., additional, Séné, G., additional, Skiff, B., additional, Sobkowiak, K., additional, Sogorb, P., additional, Soldán, F., additional, Spiridakis, A., additional, Splanska, E., additional, Sposetti, S., additional, Starkey, D., additional, Stephens, R., additional, Stiepen, A., additional, Stoss, R., additional, Strajnic, J., additional, Teng, J.-P., additional, Tumolo, G., additional, Vagnozzi, A., additional, Vanoutryve, B., additional, Vugnon, J. M., additional, Warner, B. D., additional, Waucomont, M., additional, Wertz, O., additional, Winiarski, M., additional, and Wolf, M., additional
Published: 2016
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27. SOPHIE velocimetry ofKeplertransit candidates

Author: Santerne, A., primary, Hébrard, G., additional, Deleuil, M., additional, Havel, M., additional, Correia, A. C. M., additional, Almenara, J.-M., additional, Alonso, R., additional, Arnold, L., additional, Barros, S. C. C., additional, Behrend, R., additional, Bernasconi, L., additional, Boisse, I., additional, Bonomo, A. S., additional, Bouchy, F., additional, Bruno, G., additional, Damiani, C., additional, Díaz, R. F., additional, Gravallon, D., additional, Guillot, T., additional, Labrevoir, O., additional, Montagnier, G., additional, Moutou, C., additional, Rinner, C., additional, Santos, N. C., additional, Abe, L., additional, Audejean, M., additional, Bendjoya, P., additional, Gillier, C., additional, Gregorio, J., additional, Martinez, P., additional, Michelet, J., additional, Montaigut, R., additional, Poncy, R., additional, Rivet, J.-P., additional, Rousseau, G., additional, Roy, R., additional, Suarez, O., additional, Vanhuysse, M., additional, and Verilhac, D., additional
Published: 2014
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28. An exploration of Pluto’s environment through stellar occultations

Author: Boissel, Y., primary, Sicardy, B., additional, Roques, F., additional, Gaulme, P., additional, Doressoundiram, A., additional, Widemann, T., additional, Ivanov, V. D., additional, Marco, O., additional, Mason, E., additional, Ageorges, N., additional, Mousis, O., additional, Rousselot, P., additional, Dhillon, V. S., additional, Littlefair, S. P., additional, Marsh, T. R., additional, Assafin, M., additional, Braga Ribas, F., additional, da Silva Neto, D., additional, Camargo, J. I. B., additional, Andrei, A., additional, Vieira Martins, R., additional, Behrend, R., additional, and Kretlow, M., additional
Published: 2014
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29. The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign

Author: Physics, Fauvaud, S., Sareyan, J. P., Ribas, I., Rodriguez, E., Lampens, P., Klingenberg, G., Farrell, J. A., Fumagalli, F., Simonetti, John H., Wolf, M., Santacana, G., Zhou, A. Y., Michel, R., Fox-Machado, L., Alvarez, M., Nava-Vega, A., Lopez-Gonzalez, M. J., Casanova, V. M., Aceituno, F. J., Scheggia, I., Rives, J. J., Hintz, E. G., Van Cauteren, P., Helvaci, M., Yesilyaprak, C., Graham, K. A., Kral, L., Kocian, R., Kucakova, H., Fauvaud, M., Granslo, B. H., Michelet, J., Nicholson, M. P., Vugnon, J. M., Kotkova, L., Truparova, K., Ulusoy, C., Yasarsoy, B., Avdibegtovic, A., Blazek, M., Kliner, J., Zasche, P., Bartosikova, S., Vilasek, M., Trondal, O., Van Den Abbeel, F., Behrend, R., Wucher, H., Physics, Fauvaud, S., Sareyan, J. P., Ribas, I., Rodriguez, E., Lampens, P., Klingenberg, G., Farrell, J. A., Fumagalli, F., Simonetti, John H., Wolf, M., Santacana, G., Zhou, A. Y., Michel, R., Fox-Machado, L., Alvarez, M., Nava-Vega, A., Lopez-Gonzalez, M. J., Casanova, V. M., Aceituno, F. J., Scheggia, I., Rives, J. J., Hintz, E. G., Van Cauteren, P., Helvaci, M., Yesilyaprak, C., Graham, K. A., Kral, L., Kocian, R., Kucakova, H., Fauvaud, M., Granslo, B. H., Michelet, J., Nicholson, M. P., Vugnon, J. M., Kotkova, L., Truparova, K., Ulusoy, C., Yasarsoy, B., Avdibegtovic, A., Blazek, M., Kliner, J., Zasche, P., Bartosikova, S., Vilasek, M., Trondal, O., Van Den Abbeel, F., Behrend, R., and Wucher, H.
Abstract: Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip. Most of them have very simple pulsational behaviours, only one or two radial modes being excited. Nevertheless, BL Cam is a unique object among them, being an extreme metal-deficient field high-amplitude SX Phe variable with a large number of frequencies. Based on a frequency analysis, a pulsational interpretation was previously given. Aims. We attempt to interpret the long-term behaviour of the residuals that were not taken into account in the previous Observed-Calculated (O-C) short-term analyses. Methods. An investigation of the O-C times has been carried out, using a data set based on the previous published times of light maxima, largely enriched by those obtained during an intensive multisite photometric campaign of BL Cam lasting several months. Results. In addition to a positive (161 +/- 3) x 10(-9) yr(-1) secular relative increase in the main pulsation period of BL Cam, we detected in the O-C data short- (144.2 d) and long-term (similar to 3400 d) variations, both incompatible with a scenario of stellar evolution. Conclusions. Interpreted as a light travel-time effect, the short- term O-C variation is indicative of a massive stellar component (0.46 to 1 M(circle dot)) with a short period orbit (144.2 d), within a distance of 0.7 AU from the primary. More observations are needed to confirm the long-term O-C variations: if they were also to be caused by a light travel-time effect, they could be interpreted in terms of a third component, in this case probably a brown dwarf star (>= 0.03 M(circle dot)), orbiting in similar to 3400 d at a distance of 4.5 AU from the primary.
Published: 2010

30. Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

Author: Hanuš, J., primary, Ďurech, J., additional, Brož, M., additional, Marciniak, A., additional, Warner, B. D., additional, Pilcher, F., additional, Stephens, R., additional, Behrend, R., additional, Carry, B., additional, Čapek, D., additional, Antonini, P., additional, Audejean, M., additional, Augustesen, K., additional, Barbotin, E., additional, Baudouin, P., additional, Bayol, A., additional, Bernasconi, L., additional, Borczyk, W., additional, Bosch, J.-G., additional, Brochard, E., additional, Brunetto, L., additional, Casulli, S., additional, Cazenave, A., additional, Charbonnel, S., additional, Christophe, B., additional, Colas, F., additional, Coloma, J., additional, Conjat, M., additional, Cooney, W., additional, Correira, H., additional, Cotrez, V., additional, Coupier, A., additional, Crippa, R., additional, Cristofanelli, M., additional, Dalmas, Ch., additional, Danavaro, C., additional, Demeautis, C., additional, Droege, T., additional, Durkee, R., additional, Esseiva, N., additional, Esteban, M., additional, Fagas, M., additional, Farroni, G., additional, Fauvaud, M., additional, Fauvaud, S., additional, Del Freo, F., additional, Garcia, L., additional, Geier, S., additional, Godon, C., additional, Grangeon, K., additional, Hamanowa, H., additional, Heck, N., additional, Hellmich, S., additional, Higgins, D., additional, Hirsch, R., additional, Husarik, M., additional, Itkonen, T., additional, Jade, O., additional, Kamiński, K., additional, Kankiewicz, P., additional, Klotz, A., additional, Koff, R. A., additional, Kryszczyńska, A., additional, Kwiatkowski, T., additional, Laffont, A., additional, Leroy, A., additional, Lecacheux, J., additional, Leonie, Y., additional, Leyrat, C., additional, Manzini, F., additional, Martin, A., additional, Masi, G., additional, Matter, D., additional, Michałowski, J., additional, Michałowski, M. J., additional, Michałowski, T., additional, Michelet, J., additional, Michelsen, R., additional, Morelle, E., additional, Mottola, S., additional, Naves, R., additional, Nomen, J., additional, Oey, J., additional, Ogłoza, W., additional, Oksanen, A., additional, Oszkiewicz, D., additional, Pääkkönen, P., additional, Paiella, M., additional, Pallares, H., additional, Paulo, J., additional, Pavic, M., additional, Payet, B., additional, Polińska, M., additional, Polishook, D., additional, Poncy, R., additional, Revaz, Y., additional, Rinner, C., additional, Rocca, M., additional, Roche, A., additional, Romeuf, D., additional, Roy, R., additional, Saguin, H., additional, Salom, P. A., additional, Sanchez, S., additional, Santacana, G., additional, Santana-Ros, T., additional, Sareyan, J.-P., additional, Sobkowiak, K., additional, Sposetti, S., additional, Starkey, D., additional, Stoss, R., additional, Strajnic, J., additional, Teng, J.-P., additional, Trégon, B., additional, Vagnozzi, A., additional, Velichko, F. P., additional, Waelchli, N., additional, Wagrez, K., additional, and Wücher, H., additional
Published: 2013
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31. Do Slivan states exist in the Flora family?

