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201. FRIPON: a worldwide network to track incoming meteoroids

Author: Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., Gattacceca, J., Jorda, L., Lecubin, J., Marmo, C., Rault, J. L., Vaubaillon, J., Vernazza, P., Yohia, C., Gardiol, D., Nedelcu, A., Poppe, B., Rowe, J., Forcier, M., Koschny, D., Trigo-Rodriguez, J. M., Lamy, H., Behrend, R., Ferrière, L., Barghini, D., Buzzoni, A., Carbognani, A., Di Carlo, M., Di Martino, M., Knapic, C., Londero, E., Pratesi, G., Rasetti, S., Riva, W., Stirpe, G. M., Valsecchi, G. B., Volpicelli, C. A., Zorba, S., Coward, D., Drolshagen, E., Drolshagen, G., Hernandez, O., Jehin, E., Jobin, M., King, A., Nitschelm, C., Ott, T., Sanchez-Lavega, A., Toni, A., Abraham, P., Affaticati, F., Albani, M., Andreis, A., Andrieu, T., Anghel, S., Antaluca, E., Antier, K., Appéré, T., Armand, A., Ascione, G., Audureau, Y., Auxepaules, G., Avoscan, T., Baba Aissa, D., Bacci, P., Bǎdescu, O., Baldini, R., Baldo, R., Balestrero, A., Baratoux, D., Barbotin, E., Bardy, M., Basso, S., Bautista, O., Bayle, L. D., Beck, P., Bellitto, R., Belluso, R., Benna, C., Benammi, M., Beneteau, E., Benkhaldoun, Z., Bergamini, P., Bernardi, F., Bertaina, M. E., Bessin, P., Betti, L., Bettonvil, F., Bihel, D., Birnbaum, C., Blagoi, O., Blouri, E., Boacă, I., Boatǎ, R., Bobiet, B., Bonino, R., Boros, K., Bouchet, E., Borgeot, V., Bouchez, E., Boust, D., Boudon, V., Bouman, T., Bourget, P., Brandenburg, S., Bramond, Ph., Braun, E., Bussi, A., Cacault, P., Caillier, B., Calegaro, A., Camargo, J., Caminade, S., Campana, A. P. C., Campbell-Burns, P., Canal-Domingo, R., Carell, O., Carreau, S., Cascone, E., Cattaneo, C., Cauhape, P., Cavier, P., Celestin, S., Cellino, A., Champenois, M., Chennaoui Aoudjehane, H., Chevrier, S., Cholvy, P., Chomier, L., Christou, A., Cricchio, D., Coadou, P., Cocaign, J. Y., Cochard, F., Cointin, S., Colombi, E., Colque Saavedra, J. P., Corp, L., Costa, M., Costard, F., Cottier, M., Cournoyer, P., Coustal, E., Cremonese, G., Cristea, O., Cuzon, J. C., D’Agostino, G., Daiffallah, K., Dǎnescu, C., Dardon, A., Dasse, T., Davadan, C., Debs, V., Defaix, J. P., Deleflie, F., D’Elia, M., De Luca, P., De Maria, P., Deverchère, P., Devillepoix, H., Dias, A., Di Dato, A., Di Luca, R., Dominici, F. M., Drouard, A., Dumont, J. L., Dupouy, P., Duvignac, L., Egal, A., Erasmus, N., Esseiva, N., Ebel, A., Eisengarten, B., Federici, F., Feral, S., Ferrant, G., Ferreol, E., Finitzer, P., Foucault, A., Francois, P., Frîncu, M., Froger, J. L., Gaborit, F., Gagliarducci, V., Galard, J., Gardavot, A., Garmier, M., Garnung, M., Gautier, B., Gendre, B., Gerard, D., Gerardi, A., Godet, J. P., Grandchamps, A., Grouiez, B., Groult, S., Guidetti, D., Giuli, G., Hello, Y., Henry, X., Herbreteau, G., Herpin, M., Hewins, P., Hillairet, J. J., Horak, J., Hueso, R., Huet, E., Huet, S., Hyaumé, F., Interrante, G., Isselin, Y., Jeangeorges, Y., Janeux, P., Jeanneret, P., Jobse, K., Jouin, S., Jouvard, J. M., Joy, K., Julien, J. F., Kacerek, R., Kaire, M., Kempf, M., Krier, C., Kwon, M. K., Lacassagne, L., Lachat, D., Lagain, A., Laisné, E., Lanchares, V., Laskar, J., Lazzarin, M., Leblanc, M., Lebreton, J. P., Lecomte, J., Le Dû, P., Lelong, F., Lera, S., Leoni, J. F., Le-Pichon, A., Le-Poupon, P., Leroy, A., Leto, G., Levansuu, A., Lewin, E., Lienard, A., Licchelli, D., Locatelli, H., Loehle, S., Loizeau, D., Luciani, L., Maignan, M., Manca, F., Mancuso, S., Mandon, E., Mangold, N., Mannucci, F., Maquet, L., Marant, D., Marchal, Y., Marin, J. L., Martin-Brisset, J. C., Martin, D., Mathieu, D., Maury, A., Mespoulet, N., Meyer, F., Meyer, J. Y., Meza, E., Moggi Cecchi, V., Moiroud, J. J., Millan, M., Montesarchio, M., Misiano, A., Molinari, E., Molau, S., Monari, J., Monflier, B., Monkos, A., Montemaggi, M., Monti, G., Moreau, R., Morin, J., Mourgues, R., Mousis, O., Nablanc, C., Nastasi, A., Niacşu, L., Notez, P., Ory, M., Pace, E., Paganelli, M. A., Pagola, A., Pajuelo, M., Palacián, J. F., Pallier, G., Paraschiv, P., Pardini, R., Pavone, M., Pavy, G., Payen, G., Pegoraro, A., Peña-Asensio, E., Perez, L., Pérez-Hoyos, S., Perlerin, V., Peyrot, A., Peth, F., Pic, V., Pietronave, S., Pilger, C., Piquel, M., Pisanu, T., Poppe, M., Portois, L., Prezeau, J. F., Pugno, N., Quantin, C., Quitté, G., Rambaux, N., Ravier, E., Repetti, U., Ribas, S., Richard, C., Richard, D., Rigoni, M., Rivet, J. P., Rizzi, N., Rochain, S., Rojas, J.F., Romeo, M., Rotaru, M., Rotger, M., Rougier, P., Rousselot, P., Rousset, J., Rousseu, D., Rubiera, O., Rudawska, R., Rudelle, J., Ruguet, J.P., Russo, P., Sales, S., Sauzereau, O., Salvati, F., Schieffer, M., Schreiner, D., Scribano, Y., Selvestrel, D., Serra, R., Shengold, L., Shuttleworth, A., Smareglia, R., Sohy, S., Soldi, M., Stanga, R., Steinhausser, A., Strafella, F., Sylla Mbaye, S., Smedley, A. R. D., Tagger, M., Tanga, P., Taricco, C., Teng, J. P., Tercu, J. O., Thizy, O., Thomas, J. P., Tombelli, M., Trangosi, R., Tregon, B., Trivero, P., Tukkers, A., Turcu, V., Umbriaco, G., Unda-Sanzana, E., Vairetti, R., Valenzuela, M., Valente, G., Varennes, G., Vauclair, S., Vergne, J., Verlinden, M., Vidal-Alaiz, M., Vieira-Martins, R., Viel, A., Vîntdevarǎ, D. C., Vinogradoff, V., Volpini, P., Wendling, M., Wilhelm, P., Wohlgemuth, K., Yanguas, P., Zagarella, R., Zollo, A., Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., Gattacceca, J., Jorda, L., Lecubin, J., Marmo, C., Rault, J. L., Vaubaillon, J., Vernazza, P., Yohia, C., Gardiol, D., Nedelcu, A., Poppe, B., Rowe, J., Forcier, M., Koschny, D., Trigo-Rodriguez, J. M., Lamy, H., Behrend, R., Ferrière, L., Barghini, D., Buzzoni, A., Carbognani, A., Di Carlo, M., Di Martino, M., Knapic, C., Londero, E., Pratesi, G., Rasetti, S., Riva, W., Stirpe, G. M., Valsecchi, G. B., Volpicelli, C. A., Zorba, S., Coward, D., Drolshagen, E., Drolshagen, G., Hernandez, O., Jehin, E., Jobin, M., King, A., Nitschelm, C., Ott, T., Sanchez-Lavega, A., Toni, A., Abraham, P., Affaticati, F., Albani, M., Andreis, A., Andrieu, T., Anghel, S., Antaluca, E., Antier, K., Appéré, T., Armand, A., Ascione, G., Audureau, Y., Auxepaules, G., Avoscan, T., Baba Aissa, D., Bacci, P., Bǎdescu, O., Baldini, R., Baldo, R., Balestrero, A., Baratoux, D., Barbotin, E., Bardy, M., Basso, S., Bautista, O., Bayle, L. D., Beck, P., Bellitto, R., Belluso, R., Benna, C., Benammi, M., Beneteau, E., Benkhaldoun, Z., Bergamini, P., Bernardi, F., Bertaina, M. E., Bessin, P., Betti, L., Bettonvil, F., Bihel, D., Birnbaum, C., Blagoi, O., Blouri, E., Boacă, I., Boatǎ, R., Bobiet, B., Bonino, R., Boros, K., Bouchet, E., Borgeot, V., Bouchez, E., Boust, D., Boudon, V., Bouman, T., Bourget, P., Brandenburg, S., Bramond, Ph., Braun, E., Bussi, A., Cacault, P., Caillier, B., Calegaro, A., Camargo, J., Caminade, S., Campana, A. P. C., Campbell-Burns, P., Canal-Domingo, R., Carell, O., Carreau, S., Cascone, E., Cattaneo, C., Cauhape, P., Cavier, P., Celestin, S., Cellino, A., Champenois, M., Chennaoui Aoudjehane, H., Chevrier, S., Cholvy, P., Chomier, L., Christou, A., Cricchio, D., Coadou, P., Cocaign, J. Y., Cochard, F., Cointin, S., Colombi, E., Colque Saavedra, J. P., Corp, L., Costa, M., Costard, F., Cottier, M., Cournoyer, P., Coustal, E., Cremonese, G., Cristea, O., Cuzon, J. C., D’Agostino, G., Daiffallah, K., Dǎnescu, C., Dardon, A., Dasse, T., Davadan, C., Debs, V., Defaix, J. P., Deleflie, F., D’Elia, M., De Luca, P., De Maria, P., Deverchère, P., Devillepoix, H., Dias, A., Di Dato, A., Di Luca, R., Dominici, F. M., Drouard, A., Dumont, J. L., Dupouy, P., Duvignac, L., Egal, A., Erasmus, N., Esseiva, N., Ebel, A., Eisengarten, B., Federici, F., Feral, S., Ferrant, G., Ferreol, E., Finitzer, P., Foucault, A., Francois, P., Frîncu, M., Froger, J. L., Gaborit, F., Gagliarducci, V., Galard, J., Gardavot, A., Garmier, M., Garnung, M., Gautier, B., Gendre, B., Gerard, D., Gerardi, A., Godet, J. P., Grandchamps, A., Grouiez, B., Groult, S., Guidetti, D., Giuli, G., Hello, Y., Henry, X., Herbreteau, G., Herpin, M., Hewins, P., Hillairet, J. J., Horak, J., Hueso, R., Huet, E., Huet, S., Hyaumé, F., Interrante, G., Isselin, Y., Jeangeorges, Y., Janeux, P., Jeanneret, P., Jobse, K., Jouin, S., Jouvard, J. M., Joy, K., Julien, J. F., Kacerek, R., Kaire, M., Kempf, M., Krier, C., Kwon, M. K., Lacassagne, L., Lachat, D., Lagain, A., Laisné, E., Lanchares, V., Laskar, J., Lazzarin, M., Leblanc, M., Lebreton, J. P., Lecomte, J., Le Dû, P., Lelong, F., Lera, S., Leoni, J. F., Le-Pichon, A., Le-Poupon, P., Leroy, A., Leto, G., Levansuu, A., Lewin, E., Lienard, A., Licchelli, D., Locatelli, H., Loehle, S., Loizeau, D., Luciani, L., Maignan, M., Manca, F., Mancuso, S., Mandon, E., Mangold, N., Mannucci, F., Maquet, L., Marant, D., Marchal, Y., Marin, J. L., Martin-Brisset, J. C., Martin, D., Mathieu, D., Maury, A., Mespoulet, N., Meyer, F., Meyer, J. Y., Meza, E., Moggi Cecchi, V., Moiroud, J. J., Millan, M., Montesarchio, M., Misiano, A., Molinari, E., Molau, S., Monari, J., Monflier, B., Monkos, A., Montemaggi, M., Monti, G., Moreau, R., Morin, J., Mourgues, R., Mousis, O., Nablanc, C., Nastasi, A., Niacşu, L., Notez, P., Ory, M., Pace, E., Paganelli, M. A., Pagola, A., Pajuelo, M., Palacián, J. F., Pallier, G., Paraschiv, P., Pardini, R., Pavone, M., Pavy, G., Payen, G., Pegoraro, A., Peña-Asensio, E., Perez, L., Pérez-Hoyos, S., Perlerin, V., Peyrot, A., Peth, F., Pic, V., Pietronave, S., Pilger, C., Piquel, M., Pisanu, T., Poppe, M., Portois, L., Prezeau, J. F., Pugno, N., Quantin, C., Quitté, G., Rambaux, N., Ravier, E., Repetti, U., Ribas, S., Richard, C., Richard, D., Rigoni, M., Rivet, J. P., Rizzi, N., Rochain, S., Rojas, J.F., Romeo, M., Rotaru, M., Rotger, M., Rougier, P., Rousselot, P., Rousset, J., Rousseu, D., Rubiera, O., Rudawska, R., Rudelle, J., Ruguet, J.P., Russo, P., Sales, S., Sauzereau, O., Salvati, F., Schieffer, M., Schreiner, D., Scribano, Y., Selvestrel, D., Serra, R., Shengold, L., Shuttleworth, A., Smareglia, R., Sohy, S., Soldi, M., Stanga, R., Steinhausser, A., Strafella, F., Sylla Mbaye, S., Smedley, A. R. D., Tagger, M., Tanga, P., Taricco, C., Teng, J. P., Tercu, J. O., Thizy, O., Thomas, J. P., Tombelli, M., Trangosi, R., Tregon, B., Trivero, P., Tukkers, A., Turcu, V., Umbriaco, G., Unda-Sanzana, E., Vairetti, R., Valenzuela, M., Valente, G., Varennes, G., Vauclair, S., Vergne, J., Verlinden, M., Vidal-Alaiz, M., Vieira-Martins, R., Viel, A., Vîntdevarǎ, D. C., Vinogradoff, V., Volpini, P., Wendling, M., Wilhelm, P., Wohlgemuth, K., Yanguas, P., Zagarella, R., and Zollo, A.
Abstract: Context. Until recently, camera networks designed for monitoring fireballs worldwide were not fully automated, implying that in case of a meteorite fall, the recovery campaign was rarely immediate. This was an important limiting factor as the most fragile – hence precious – meteorites must be recovered rapidly to avoid their alteration. Aims. The Fireball Recovery and InterPlanetary Observation Network (FRIPON) scientific project was designed to overcome this limitation. This network comprises a fully automated camera and radio network deployed over a significant fraction of western Europe and a small fraction of Canada. As of today, it consists of 150 cameras and 25 European radio receivers and covers an area of about 1.5 × 106 km2. Methods. The FRIPON network, fully operational since 2018, has been monitoring meteoroid entries since 2016, thereby allowing the characterization of their dynamical and physical properties. In addition, the level of automation of the network makes it possible to trigger a meteorite recovery campaign only a few hours after it reaches the surface of the Earth. Recovery campaigns are only organized for meteorites with final masses estimated of at least 500 g, which is about one event per year in France. No recovery campaign is organized in the case of smaller final masses on the order of 50 to 100 g, which happens about three times a year; instead, the information is delivered to the local media so that it can reach the inhabitants living in the vicinity of the fall. Results. Nearly 4000 meteoroids have been detected so far and characterized by FRIPON. The distribution of their orbits appears to be bimodal, with a cometary population and a main belt population. Sporadic meteors amount to about 55% of all meteors. A first estimate of the absolute meteoroid flux (mag < –5; meteoroid size ≥~1 cm) amounts to 1250/yr/106 km

202. Thermal properties of slowly rotating asteroids: Results from a targeted survey

Author: Marciniak, A, Ali-Lagoa, V, Muller, T.G, Szakáts, R, Molnár, L, Pál, A, Antonini, P, Barbotin, E, Behrend, R, Bernasconi, L, Butkiewicz-Bak, M, Crippa, R, Duffard, R, Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S, Goncalves, R, Grice, J, Grzeskowiak, I, Hirsch, R, Horbowicz, J, Kaminski, K, Kaminska, M.K, Kim, D.H, Kim, M.J, Konstanciak, I, Kudak, V, Kulczak, P, Maestre, J.L, Manzini, F, Marks, S, Monteiro, F, Ogłoza, W, Oszkiewicz, D, Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R, Sanabria, J.J, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Zejmo, M, Zukowski, K, Marciniak, A, Ali-Lagoa, V, Muller, T.G, Szakáts, R, Molnár, L, Pál, A, Antonini, P, Barbotin, E, Behrend, R, Bernasconi, L, Butkiewicz-Bak, M, Crippa, R, Duffard, R, Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S, Goncalves, R, Grice, J, Grzeskowiak, I, Hirsch, R, Horbowicz, J, Kaminski, K, Kaminska, M.K, Kim, D.H, Kim, M.J, Konstanciak, I, Kudak, V, Kulczak, P, Maestre, J.L, Manzini, F, Marks, S, Monteiro, F, Ogłoza, W, Oszkiewicz, D, Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R, Sanabria, J.J, 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 and 3+−333 and 45+−6030 J m−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.

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

Author: Rozek, A., Lowry, S.C., Rozitis, Benjamin, Green, Simon, Snodgrass, Colin, Weissman, P.R., Fitzsimmons, A., Hicks, M.D., Lawrence, K.J., Duddy, S.R., Wolters, Stephen, Roberts-Borsani, G., Behrend, R., Manzini, F., Rozek, A., Lowry, S.C., Rozitis, Benjamin, Green, Simon, Snodgrass, Colin, Weissman, P.R., Fitzsimmons, A., Hicks, M.D., Lawrence, K.J., Duddy, S.R., Wolters, Stephen, Roberts-Borsani, G., Behrend, R., and Manzini, F.
Abstract: Context: The near-Earth asteroid (1917) Cuyo was subject to radar and lightcurve observations during a close approach in 1989, and observed up until 2008. It was selected as one of our ESO Large Programme targets, aimed at observational detections of the YORP effect through long-term lightcurve monitoring and physical modelling of near-Earth asteroids. Aims: We aimed to constrain physical properties of Cuyo: shape, spin-state, and spectroscopic & thermophysical properties of the surface. Methods: We acquired photometric lightcurves of Cuyo spanning the period between 2010 and 2013, which we combined with published lightcurves from 1989-2008. Our thermal-infrared observations were obtained in 2011. Rotationally-resolved optical spectroscopy data were acquired in 2011 and combined with all available published spectra to investigate any surface material variegation. Results: We developed a convex lightcurve-inversion shape of Cuyo that suggests the presence of an equatorial ridge, typical for an evolved system close to shedding mass due to fast rotation. We determine limits of YORP strength through lightcurve-based spin-state modelling, including both negative and positive acceleration values, between -0.7x10-8 rad day-2 and 1.7x10-8 rad day-2. Thermo-physical modelling with the ATPM provides constraints on the geometric albedo, PV = 0.24 ± 0.07, the effective diameter Deff = 3.15 ± 0.08 km, the thermal inertia, 44 ±- 9 J m-2s-1/2K-1, and a roughness fraction of 0.52 ± 0.26. This enabled a YORP strength prediction of (-6.39 ± 0.96)x10-10 rad day-2. We also see evidence of surface compositional variation. Conclusions: The low value of YORP predicted by means of thermophysical analysis, consistent with the results of the lightcurve s