Author: Kryszczyńska, A., primary, Colas, F., additional, Polińska, M., additional, Hirsch, R., additional, Ivanova, V., additional, Apostolovska, G., additional, Bilkina, B., additional, Velichko, F. P., additional, Kwiatkowski, T., additional, Kankiewicz, P., additional, Vachier, F., additional, Umlenski, V., additional, Michałowski, T., additional, Marciniak, A., additional, Maury, A., additional, Kamiński, K., additional, Fagas, M., additional, Dimitrov, W., additional, Borczyk, W., additional, Sobkowiak, K., additional, Lecacheux, J., additional, Behrend, R., additional, Klotz, A., additional, Bernasconi, L., additional, Crippa, R., additional, Manzini, F., additional, Poncy, R., additional, Antonini, P., additional, Oszkiewicz, D., additional, and Santana-Ros, T., additional
Published: 2012
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32. Photometry and models of selected main belt asteroids

Author: Marciniak, A., primary, Bartczak, P., additional, Santana-Ros, T., additional, Michałowski, T., additional, Antonini, P., additional, Behrend, R., additional, Bembrick, C., additional, Bernasconi, L., additional, Borczyk, W., additional, Colas, F., additional, Coloma, J., additional, Crippa, R., additional, Esseiva, N., additional, Fagas, M., additional, Fauvaud, M., additional, Fauvaud, S., additional, Ferreira, D. D. M., additional, Hein Bertelsen, R. P., additional, Higgins, D., additional, Hirsch, R., additional, Kajava, J. J. E., additional, Kamiński, K., additional, Kryszczyńska, A., additional, Kwiatkowski, T., additional, Manzini, F., additional, Michałowski, J., additional, Michałowski, M. J., additional, Paschke, A., additional, Polińska, M., additional, Poncy, R., additional, Roy, R., additional, Santacana, G., additional, Sobkowiak, K., additional, Stasik, M., additional, Starczewski, S., additional, Velichko, F., additional, Wucher, H., additional, and Zafar, T., additional
Published: 2012
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33. A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method

Author: Hanuš, J., primary, Ďurech, J., additional, Brož, M., additional, Warner, B. D., additional, Pilcher, F., additional, Stephens, R., additional, Oey, J., additional, Bernasconi, L., additional, Casulli, S., additional, Behrend, R., additional, Polishook, D., additional, Henych, T., additional, Lehký, M., additional, Yoshida, F., additional, and Ito, T., additional
Published: 2011
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34. Photometry and models of selected main belt asteroids

Author: Marciniak, A., primary, Michałowski, T., additional, Polińska, M., additional, Bartczak, P., additional, Hirsch, R., additional, Sobkowiak, K., additional, Kamiński, K., additional, Fagas, M., additional, Behrend, R., additional, Bernasconi, L., additional, Bosch, J.-G., additional, Brunetto, L., additional, Choisay, F., additional, Coloma, J., additional, Conjat, M., additional, Farroni, G., additional, Manzini, F., additional, Pallares, H., additional, Roy, R., additional, Kwiatkowski, T., additional, Kryszczyńska, A., additional, Rudawska, R., additional, Starczewski, S., additional, Michałowski, J., additional, and Ludick, P., additional
Published: 2011
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35. Physical properties of the ESA Rosetta target asteroid (21) Lutetia

Author: Carry, B., primary, Kaasalainen, M., additional, Leyrat, C., additional, Merline, W. J., additional, Drummond, J. D., additional, Conrad, A., additional, Weaver, H. A., additional, Tamblyn, P. M., additional, Chapman, C. R., additional, Dumas, C., additional, Colas, F., additional, Christou, J. C., additional, Dotto, E., additional, Perna, D., additional, Fornasier, S., additional, Bernasconi, L., additional, Behrend, R., additional, Vachier, F., additional, Kryszczynska, A., additional, Polinska, M., additional, Fulchignoni, M., additional, Roy, R., additional, Naves, R., additional, Poncy, R., additional, and Wiggins, P., additional
Published: 2010
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36. The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign

Author: Fauvaud, S., primary, Sareyan, J.-P., additional, Ribas, I., additional, Rodríguez, E., additional, Lampens, P., additional, Klingenberg, G., additional, Farrell, J. A., additional, Fumagalli, F., additional, Simonetti, J. H., additional, Wolf, M., additional, Santacana, G., additional, Zhou, A.-Y., additional, Michel, R., additional, Fox-Machado, L., additional, Alvarez, M., additional, Nava-Vega, A., additional, López-González, M. J., additional, Casanova, V. M., additional, Aceituno, F. J., additional, Scheggia, I., additional, Rives, J.-J., additional, Hintz, E. G., additional, Van Cauteren, P., additional, Helvaci, M., additional, Yesilyaprak, C., additional, Graham, K. A., additional, Král, L., additional, Kocián, R., additional, Kučáková, H., additional, Fauvaud, M., additional, Granslo, B. H., additional, Michelet, J., additional, Nicholson, M. P., additional, Vugnon, J.-M., additional, Kotková, L., additional, Truparová, K., additional, Ulusoy, C., additional, Yasarsoy, B., additional, Avdibegovic, A., additional, Blaĭek, M., additional, Kliner, J., additional, Zasche, P., additional, Bartošíková, S., additional, Vilášek, M., additional, Trondal, O., additional, Van Den Abbeel, F., additional, Behrend, R., additional, and Wücher, H., additional
Published: 2010
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37. Photometry and models of selected main belt asteroids

Author: Marciniak, A., primary, Michałowski, T., additional, Hirsch, R., additional, Behrend, R., additional, Bernasconi, L., additional, Descamps, P., additional, Colas, F., additional, Sobkowiak, K., additional, Kamiński, K., additional, Kryszczyńska, A., additional, Kwiatkowski, T., additional, Polińska, M., additional, Rudawska, R., additional, Fauvaud, S., additional, Santacana, G., additional, Bruno, A., additional, Fauvaud, M., additional, Teng-Chuen-Yu, J.-P., additional, and Peyrot, A., additional
Published: 2009
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38. Asteroid models from combined sparse and dense photometric data

Author: Ďurech, J., primary, Kaasalainen, M., additional, Warner, B. D., additional, Fauerbach, M., additional, Marks, S. A., additional, Fauvaud, S., additional, Fauvaud, M., additional, Vugnon, J.-M., additional, Pilcher, F., additional, Bernasconi, L., additional, and Behrend, R., additional
Published: 2008
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39. Photometry and models of selected main belt asteroids

Author: Marciniak, A., primary, Michałowski, T., additional, Kaasalainen, M., additional, Kryszczyńska, A., additional, Kwiatkowski, T., additional, Hirsch, R., additional, Kamiński, K., additional, Fagas, M., additional, Polińska, M., additional, Velichko, F. P., additional, Michałowski, M. J., additional, Snodgrass, C., additional, Behrend, R., additional, and Bernasconi, L., additional
Published: 2007
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40. Physical models of ten asteroids from an observers' collaboration network

Author: Ďurech, J., primary, Kaasalainen, M., additional, Marciniak, A., additional, Allen, W. H., additional, Behrend, R., additional, Bembrick, C., additional, Bennett, T., additional, Bernasconi, L., additional, Berthier, J., additional, Bolt, G., additional, Boroumand, S., additional, Crespo da Silva, L., additional, Crippa, R., additional, Crow, M., additional, Durkee, R., additional, Dymock, R., additional, Fagas, M., additional, Fauerbach, M., additional, Fauvaud, S., additional, Frey, M., additional, Gonçalves, R., additional, Hirsch, R., additional, Jardine, D., additional, Kamiński, K., additional, Koff, R., additional, Kwiatkowski, T., additional, López, A., additional, Manzini, F., additional, Michałowski, T., additional, Pacheco, R., additional, Pan, M., additional, Pilcher, F., additional, Poncy, R., additional, Pray, D., additional, Pych, W., additional, Roy, R., additional, Santacana, G., additional, Slivan, S., additional, Sposetti, S., additional, Stephens, R., additional, Warner, B., additional, and Wolf, M., additional
Published: 2007
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41. SOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet.