204. Scaling slowly rotating asteroids with stellar occultations

Author: Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Butkiewicz-Bąk, M., Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D.-H., Kim, M.-J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Könyves-Tóth, R., Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J, Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., Żywica, S., Marciniak, A., Ďurech, J., Choukroun, A., Hanuš, J., Ogłoza, W., Szakáts, R., Molnár, L., Pál, A., Monteiro, F., Frappa, E., Beisker, W., Pavlov, H., Moore, J., Adomavičienė, R., Aikawa, R., Andersson, S., Antonini, P., Argentin, Y., Asai, A., Assoignon, P., Barton, J., Baruffetti, P., Bath, K. L., Behrend, R., Benedyktowicz, L., Bernasconi, L., Biguet, G., Billiani, M., Błażewicz, D., Boninsegna, R., Borkowski, M., Bosch, J., Brazill, S., Bronikowska, M., Bruno, A., Butkiewicz-Bąk, M., Caron, J., Casalnuovo, G., Castellani, J. J., Ceravolo, P., Conjat, M., Delincak, P., Delpau, J., Demeautis, C., Demirkol, A., Dróżdż, M., Duffard, R., Durandet, C., Eisfeldt, D., Evangelista, M., Fauvaud, S., Fauvaud, M., Ferrais, M., Filipek, M., Fini, P., Fukui, K., Gährken, B., Geier, S., George, T., Goffin, B., Golonka, J., Goto, T., Grice, J., Guhl, K., Halíř, K., Hanna, W., Harman, M., Hashimoto, A., Hasubick, W., Higgins, D., Higuchi, M., Hirose, T., Hirsch, R., Hofschulz, O., Horaguchi, T., Horbowicz, J., Ida, M., Ignácz, B., Ishida, M., Isobe, K., Jehin, E., Joachimczyk, B., Jones, A., Juan, J., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kasebe, H., Kattentidt, B., Kim, D.-H., Kim, M.-J., Kitazaki, K., Klotz, A., Komraus, M., Konstanciak, I., Könyves-Tóth, R., Kouno, K., Kowald, E., Krajewski, J., Krannich, G., Kreutzer, A., Kryszczyńska, A., Kubánek, J., Kudak, V., Kugel, F., Kukita, R., Kulczak, P., Lazzaro, D., Licandro, J., Livet, F., Maley, P., Manago, N., Mánek, J., Manna, A., Matsushita, H., Meister, S., Mesquita, W., Messner, S., Michelet, J., Michimani, J., Mieczkowska, I., Morales, N., Motyliński, M., Murawiecka, M., Newman, J., Nikitin, V., Nishimura, M., Oey, J., Oszkiewicz, D., Owada, M., Pakštienė, E., Pawłowski, M., Pereira, W., Perig, V., Perła, J., Pilcher, F., Podlewska-Gaca, E., Polák, J., Polakis, T., Polińska, M., Popowicz, A., Richard, F., Rives, J. J, Rodrigues, T., Rogiński, Ł., Rondón, E., Rottenborn, M., Schäfer, R., Schnabel, C., Schreurs, O., Selva, A., Simon, M., Skiff, B., Skrutskie, M., Skrzypek, J., Sobkowiak, K., Sonbas, E., Sposetti, S., Stuart, P., Szyszka, K., Terakubo, K., Thomas, W., Trela, P., Uchiyama, S., Urbanik, M., Vaudescal, G., Venable, R., Watanabe, Ha., Watanabe, Hi., Winiarski, M., Wróblewski, R., Yamamura, H., Yamashita, M., Yoshihara, H., Zawilski, M., Zelený, P., Żejmo, M., Żukowski, K., and Żywica, S.
Abstract: Context. As evidenced by recent survey results, the majority of asteroids are slow rotators (spin periods longer than 12 h), but lack spin and shape models because of selection bias. This bias is skewing our overall understanding of the spins, shapes, and sizes of asteroids, as well as of their other properties. Also, diameter determinations for large (>60 km) and medium-sized asteroids (between 30 and 60 km) often vary by over 30% for multiple reasons. Aims. Our long-term project is focused on a few tens of slow rotators with periods of up to 60 h. We aim to obtain their full light curves and reconstruct their spins and shapes. We also precisely scale the models, typically with an accuracy of a few percent. Methods. We used wide sets of dense light curves for spin and shape reconstructions via light-curve inversion. Precisely scaling them with thermal data was not possible here because of poor infrared datasets: large bodies tend to saturate in WISE mission detectors. Therefore, we recently also launched a special campaign among stellar occultation observers, both in order to scale these models and to verify the shape solutions, often allowing us to break the mirror pole ambiguity. Results. The presented scheme resulted in shape models for 16 slow rotators, most of them for the first time. Fitting them to chords from stellar occultation timings resolved previous inconsistencies in size determinations. For around half of the targets, this fitting also allowed us to identify a clearly preferred pole solution from the pair of two mirror pole solutions, thus removing the ambiguity inherent to light-curve inversion. We also address the influence of the uncertainty of the shape models on the derived diameters. Conclusions. Overall, our project has already provided reliable models for around 50 slow rotators. Such well-determined and scaled asteroid shapes will, for example, constitute a solid basis fo

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

Author: Rozek, A., Lowry, S.C., Rozitis, Benjamin, Green, Simon, Snodgrass, Colin, Weissman, P.R., Fitzsimmons, A., Hicks, M.D., Lawrence, K.J., Duddy, S.R., Wolters, Stephen, Roberts-Borsani, G., Behrend, R., Manzini, F., Rozek, A., Lowry, S.C., Rozitis, Benjamin, Green, Simon, Snodgrass, Colin, Weissman, P.R., Fitzsimmons, A., Hicks, M.D., Lawrence, K.J., Duddy, S.R., Wolters, Stephen, Roberts-Borsani, G., Behrend, R., and Manzini, F.
Abstract: Context: The near-Earth asteroid (1917) Cuyo was subject to radar and lightcurve observations during a close approach in 1989, and observed up until 2008. It was selected as one of our ESO Large Programme targets, aimed at observational detections of the YORP effect through long-term lightcurve monitoring and physical modelling of near-Earth asteroids. Aims: We aimed to constrain physical properties of Cuyo: shape, spin-state, and spectroscopic & thermophysical properties of the surface. Methods: We acquired photometric lightcurves of Cuyo spanning the period between 2010 and 2013, which we combined with published lightcurves from 1989-2008. Our thermal-infrared observations were obtained in 2011. Rotationally-resolved optical spectroscopy data were acquired in 2011 and combined with all available published spectra to investigate any surface material variegation. Results: We developed a convex lightcurve-inversion shape of Cuyo that suggests the presence of an equatorial ridge, typical for an evolved system close to shedding mass due to fast rotation. We determine limits of YORP strength through lightcurve-based spin-state modelling, including both negative and positive acceleration values, between -0.7x10-8 rad day-2 and 1.7x10-8 rad day-2. Thermo-physical modelling with the ATPM provides constraints on the geometric albedo, PV = 0.24 ± 0.07, the effective diameter Deff = 3.15 ± 0.08 km, the thermal inertia, 44 ±- 9 J m-2s-1/2K-1, and a roughness fraction of 0.52 ± 0.26. This enabled a YORP strength prediction of (-6.39 ± 0.96)x10-10 rad day-2. We also see evidence of surface compositional variation. Conclusions: The low value of YORP predicted by means of thermophysical analysis, consistent with the results of the lightcurve s

206. Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Author: Marciniak, A., Ďurech, J., Alí-Lagoa, V., Ogłoza, W., Szakáts, R., Müller, T. G., Molnár, L., Pál, A., Monteiro, F., Arcoverde, P., Behrend, R., Benkhaldoun, Z., Bernasconi, L., Bosch, J., Brincat, S., Brunetto, L., Butkiewicz - Bąk, M., Del Freo, F., Duffard, R., Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, M., Geier, S., Golonka, J., Grice, J., Hirsch, R., Horbowicz, J., Jehin, E., Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, M.-J., Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, N., Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, E., Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K., Marciniak, A., Ďurech, J., Alí-Lagoa, V., Ogłoza, W., Szakáts, R., Müller, T. G., Molnár, L., Pál, A., Monteiro, F., Arcoverde, P., Behrend, R., Benkhaldoun, Z., Bernasconi, L., Bosch, J., Brincat, S., Brunetto, L., Butkiewicz - Bąk, M., Del Freo, F., Duffard, R., Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, M., Geier, S., Golonka, J., Grice, J., Hirsch, R., Horbowicz, J., Jehin, E., Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M. K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, M.-J., Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, N., Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, E., Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, R., Sanabria, J. J., Santana-Ros, T., Skiff, B., Skrzypek, J., Sobkowiak, K., Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., and Żukowski, K.
Abstract: Context. Recent results for asteroid rotation periods from the TESS mission showed how strongly previous studies have underestimated the number of slow rotators, revealing the importance of studying those targets. For most slowly rotating asteroids (those with P > 12 h), no spin and shape model is available because of observation selection effects. This hampers determination of their thermal parameters and accurate sizes. Also, it is still unclear whether signatures of different surface material properties can be seen in thermal inertia determined from mid-infrared thermal flux fitting. Aims. We continue our campaign in minimising selection effects among main belt asteroids. Our targets are slow rotators with low light-curve amplitudes. Our goal is to provide their scaled spin and shape models together with thermal inertia, albedo, and surface roughness to complete the statistics. Methods. Rich multi-apparition datasets of dense light curves are supplemented with data from Kepler and TESS spacecrafts. In addition to data in the visible range, we also use thermal data from infrared space observatories (mainly IRAS, Akari and WISE) in a combined optimisation process using the Convex Inversion Thermophysical Model. This novel method has so far been applied to only a few targets, and therefore in this work we further validate the method itself. Results. We present the models of 16 slow rotators, including two updated models. All provide good fits to both thermal and visible data.The obtained sizes are on average accurate at the 5% precision level, with diameters found to be in the range from 25 to 145 km. The rotation periods of our targets range from 11 to 59 h, and the thermal inertia covers a wide range of values, from 2 to <400 J m−2 s−1∕2 K−1, not showing any correlation with the period. Conclusions. With this wor

207. VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis

Author: Vernazza, P., Ferrais, M., Jorda, L., Hanuš, J., Carry, B., Marsset, M., Brož, M., Fetick, R., Viikinkoski, M., Marchis, F., Vachier, F., Drouard, A., Fusco, T., Birlan, M., Podlewska-Gaca, E., Rambaux, N., Neveu, M., Bartczak, P., Dudziński, G., Jehin, E., Beck, P., Berthier, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Dumas, C., Ďurech, J., Grice, J., Kaasalainen, M., Kryszczynska, A., Lamy, P., Le Coroller, H., Marciniak, A., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O., Yang, B., Antonini, P., Audejean, M., Aurard, P., Behrend, R., Benkhaldoun, Z., Bosch, J. M., Chapman, A., Dalmon, L., Fauvaud, S., Hamanowa, Hiroko, Hamanowa, Hiromi, His, J., Jones, A., Kim, D.-H., Kim, M.-J., Krajewski, J., Labrevoir, O., Leroy, A., Livet, F., Molina, D., Montaigut, R., Oey, J., Payre, N., Reddy, V., Sabin, P., Sanchez, A. G., Socha, L., Vernazza, P., Ferrais, M., Jorda, L., Hanuš, J., Carry, B., Marsset, M., Brož, M., Fetick, R., Viikinkoski, M., Marchis, F., Vachier, F., Drouard, A., Fusco, T., Birlan, M., Podlewska-Gaca, E., Rambaux, N., Neveu, M., Bartczak, P., Dudziński, G., Jehin, E., Beck, P., Berthier, J., Castillo-Rogez, J., Cipriani, F., Colas, F., Dumas, C., Ďurech, J., Grice, J., Kaasalainen, M., Kryszczynska, A., Lamy, P., Le Coroller, H., Marciniak, A., Michalowski, T., Michel, P., Santana-Ros, T., Tanga, P., Vigan, A., Witasse, O., Yang, B., Antonini, P., Audejean, M., Aurard, P., Behrend, R., Benkhaldoun, Z., Bosch, J. M., Chapman, A., Dalmon, L., Fauvaud, S., Hamanowa, Hiroko, Hamanowa, Hiromi, His, J., Jones, A., Kim, D.-H., Kim, M.-J., Krajewski, J., Labrevoir, O., Leroy, A., Livet, F., Molina, D., Montaigut, R., Oey, J., Payre, N., Reddy, V., Sabin, P., Sanchez, A. G., and Socha, L.
Abstract: Context. Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remained poorly constrained. The improved capabilities of the SPHERE/ZIMPOL instrument have opened new doors into ground-based asteroid exploration. Aims. To constrain the formation and evolution of a representative sample of large asteroids, we conducted a high-angular-resolution imaging survey of 42 large main-belt asteroids with VLT/SPHERE/ZIMPOL. Our asteroid sample comprises 39 bodies with D ≥ 100 km and in particular most D ≥ 200 km main-belt asteroids (20/23). Furthermore, it nicely reflects the compositional diversity present in the main belt as the sampled bodies belong to the following taxonomic classes: A, B, C, Ch/Cgh, E/M/X, K, P/T, S, and V. Methods. The SPHERE/ZIMPOL images were first used to reconstruct the 3D shape of all targets with both the ADAM and MPCD reconstruction methods. We subsequently performed a detailed shape analysis and constrained the density of each target using available mass estimates including our own mass estimates in the case of multiple systems. Results. The analysis of the reconstructed shapes allowed us to identify two families of objects as a function of their diameters, namely “spherical” and “elongated” bodies. A difference in rotation period appears to be the main origin of this bimodality. In addition, all but one object (216 Kleopatra) are located along the Maclaurin sequence with large volatile-rich bodies being the closest to the latter. Our results further reveal that the primaries of most multiple systems possess a rotation period of shorter than 6 h and an elongated shape (c/a ≤ 0.65). Densities in our sample range from ~1.3 g cm−3 (87 Sylvia) to ~4.3 g cm−3 (22 Kalliope). Furthermore, th

208. Physical parameters of selected Gaia mass asteroids

Author: Podlewska-Gaca, E., Marciniak, A., Alí-Lagoa, V., Bartczak, P., Müller, T. G., Szakáts, R., Duffard, R., Molnár, L., Pál, A., Butkiewicz-Bąk, M., Dudziński, G., Dziadura, K., Antonini, P., Asenjo, V., Audejean, M., Benkhaldoun, Z., Behrend, R., Bernasconi, L., Bosch, J. M., Chapman, A., Dintinjana, B., Farkas, A., Ferrais, M., Geier, S., Grice, J., Hirsh, R., Jacquinot, H., Jehin, E., Jones, A., Molina, D., Morales, N., Parley, N., Poncy, R., Roy, R., Santana-Ros, T., Seli, B., Sobkowiak, K., Verebélyi, E., Żukowski, K., Podlewska-Gaca, E., Marciniak, A., Alí-Lagoa, V., Bartczak, P., Müller, T. G., Szakáts, R., Duffard, R., Molnár, L., Pál, A., Butkiewicz-Bąk, M., Dudziński, G., Dziadura, K., Antonini, P., Asenjo, V., Audejean, M., Benkhaldoun, Z., Behrend, R., Bernasconi, L., Bosch, J. M., Chapman, A., Dintinjana, B., Farkas, A., Ferrais, M., Geier, S., Grice, J., Hirsh, R., Jacquinot, H., Jehin, E., Jones, A., Molina, D., Morales, N., Parley, N., Poncy, R., Roy, R., Santana-Ros, T., Seli, B., Sobkowiak, K., Verebélyi, E., 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.

209. Evidence for differentiation of the most primitive small bodies

Author: Carry, B., Vernazza, P., Vachier, F., Neveu, M., Berthier, J., Hanuš, J., Ferrais, M., Jorda, L., Marsset, M., Viikinkoski, M., Bartczak, P., Behrend, R., Benkhaldoun, Z., Birlan, M., Castillo-Rogez, J., Cipriani, F., Colas, F., Drouard, A., Dudziński, G. P., Desmars, J., Dumas, C., Ďurech, J., Fetick, R., Fusco, T., Grice, J., Jehin, E., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marchis, F., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Podlewska-Gaca, E., Rambaux, N., Santana-Ros, T., Storrs, A., Tanga, P., Vigan, A., Warner, B., Wieczorek, M., Witasse, O., Yang, B., Carry, B., Vernazza, P., Vachier, F., Neveu, M., Berthier, J., Hanuš, J., Ferrais, M., Jorda, L., Marsset, M., Viikinkoski, M., Bartczak, P., Behrend, R., Benkhaldoun, Z., Birlan, M., Castillo-Rogez, J., Cipriani, F., Colas, F., Drouard, A., Dudziński, G. P., Desmars, J., Dumas, C., Ďurech, J., Fetick, R., Fusco, T., Grice, J., Jehin, E., Kaasalainen, M., Kryszczynska, A., Lamy, P., Marchis, F., Marciniak, A., Michalowski, T., Michel, P., Pajuelo, M., Podlewska-Gaca, E., Rambaux, N., Santana-Ros, T., Storrs, A., Tanga, P., Vigan, A., Warner, B., Wieczorek, M., Witasse, O., and Yang, B.
Abstract: Context. Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related to the Jupiter Trojans, comets, and small Kuiper belt objects (KBOs). Indeed, the spectral properties of P- and D-type asteroids resemble that of anhydrous cometary dust. Aims. We aim to gain insights into the above classes of bodies by characterizing the internal structure of a large P- and D-type asteroid. Methods. We report high-angular-resolution imaging observations of the P-type asteroid (87) Sylvia with the Very Large Telescope Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument. These images were used to reconstruct the 3D shape of Sylvia. Our images together with those obtained in the past with large ground-based telescopes were used to study the dynamics of its two satellites. We also modeled Sylvia's thermal evolution. Results. The shape of Sylvia appears flattened and elongated (a/b 1.45; a/c 1.84). We derive a volume-equivalent diameter of 271 ± 5 km and a low density of 1378 ± 45 kg m-3. The two satellites orbit Sylvia on circular, equatorial orbits. The oblateness of Sylvia should imply a detectable nodal precession which contrasts with the fully-Keplerian dynamics of its two satellites. This reveals an inhomogeneous internal structure, suggesting that Sylvia is differentiated. Conclusions. Sylvia's low density and differentiated interior can be explained by partial melting and mass redistribution through water percolation. The outer shell should be composed of material similar to interplanetary dust particles (IDPs) and the core should be similar to aqueously altered IDPs or carbonaceous chondrite meteorites such as the Tagish Lake meteorite. Numerical simulations of the thermal evolution of Sylvia show that for a body of such a size, partial melting was