Author: Santos, N. C., Santerne, A., Boisse, I., Behrend, R., Rousseau, G., Bernasconi, L., Bonomo, A. S., Labrevoir, O., Rinner, C., Audejean, M., Gillier, C., Michelet, J., Montaigut, R., Gregorio, J., Martinez, P., Poncy, R., Roy, R., Vanhuysse, M., Verilhac, D., and Deleuil, M.
Subjects: EXTRASOLAR planets, VELOCIMETRY, SPECTROGRAPHS, SPECTRAL energy distribution, BINARY systems (Astronomy), PLANETARY orbits, LIGHT curves
Abstract: 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 Kepler space telescope and then validated thanks to a radial velocity follow-up with the SOPHIE spectrograph. It orbits its host star with a period of 86.647661 d ± 3 s and a high eccentricity of 0.772 ± 0.045. The planet transits the main star of a metal-rich, relatively old binary system with stars of mass of 0.99± 0.05 M☉ and 0.70 ± 0.07 M☉ for the primary and secondary, respectively. This binary system is constrained thanks to a self-consistent modelling of the Kepler transit light curve, the SOPHIE radial velocities, line bisector and full-width half maximum (FWHM) variations, and the spectral energy distribution. However, future observations are needed to confirm it. The PASTIS fully-Bayesian software was used to validate the nature of the planet and to determine which star of the binary system is the transit host. By accounting for the dilution from the binary both in photometry and in radial velocity, we find that the planet has a mass of 1.45 ± 0.35 M2+, and a radius of 0.94 ± 0.12 R2+, and thus a bulk density of 2.1 ± 1.2 g cm-3. The planet has an equilibrium temperature of 511± 50 K, making it one of the few known members of the warm-Jupiter population. The HARPS-N spectrograph was also used to observe a transit of KOI-1257 b, simultaneously with a joint amateur and professional photometric follow-up, with the aim of constraining the orbital obliquity of the planet. However, the Rossiter-McLaughlin effect was not clearly detected, resulting in poor constraints on the orbital obliquity of the planet. [ABSTRACT FROM AUTHOR]
Published: 2014
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42. Continuous optical monitoring during the prompt emission of GRB 060111B

Author: Klotz, A., primary, Gendre, B., additional, Stratta, G., additional, Atteia, J. L., additional, Boër, M., additional, Malacrino, F., additional, Damerdji, Y., additional, and Behrend, R., additional
Published: 2006
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43. Radius and mass of a transiting M dwarf near the hydrogen-burning limit

Author: Pont, F., primary, Moutou, C., additional, Bouchy, F., additional, Behrend, R., additional, Mayor, M., additional, Udry, S., additional, Queloz, D., additional, Santos, N., additional, and Melo, C., additional
Published: 2006
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44. Four new binary minor planets: (854) Frostia, (1089) Tama, (1313) Berna, (4492) Debussy

Author: Behrend, R., primary, Bernasconi, L., additional, Roy, R., additional, Klotz, A., additional, Colas, F., additional, Antonini, P., additional, Aoun, R., additional, Augustesen, K., additional, Barbotin, E., additional, Berger, N., additional, Berrouachdi, H., additional, Brochard, E., additional, Cazenave, A., additional, Cavadore, C., additional, Coloma, J., additional, Cotrez, V., additional, Deconihout, S., additional, Demeautis, C., additional, Dorseuil, J., additional, Dubos, G., additional, Durkee, R., additional, Frappa, E., additional, Hormuth, F., additional, Itkonen, T., additional, Jacques, C., additional, Kurtze, L., additional, Laffont, A., additional, Lavayssière, M., additional, Lecacheux, J., additional, Leroy, A., additional, Manzini, F., additional, Masi, G., additional, Matter, D., additional, Michelsen, R., additional, Nomen, J., additional, Oksanen, A., additional, Pääkkönen, P., additional, Peyrot, A., additional, Pimentel, E., additional, Pray, D., additional, Rinner, C., additional, Sanchez, S., additional, Sonnenberg, K., additional, Sposetti, S., additional, Starkey, D., additional, Stoss, R., additional, Teng, J.-P., additional, Vignand, M., additional, and Waelchli, N., additional
Published: 2006
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45. Early re-brightening of the afterglow of GRB 050525a

Author: Klotz, A., primary, Boër, M., additional, Atteia, J. L., additional, Stratta, G., additional, Behrend, R., additional, Malacrino, F., additional, and Damerdji, Y., additional
Published: 2005
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46. Eclipsing binary asteroid 90 Antiope

Author: Michałowski, T., primary, Bartczak, P., additional, Velichko, F. P., additional, Kryszczyńska, A., additional, Kwiatkowski, T., additional, Breiter, S., additional, Colas, F., additional, Fauvaud, S., additional, Marciniak, A., additional, Michałowski, J., additional, Hirsch, R., additional, Behrend, R., additional, Bernasconi, L., additional, Rinner, C., additional, and Charbonnel, S., additional
Published: 2004
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47. Formation of massive stars by growing accretion rate

Author: Behrend, R., primary and Maeder, A., additional
Published: 2001
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