210. FRIPON: a worldwide network to track incoming meteoroids

Author: Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., Gattacceca, J., Jorda, L., Lecubin, J., Marmo, C., Rault, J. L., Vaubaillon, J., Vernazza, P., Yohia, C., Gardiol, D., Nedelcu, A., Poppe, B., Rowe, J., Forcier, M., Koschny, D., Trigo-Rodriguez, J. M., Lamy, H., Behrend, R., Ferrière, L., Barghini, D., Buzzoni, A., Carbognani, A., Di Carlo, M., Di Martino, M., Knapic, C., Londero, E., Pratesi, G., Rasetti, S., Riva, W., Stirpe, G. M., Valsecchi, G. B., Volpicelli, C. A., Zorba, S., Coward, D., Drolshagen, E., Drolshagen, G., Hernandez, O., Jehin, E., Jobin, M., King, A., Nitschelm, C., Ott, T., Sanchez-Lavega, A., Toni, A., Abraham, P., Affaticati, F., Albani, M., Andreis, A., Andrieu, T., Anghel, S., Antaluca, E., Antier, K., Appéré, T., Armand, A., Ascione, G., Audureau, Y., Auxepaules, G., Avoscan, T., Baba Aissa, D., Bacci, P., Bǎdescu, O., Baldini, R., Baldo, R., Balestrero, A., Baratoux, D., Barbotin, E., Bardy, M., Basso, S., Bautista, O., Bayle, L. D., Beck, P., Bellitto, R., Belluso, R., Benna, C., Benammi, M., Beneteau, E., Benkhaldoun, Z., Bergamini, P., Bernardi, F., Bertaina, M. E., Bessin, P., Betti, L., Bettonvil, F., Bihel, D., Birnbaum, C., Blagoi, O., Blouri, E., Boacă, I., Boatǎ, R., Bobiet, B., Bonino, R., Boros, K., Bouchet, E., Borgeot, V., Bouchez, E., Boust, D., Boudon, V., Bouman, T., Bourget, P., Brandenburg, S., Bramond, Ph., Braun, E., Bussi, A., Cacault, P., Caillier, B., Calegaro, A., Camargo, J., Caminade, S., Campana, A. P. C., Campbell-Burns, P., Canal-Domingo, R., Carell, O., Carreau, S., Cascone, E., Cattaneo, C., Cauhape, P., Cavier, P., Celestin, S., Cellino, A., Champenois, M., Chennaoui Aoudjehane, H., Chevrier, S., Cholvy, P., Chomier, L., Christou, A., Cricchio, D., Coadou, P., Cocaign, J. Y., Cochard, F., Cointin, S., Colombi, E., Colque Saavedra, J. P., Corp, L., Costa, M., Costard, F., Cottier, M., Cournoyer, P., Coustal, E., Cremonese, G., Cristea, O., Cuzon, J. C., D’Agostino, G., Daiffallah, K., Dǎnescu, C., Dardon, A., Dasse, T., Davadan, C., Debs, V., Defaix, J. P., Deleflie, F., D’Elia, M., De Luca, P., De Maria, P., Deverchère, P., Devillepoix, H., Dias, A., Di Dato, A., Di Luca, R., Dominici, F. M., Drouard, A., Dumont, J. L., Dupouy, P., Duvignac, L., Egal, A., Erasmus, N., Esseiva, N., Ebel, A., Eisengarten, B., Federici, F., Feral, S., Ferrant, G., Ferreol, E., Finitzer, P., Foucault, A., Francois, P., Frîncu, M., Froger, J. L., Gaborit, F., Gagliarducci, V., Galard, J., Gardavot, A., Garmier, M., Garnung, M., Gautier, B., Gendre, B., Gerard, D., Gerardi, A., Godet, J. P., Grandchamps, A., Grouiez, B., Groult, S., Guidetti, D., Giuli, G., Hello, Y., Henry, X., Herbreteau, G., Herpin, M., Hewins, P., Hillairet, J. J., Horak, J., Hueso, R., Huet, E., Huet, S., Hyaumé, F., Interrante, G., Isselin, Y., Jeangeorges, Y., Janeux, P., Jeanneret, P., Jobse, K., Jouin, S., Jouvard, J. M., Joy, K., Julien, J. F., Kacerek, R., Kaire, M., Kempf, M., Krier, C., Kwon, M. K., Lacassagne, L., Lachat, D., Lagain, A., Laisné, E., Lanchares, V., Laskar, J., Lazzarin, M., Leblanc, M., Lebreton, J. P., Lecomte, J., Le Dû, P., Lelong, F., Lera, S., Leoni, J. F., Le-Pichon, A., Le-Poupon, P., Leroy, A., Leto, G., Levansuu, A., Lewin, E., Lienard, A., Licchelli, D., Locatelli, H., Loehle, S., Loizeau, D., Luciani, L., Maignan, M., Manca, F., Mancuso, S., Mandon, E., Mangold, N., Mannucci, F., Maquet, L., Marant, D., Marchal, Y., Marin, J. L., Martin-Brisset, J. C., Martin, D., Mathieu, D., Maury, A., Mespoulet, N., Meyer, F., Meyer, J. Y., Meza, E., Moggi Cecchi, V., Moiroud, J. J., Millan, M., Montesarchio, M., Misiano, A., Molinari, E., Molau, S., Monari, J., Monflier, B., Monkos, A., Montemaggi, M., Monti, G., Moreau, R., Morin, J., Mourgues, R., Mousis, O., Nablanc, C., Nastasi, A., Niacşu, L., Notez, P., Ory, M., Pace, E., Paganelli, M. A., Pagola, A., Pajuelo, M., Palacián, J. F., Pallier, G., Paraschiv, P., Pardini, R., Pavone, M., Pavy, G., Payen, G., Pegoraro, A., Peña-Asensio, E., Perez, L., Pérez-Hoyos, S., Perlerin, V., Peyrot, A., Peth, F., Pic, V., Pietronave, S., Pilger, C., Piquel, M., Pisanu, T., Poppe, M., Portois, L., Prezeau, J. F., Pugno, N., Quantin, C., Quitté, G., Rambaux, N., Ravier, E., Repetti, U., Ribas, S., Richard, C., Richard, D., Rigoni, M., Rivet, J. P., Rizzi, N., Rochain, S., Rojas, J.F., Romeo, M., Rotaru, M., Rotger, M., Rougier, P., Rousselot, P., Rousset, J., Rousseu, D., Rubiera, O., Rudawska, R., Rudelle, J., Ruguet, J.P., Russo, P., Sales, S., Sauzereau, O., Salvati, F., Schieffer, M., Schreiner, D., Scribano, Y., Selvestrel, D., Serra, R., Shengold, L., Shuttleworth, A., Smareglia, R., Sohy, S., Soldi, M., Stanga, R., Steinhausser, A., Strafella, F., Sylla Mbaye, S., Smedley, A. R. D., Tagger, M., Tanga, P., Taricco, C., Teng, J. P., Tercu, J. O., Thizy, O., Thomas, J. P., Tombelli, M., Trangosi, R., Tregon, B., Trivero, P., Tukkers, A., Turcu, V., Umbriaco, G., Unda-Sanzana, E., Vairetti, R., Valenzuela, M., Valente, G., Varennes, G., Vauclair, S., Vergne, J., Verlinden, M., Vidal-Alaiz, M., Vieira-Martins, R., Viel, A., Vîntdevarǎ, D. C., Vinogradoff, V., Volpini, P., Wendling, M., Wilhelm, P., Wohlgemuth, K., Yanguas, P., Zagarella, R., Zollo, A., Colas, F., Zanda, B., Bouley, S., Jeanne, S., Malgoyre, A., Birlan, M., Blanpain, C., Gattacceca, J., Jorda, L., Lecubin, J., Marmo, C., Rault, J. L., Vaubaillon, J., Vernazza, P., Yohia, C., Gardiol, D., Nedelcu, A., Poppe, B., Rowe, J., Forcier, M., Koschny, D., Trigo-Rodriguez, J. M., Lamy, H., Behrend, R., Ferrière, L., Barghini, D., Buzzoni, A., Carbognani, A., Di Carlo, M., Di Martino, M., Knapic, C., Londero, E., Pratesi, G., Rasetti, S., Riva, W., Stirpe, G. M., Valsecchi, G. B., Volpicelli, C. A., Zorba, S., Coward, D., Drolshagen, E., Drolshagen, G., Hernandez, O., Jehin, E., Jobin, M., King, A., Nitschelm, C., Ott, T., Sanchez-Lavega, A., Toni, A., Abraham, P., Affaticati, F., Albani, M., Andreis, A., Andrieu, T., Anghel, S., Antaluca, E., Antier, K., Appéré, T., Armand, A., Ascione, G., Audureau, Y., Auxepaules, G., Avoscan, T., Baba Aissa, D., Bacci, P., Bǎdescu, O., Baldini, R., Baldo, R., Balestrero, A., Baratoux, D., Barbotin, E., Bardy, M., Basso, S., Bautista, O., Bayle, L. D., Beck, P., Bellitto, R., Belluso, R., Benna, C., Benammi, M., Beneteau, E., Benkhaldoun, Z., Bergamini, P., Bernardi, F., Bertaina, M. E., Bessin, P., Betti, L., Bettonvil, F., Bihel, D., Birnbaum, C., Blagoi, O., Blouri, E., Boacă, I., Boatǎ, R., Bobiet, B., Bonino, R., Boros, K., Bouchet, E., Borgeot, V., Bouchez, E., Boust, D., Boudon, V., Bouman, T., Bourget, P., Brandenburg, S., Bramond, Ph., Braun, E., Bussi, A., Cacault, P., Caillier, B., Calegaro, A., Camargo, J., Caminade, S., Campana, A. P. C., Campbell-Burns, P., Canal-Domingo, R., Carell, O., Carreau, S., Cascone, E., Cattaneo, C., Cauhape, P., Cavier, P., Celestin, S., Cellino, A., Champenois, M., Chennaoui Aoudjehane, H., Chevrier, S., Cholvy, P., Chomier, L., Christou, A., Cricchio, D., Coadou, P., Cocaign, J. Y., Cochard, F., Cointin, S., Colombi, E., Colque Saavedra, J. P., Corp, L., Costa, M., Costard, F., Cottier, M., Cournoyer, P., Coustal, E., Cremonese, G., Cristea, O., Cuzon, J. C., D’Agostino, G., Daiffallah, K., Dǎnescu, C., Dardon, A., Dasse, T., Davadan, C., Debs, V., Defaix, J. P., Deleflie, F., D’Elia, M., De Luca, P., De Maria, P., Deverchère, P., Devillepoix, H., Dias, A., Di Dato, A., Di Luca, R., Dominici, F. M., Drouard, A., Dumont, J. L., Dupouy, P., Duvignac, L., Egal, A., Erasmus, N., Esseiva, N., Ebel, A., Eisengarten, B., Federici, F., Feral, S., Ferrant, G., Ferreol, E., Finitzer, P., Foucault, A., Francois, P., Frîncu, M., Froger, J. L., Gaborit, F., Gagliarducci, V., Galard, J., Gardavot, A., Garmier, M., Garnung, M., Gautier, B., Gendre, B., Gerard, D., Gerardi, A., Godet, J. P., Grandchamps, A., Grouiez, B., Groult, S., Guidetti, D., Giuli, G., Hello, Y., Henry, X., Herbreteau, G., Herpin, M., Hewins, P., Hillairet, J. J., Horak, J., Hueso, R., Huet, E., Huet, S., Hyaumé, F., Interrante, G., Isselin, Y., Jeangeorges, Y., Janeux, P., Jeanneret, P., Jobse, K., Jouin, S., Jouvard, J. M., Joy, K., Julien, J. F., Kacerek, R., Kaire, M., Kempf, M., Krier, C., Kwon, M. K., Lacassagne, L., Lachat, D., Lagain, A., Laisné, E., Lanchares, V., Laskar, J., Lazzarin, M., Leblanc, M., Lebreton, J. P., Lecomte, J., Le Dû, P., Lelong, F., Lera, S., Leoni, J. F., Le-Pichon, A., Le-Poupon, P., Leroy, A., Leto, G., Levansuu, A., Lewin, E., Lienard, A., Licchelli, D., Locatelli, H., Loehle, S., Loizeau, D., Luciani, L., Maignan, M., Manca, F., Mancuso, S., Mandon, E., Mangold, N., Mannucci, F., Maquet, L., Marant, D., Marchal, Y., Marin, J. L., Martin-Brisset, J. C., Martin, D., Mathieu, D., Maury, A., Mespoulet, N., Meyer, F., Meyer, J. Y., Meza, E., Moggi Cecchi, V., Moiroud, J. J., Millan, M., Montesarchio, M., Misiano, A., Molinari, E., Molau, S., Monari, J., Monflier, B., Monkos, A., Montemaggi, M., Monti, G., Moreau, R., Morin, J., Mourgues, R., Mousis, O., Nablanc, C., Nastasi, A., Niacşu, L., Notez, P., Ory, M., Pace, E., Paganelli, M. A., Pagola, A., Pajuelo, M., Palacián, J. F., Pallier, G., Paraschiv, P., Pardini, R., Pavone, M., Pavy, G., Payen, G., Pegoraro, A., Peña-Asensio, E., Perez, L., Pérez-Hoyos, S., Perlerin, V., Peyrot, A., Peth, F., Pic, V., Pietronave, S., Pilger, C., Piquel, M., Pisanu, T., Poppe, M., Portois, L., Prezeau, J. F., Pugno, N., Quantin, C., Quitté, G., Rambaux, N., Ravier, E., Repetti, U., Ribas, S., Richard, C., Richard, D., Rigoni, M., Rivet, J. P., Rizzi, N., Rochain, S., Rojas, J.F., Romeo, M., Rotaru, M., Rotger, M., Rougier, P., Rousselot, P., Rousset, J., Rousseu, D., Rubiera, O., Rudawska, R., Rudelle, J., Ruguet, J.P., Russo, P., Sales, S., Sauzereau, O., Salvati, F., Schieffer, M., Schreiner, D., Scribano, Y., Selvestrel, D., Serra, R., Shengold, L., Shuttleworth, A., Smareglia, R., Sohy, S., Soldi, M., Stanga, R., Steinhausser, A., Strafella, F., Sylla Mbaye, S., Smedley, A. R. D., Tagger, M., Tanga, P., Taricco, C., Teng, J. P., Tercu, J. O., Thizy, O., Thomas, J. P., Tombelli, M., Trangosi, R., Tregon, B., Trivero, P., Tukkers, A., Turcu, V., Umbriaco, G., Unda-Sanzana, E., Vairetti, R., Valenzuela, M., Valente, G., Varennes, G., Vauclair, S., Vergne, J., Verlinden, M., Vidal-Alaiz, M., Vieira-Martins, R., Viel, A., Vîntdevarǎ, D. C., Vinogradoff, V., Volpini, P., Wendling, M., Wilhelm, P., Wohlgemuth, K., Yanguas, P., Zagarella, R., and Zollo, A.
Abstract: Context. Until recently, camera networks designed for monitoring fireballs worldwide were not fully automated, implying that in case of a meteorite fall, the recovery campaign was rarely immediate. This was an important limiting factor as the most fragile – hence precious – meteorites must be recovered rapidly to avoid their alteration. Aims. The Fireball Recovery and InterPlanetary Observation Network (FRIPON) scientific project was designed to overcome this limitation. This network comprises a fully automated camera and radio network deployed over a significant fraction of western Europe and a small fraction of Canada. As of today, it consists of 150 cameras and 25 European radio receivers and covers an area of about 1.5 × 106 km2. Methods. The FRIPON network, fully operational since 2018, has been monitoring meteoroid entries since 2016, thereby allowing the characterization of their dynamical and physical properties. In addition, the level of automation of the network makes it possible to trigger a meteorite recovery campaign only a few hours after it reaches the surface of the Earth. Recovery campaigns are only organized for meteorites with final masses estimated of at least 500 g, which is about one event per year in France. No recovery campaign is organized in the case of smaller final masses on the order of 50 to 100 g, which happens about three times a year; instead, the information is delivered to the local media so that it can reach the inhabitants living in the vicinity of the fall. Results. Nearly 4000 meteoroids have been detected so far and characterized by FRIPON. The distribution of their orbits appears to be bimodal, with a cometary population and a main belt population. Sporadic meteors amount to about 55% of all meteors. A first estimate of the absolute meteoroid flux (mag < –5; meteoroid size ≥~1 cm) amounts to 1250/yr/106 km

211. Thermal properties of slowly rotating asteroids: Results from a targeted survey

Author: Marciniak, A, Ali-Lagoa, V, Muller, T.G, Szakáts, R, Molnár, L, Pál, A, Antonini, P, Barbotin, E, Behrend, R, Bernasconi, L, Butkiewicz-Bak, M, Crippa, R, Duffard, R, Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S, Marciniak, A, Ali-Lagoa, V, Muller, T.G, Szakáts, R, Molnár, L, Pál, A, Antonini, P, Barbotin, E, Behrend, R, Bernasconi, L, Butkiewicz-Bak, M, Crippa, R, Duffard, R, Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, and Geier, S
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 and 3+−333 and 45+−6030 J m−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.

212. The non-convex shape of (234) Barbara, the first Barbarian

Author: Tanga, P., Carry, B., Colas, F., Delbo, M., Matter, A., Hanuš, J., Alí Lagoa, V., Andrei, A. H., Assafin, M., Audejean, M., Behrend, R., Camargo, J. I. B., Carbognani, A., Cedrés Reyes, M., Conjat, M., Cornero, N., Coward, D., Crippa, R., de Ferra Fantin, E., Devogéle, M., Dubos, G., Frappa, E., Gillon, M., Hamanowa, H., Jehin, E., Klotz, A., Kryszczyńska, A., Lecacheux, J., Leroy, A., Manfroid, J., Manzini, F., Maquet, L., Morelle, E., Mottola, S., Polińska, M., Roy, R., Todd, M., Vachier, F., Vera Hernández, C., Wiggins, P., Tanga, P., Carry, B., Colas, F., Delbo, M., Matter, A., Hanuš, J., Alí Lagoa, V., Andrei, A. H., Assafin, M., Audejean, M., Behrend, R., Camargo, J. I. B., Carbognani, A., Cedrés Reyes, M., Conjat, M., Cornero, N., Coward, D., Crippa, R., de Ferra Fantin, E., Devogéle, M., Dubos, G., Frappa, E., Gillon, M., Hamanowa, H., Jehin, E., Klotz, A., Kryszczyńska, A., Lecacheux, J., Leroy, A., Manfroid, J., Manzini, F., Maquet, L., Morelle, E., Mottola, S., Polińska, M., Roy, R., Todd, M., Vachier, F., Vera Hernández, C., and Wiggins, P.
Abstract: Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever found in the Solar system. It exhibits several peculiar features, most notably its polarimetric behaviour. In recent years other objects sharing the same property (collectively known as ‘Barbarians') have been discovered. Interferometric observations in the mid-infrared with the ESO VLTI (Very Large Telescope Interferometer) suggested that (234) Barbara might have a bi-lobated shape or even a large companion satellite. We use a large set of 57 optical light curves acquired between 1979 and 2014, together with the timings of two stellar occultations in 2009, to determine the rotation period, spin-vector coordinates, and 3-D shape of (234) Barbara, using two different shape reconstruction algorithms. By using the light curves combined to the results obtained from stellar occultations, we are able to show that the shape of (234) Barbara exhibits large concave areas. Possible links of the shape to the polarimetric properties and the object evolution are discussed. We also show that VLTI data can be modelled without the presence of a satellite

213. Die spontane Leberruptur bei Eklampsie

Author: Seeler, M., primary, Behrend, R., additional, Mörl, F., additional, and Körner, J., additional
Published: 1987
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214. Diagnostik von Meningiomen der dritten Stirnhirnwindung

Author: Behrend, R. Ch., primary
Published: 1962
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215. Neue Behandlungsmethoden in der neurologischen Rehabilitation*

Author: Behrend, R. Ch., primary
Published: 1968
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216. �ber Virulenzschwankungen des Poliomyelitis Lansing-Virus bei fortlaufenden M�usepassagen

Author: Behrend, R. Ch., primary and Schulz, H. W., additional
Published: 1950
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217. Ueber Dimethylsulfaminsäure

Author: Behrend, R., primary
Published: 1882
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218. Ueber die Einwirkung von Phenylisocyanat auf Aminocrotonsäureester

Author: Behrend, R., primary and Meyer, Ferd. C., additional
Published: 1900
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219. Ueber die Monobenzoylderivate der beiden Dibenzylhydrazine

Author: Eberhardt, G., primary and Behrend, R., additional
Published: 1903
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220. Über Erfahrungen mit neueren Mitteln zur Behandlung des Parkinsonismus

Author: Behrend, R. Ch., primary
Published: 1952
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221. Charles Lefebvre: Leçons d'introduction à l'histoire du droit matrimonial français

Author: Behrend, R., primary
Published: 1902
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222. Zur Prophylaxe und Therapie der Poliomyelitis

Author: Pette, H., primary and Behrend, R. Ch., additional
Published: 1950
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223. Ueber substituirte Sulfamide und Amidosulfurylchloride

Author: Behrend, R., primary
Published: 1882
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224. Henri Beaune: Nouveaux fragments de droit et d'histoire

Author: Behrend, R., primary
Published: 1902
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225. Investigations on periphytic algae: comparing distinct years in the presence and absence of submerged macrophytes.

Author: Neif, E. M., Behrend, R. D. L., and odrigues, L.
Subjects: ALGAE, MACROPHYTES, HABITATS, AQUATIC ecology, SPECIES diversity
Published: 2014
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226. Spin states of asteroids in the Eos collisional family.

Author: Hanuš, J., Delbo’, M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., and Esseiva, N.
Subjects: *ROTATION of asteroids, *CATASTROPHISM, *THERMOPHYSICAL properties, *ASTRONOMICAL photometry, *NEAR infrared spectroscopy
Abstract: Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. We aim to increase the number of asteroid shape models and rotation states within the Eos collision family, as well as to revise previously published shape models from the literature. Such results can be used to constrain theoretical collisional and evolution models of the family, or to estimate other physical parameters by a thermophysical modeling of the thermal infrared data. We use all available disk-integrated optical data (i.e., classical dense-in-time photometry obtained from public databases and through a large collaboration network as well as sparse-in-time individual measurements from a few sky surveys) as input for the convex inversion method, and derive 3D shape models of asteroids together with their rotation periods and orientations of rotation axes. We present updated shape models for 15 asteroids and new shape model determinations for 16 asteroids. Together with the already published models from the publicly available DAMIT database, we compiled a sample of 56 Eos family members with known shape models that we used in our analysis of physical properties within the family. Rotation states of asteroids smaller than  ∼ 20 km are heavily influenced by the YORP effect, whilst the large objects more or less retained their rotation state properties since the family creation. Moreover, we also present a shape model and bulk density of asteroid (423) Diotima, an interloper in the Eos family, based on the disk-resolved data obtained by the Near InfraRed Camera (Nirc2) mounted on the W.M. Keck II telescope. [ABSTRACT FROM AUTHOR]
Published: 2018
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227. The small binary asteroid (939) Isberga.

Author: Carry, B., Matter, A., Scheirich, P., Pravec, P., Molnar, L., Mottola, S., Carbognani, A., Jehin, E., Marciniak, A., Binzel, R.P., DeMeo, F.E., Birlan, M., Delbo, M., Barbotin, E., Behrend, R., Bonnardeau, M., Colas, F., Farissier, P., Fauvaud, M., and Fauvaud, S.
Subjects: *ASTEROIDS, *INFRARED spectroscopy, *ASTRONOMICAL observations, *LIGHT curves, *INTERFEROMETERS, *PLANETARY orbits
Abstract: In understanding the composition and internal structure of asteroids, their density is perhaps the most diagnostic quantity. We aim here at characterizing the surface composition, mutual orbit, size, mass, and density of the small main-belt binary asteroid (939) Isberga. For that, we conduct a suite of multi-technique observations, including optical lightcurves over many epochs, near-infrared spectroscopy, and interferometry in the thermal infrared. We develop a simple geometric model of binary systems to analyze the interferometric data in combination with the results of the lightcurve modeling. From spectroscopy, we classify Ibserga as a Sq-type asteroid, consistent with the albedo of 0.14 - 0.06 + 0.09 (all uncertainties are reported as 3- σ range) we determine (average albedo of S-types is 0.197 ± 0.153, see Pravec et al. (Pravec et al. [2012]. Icarus 221, 365–387). Lightcurve analysis reveals that the mutual orbit has a period of 26.6304 ± 0.0001 h, is close to circular (eccentricity lower than 0.1), and has pole coordinates within 7° of (225°, +86°) in Ecliptic J2000, implying a low obliquity of 1.5 - 1.5 + 6.0 deg . The combined analysis of lightcurves and interferometric data allows us to determine the dimension of the system and we find volume-equivalent diameters of 12.4 - 1.2 + 2.5 km and 3.6 - 0.3 + 0.7 km for Isberga and its satellite, circling each other on a 33 km wide orbit. Their density is assumed equal and found to be 2.91 - 2.01 + 1.72 g cm - 3 , lower than that of the associated ordinary chondrite meteorites, suggesting the presence of some macroporosity, but typical of S-types of the same size range (Carry [2012]. Planet. Space Sci. 73, 98–118). The present study is the first direct measurement of the size of a small main-belt binary. Although the interferometric observations of Isberga are at the edge of MIDI capabilities, the method described here is applicable to others suites of instruments (e.g., LBT, ALMA). [ABSTRACT FROM AUTHOR]
Published: 2015
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228. Feeling the responsibility: Exploring the emotional experiences of final-year medical students when carrying out clinical tasks.

Author: Alexander M, Behrend R, Franz A, and Peters H
Abstract: Purpose: The concept of Entrustable Professional Activities (EPA) is increasingly used to operationalize learning in the clinical workplace, yet little is known about the emotions of learners feeling the responsibility when carrying out professional tasks., Methods: We explored the emotional experiences of medical students in their final clerkship year when performing clinical tasks. We used an online reflective diary. Text entries were analysed using inductive-deductive content analysis with reference to the EPA framework and the control-value theory of achievement emotions., Results: Students described a wide range of emotions related to carrying out various clinical tasks. They reported positive-activating emotions, ranging from enjoyment to relaxation, and negative-deactivating emotions, ranging from anxiety to boredom. Emotions varied across individual students and were related to the characteristics of a task, an increasing level of autonomy, the students' perceived ability to perform a task and the level of supervision provided., Discussion: Emotions are widely present and impact on the workplace learning of medical students which is related to key elements of the EPA framework. Supervisors play a key role in eliciting positive-activating emotions and the motivation to learn by providing a level of supervision and guidance appropriate to the students' perceived ability to perform the task.
Published: 2024
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229. Development of a project for interprofessional collaboration between medical and pharmacy students to improve medication safety in polypharmacy (PILLE).

Author: Gehrke-Beck S, Petersen M, Herrmann WJ, Zimmermann N, Daub E, Seeger J, Schulz J, Czimmeck C, Lauterbach N, Peters H, Kloft C, Schulz M, Siebenbrodt I, and Behrend R
Subjects: Humans, Polypharmacy, Curriculum, Learning, Students, Pharmacy, Students, Medical
Abstract: Aim: Interprofessional collaboration is particularly relevant to patient safety in outpatient care with polypharmacy. The educational project "PILLE" is meant to give medical and pharmacy students an understanding of the roles and competencies needed for cooperation in the provision of healthcare and to enable interprofessional learning., Method: The curriculum is aimed at pharmacy and medical students and was developed in six steps according to the Kern cycle. It is comprised of an interprofessional seminar, a joint practical training in a simulated pharmacy, and a tandem job shadowing at a primary care practice. The project was implemented in three stages due to the pandemic: The interprofessional online seminar based on the ICAP model and the digital inverted classroom was held in the 2020 winter semester; the interprofessional practical training was added in the 2021 summer semester; and the interprofessional tandem job shadowing at a primary care practice in the 2021 winter semester. Attitudes toward interprofessional learning, among other things, was measured in the evaluation using the SPICE-2D questionnaire (Student Perceptions of Physician-Pharmacist Interprofessional Clinical Education)., Results: In the first three semesters, a total of 105 students (46 pharmacy, 59 medicine) participated in the project, of which 78 participated in the evaluation (74% response rate). The students stated, in particular, that they had learned about the competencies and roles of the other profession and desired additional and more specific preparatory materials for the course sessions. The SPICE-2D questionnaire showed high values for both groups of students already in the pre-survey and these increased further as a result of the project., Conclusion: Joint case-based learning could be implemented under the conditions imposed by the pandemic. Online teaching is a low-threshold means to enable interprofessional exchange., Competing Interests: The authors declare that they have no competing interests., (Copyright © 2023 Gehrke-Beck et al.)
Published: 2023
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230. [Development of Interprofessional Learning Outcomes for Health Professions at Charité - Universitätsmedizin Berlin - A Delphi-Study].

Author: Behrend R, Herinek D, Kienle R, Arnold F, and Peters H
Subjects: Berlin, Germany, Health Personnel, Humans, Health Occupations, Interprofessional Relations
Abstract: Objectives: The impact of interprofessional (IP) collaboration on patient-centered care is constantly increasing. Health professional students need to be prepared for interprofessional collaboration in the workplace. The Charité - Universitätsmedizin Berlin aims to establish a common understanding of interprofessionalism in order to further develop interprofessional education. The aim of this study was to develop a framework with IP learning outcomes for the local context., Materials and Methods: IP training goals were developed and validated in a systematic, 2-step process. First, a working group (n=12) developed a draft of IP outcomes using the nominal group technique. This draft was validated with a Delphi study in 2 rounds with IP faculty members and students (n=17)., Results: A framework of IP learning outcomes was developed and validated. It included an introductory text and 4 competency domains. Each domain defined a title, a description and operationalized learning outcomes for the areas of knowledge, skills and attitude., Conclusions: The framework resulting from the development and validation of IP learning outcomes at the Charité - Universitätsmedizin Berlin can be used as a basis for the coordinated implementation of IPE at the faculty. This framework may serve other faculties as a basis for their own development of interprofessional education., Competing Interests: Die Autorinnen/Autoren geben an, dass kein Interessenkonflikt besteht., (Thieme. All rights reserved.)
Published: 2022
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231. Position paper of the GMA Committee Interprofessional Education in the Health Professions - current status and outlook.

Author: Kaap-Fröhlich S, Ulrich G, Wershofen B, Ahles J, Behrend R, Handgraaf M, Herinek D, Mitzkat A, Oberhauser H, Scherer T, Schlicker A, Straub C, Waury Eichler R, Wesselborg B, Witti M, Huber M, and Bode SFN
Subjects: Curriculum, Health Occupations, Humans, Pandemics, COVID-19 epidemiology, Interprofessional Education
Abstract: In the wake of local initiatives and developmental funding programs, interprofessionality is now included in national curricula in the German-speaking countries. Based on the 3P model (presage, process, product), this position paper presents the development of interprofessional education in recent years in Germany, Austria and Switzerland and places it in an international context. Core aspects as legal frameworks, including amendments to occupational regulations as well as the formation of networks and faculty development are basic requirements for interprofessional education. New topics and educational settings take shape in the process of interprofessional education: patient perspectives and teaching formats, such as online courses, become more important or are newly established. The influence of the COVID-19 pandemic on interprofessional education is explored as well. Among many new interprofessional courses, particularly the implementation of interprofessional training wards in Germany and Switzerland are positive examples of successful interprofessional education. The objective of interprofessional education continues to be the acquisition of interprofessional competencies. The main focus is now centered on evaluating this educational format and testing for the corresponding competencies. In the future, more capacities will be required for interprofessional continuing education and post-graduate education. Structured research programs are essential to ascertain the effects of interprofessional education in the German-speaking countries. In this position paper the GMA committee on interprofessional education encourages further advancement of this topic and expresses the aim to continue cooperating with other networks to strengthen and intensify interprofessional education and collaboration in healthcare., Competing Interests: The authors declare that they have no competing interests., (Copyright © 2022 Kaap-Fröhlich et al.)
Published: 2022
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232. How do medical students learn conceptual knowledge? High-, moderate- and low-utility learning techniques and perceived learning difficulties.

Author: Franz A, Oberst S, Peters H, Berger R, and Behrend R
Subjects: Adult, Clinical Competence, Curriculum, Female, Humans, Learning, Male, Young Adult, Education, Medical, Undergraduate methods, Students, Medical
Abstract: Background: Acquiring medical knowledge is a key competency for medical students and a lifelong requirement for physicians. Learning techniques can improve academic success and help students cope with stressors. To support students' learning process medical faculties should know about learning techniques. The purpose of this study is to analyse the preferred learning techniques of female and male as well as junior and senior medical students and how these learning techniques are related to perceived learning difficulties., Methods: In 2019, we conducted an online survey with students of the undergraduate, competency-based curriculum of medicine at Charité - Universitätsmedizin Berlin. We chose ten learning techniques of high, moderate and low utility according to Dunlosky et al. (2013) and we asked medical students to rate their preferred usage of those techniques using a 5-point Likert scale. We applied t-tests to show differences in usage between female and male as well as junior and senior learners. Additionally, we conducted a multiple regression analysis to explore the predictive power of learning techniques regarding perceived difficulties., Results: A total of 730 medical students (488 women, 242 men, M age = 24.85, SD = 4.49) use three techniques the most: 'highlighting' (low utility), 'self-explanation' (moderate utility) and 'practice testing' (high utility). Female students showed a significantly higher usage of low-utility learning techniques (t(404.24) = -7.13, p < .001) and a higher usage of high-utility learning techniques (t(728) = -2.50, p < .05) than male students (M = 3.55, SD = .95). Compared to junior students (second to sixth semester; M = 3.65, SD = .71), senior students (seventh semester to final clerkship year; M = 3.52, SD = .73) showed a lower use of low-utility learning techniques (t(603) = 2.15, p < .05). Usage of low-utility techniques is related to more difficulties (β = .08, t(724) = 2.13, p < .05). Usage of moderate-utility techniques is related to less learning difficulties (β = -.13, t(599) = -3.21, p < .01)., Conclusions: Students use a wide range of low-, moderate- and high-utility learning techniques. The use of learning techniques has an influence on the difficulties perceived by students. Therefore, they could benefit from knowing about and using high-utility learning techniques to facilitate their learning. Faculties should inform their students about effective learning and introduce them to useful learning techniques., (© 2022. The Author(s).)
Published: 2022
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233. Medical students' ratings of the relevance and actual implementation of interprofessional education and preferences for teaching formats: comparison by gender and prior education.

Author: Behrend R, Czeskleba A, Rollinger T, Petzold M, Roa Romero Y, Raspe R, Maaz A, and Peters H
Subjects: Adult, Attitude of Health Personnel, Berlin, Curriculum standards, Curriculum statistics & numerical data, Education, Medical, Undergraduate methods, Education, Medical, Undergraduate statistics & numerical data, Educational Status, Female, Humans, Male, Sex Factors, Students, Medical statistics & numerical data, Surveys and Questionnaires, Teaching psychology, Teaching statistics & numerical data, Education, Medical, Undergraduate standards, Interprofessional Relations, Students, Medical psychology, Teaching standards
Abstract: Objectives: Interprofessional education is becoming increasingly important for collaboration in patient care. In the national context, there are few empirical studies on the assessment of medical students as important stakeholders in their education. Method: Students (N=2,974) participated in a semester-wide online evaluation of the modular curriculum of medicine at the Charité Berlin. Socio-demographic data (including gender, completion of prior education/studies), assessments of the relevance and extent of interprofessional collaboration and preferences for interprofessional education in various teaching formats were collected. Results: In total, data from 1,019 students were included in the evaluation. The relevance of interprofessional collaboration was considered high by medical students. Female students rated the relevance higher than male students. The completion of pre-education (vocational training or study) had no additional influence. The actual implementation of interprofessional education was rated equally low by female and male students. Medical students rated patient-centred, interactive small group formats as particularly suitable for interprofessional education. There were no gender differences, but the effect was more pronounced among students with vocational training. Conclusion: The assessments of female and male students show a large difference between the perceived relevance and the actual implementation of interprofessional collaboration in the modular curriculum of medicine. This study provides an empirical basis for the actual implementation of interprofessional collaboration and students' views on suitable teaching formats for interprofessional education., Competing Interests: The authors declare that they have no competing interests., (Copyright © 2020 Behrend et al.)
Published: 2020
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234. Student participation in the development of interprofessional education courses: Perceptions and experiences of faculty members and the students.

Author: Behrend R, Franz A, Czeskleba A, Maaz A, and Peters H
Subjects: Cooperative Behavior, Focus Groups, Germany, Health Education methods, Humans, Attitude of Health Personnel, Faculty psychology, Health Occupations education, Interprofessional Relations, Program Development methods, Students, Health Occupations psychology
Abstract: Introduction: Student participation has shown positive effects on the curriculum development process for a single health profession. This qualitative study explores faculty members' and students' perceptions and experiences regarding student participation in interprofessional course development. Methods: Interprofessional courses were developed and implemented by interprofessional teams of faculty members and students. Two focus group discussions were carried out: one with faculty members and one with students. Results: Students contributed to both the process and the results of interprofessional course development in a complementary manner. Student participation was facilitated via motivation for and through work on interprofessional education, a balance between clarity on tasks and students' autonomy, and a low-hierarchy team atmosphere. Students developed professionally, and faculty members saw them as future ambassadors for interprofessional collaboration. Conclusions: This study provides multiple qualitative evidence for a positive, complementary role of student participation in interprofessional course development. A number of factors were identified that should be nurtured to facilitate this effect. Our findings may stimulate and guide other schools to actively involve students in the development of interprofessional education.
Published: 2019
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235. Heterogeneous learning cultures in interprofessional education: a teacher training.

Author: Behrend R, Mette M, Partecke M, Reichel K, and Wershofen B
Subjects: Education trends, Faculty psychology, Feedback, Humans, Interprofessional Relations, Learning, Culture, Education methods, Faculty education
Abstract: Aim: Due to the political demand for the integration of interprofessional (IP) learning into the undergraduate education of health professionals, teachers now have to create and perform IP courses. The IP and thus heterogeneous learning groups pose a special challenge. The presented project aimed at designing a workshop training to support teachers to reflect on heterogeneous learning cultures and to prepare for IP teaching. Methods: The workshop concept was developed in using the Plan-Do-Check-Act (PDCA) cycle and included planning, several rounds of testing and the evaluation of the concept. All planning steps in the development of the workshop concept followed the principles of cooperative learning. The concept evolved in an iterative process based on participants' feedback and facilitators' self-reflection. Results: The resulting workshop concept includes theoretical input as well as discussion, teamwork and participants' self-reflection. The workshop's core element is the work assignment to develop an IP teaching session considering different learning cultures. Work results and experiences are discussed with the entire group and required skills of IP teachers are identified. Conclusion: The subjective feedback of participants regarding their satisfaction and knowledge gained indicates that the workshop concept is well received. The joint planning of an IP teaching session highlights particularities resulting from heterogeneous learning cultures. These should be utilized in IP education to better prepare learners for IP cooperation in the workplace., Competing Interests: The authors declare that they have no competing interests.
Published: 2019
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236. The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation.

Author: Ortiz JL, Santos-Sanz P, Sicardy B, Benedetti-Rossi G, Bérard D, Morales N, Duffard R, Braga-Ribas F, Hopp U, Ries C, Nascimbeni V, Marzari F, Granata V, Pál A, Kiss C, Pribulla T, Komžík R, Hornoch K, Pravec P, Bacci P, Maestripieri M, Nerli L, Mazzei L, Bachini M, Martinelli F, Succi G, Ciabattari F, Mikuz H, Carbognani A, Gaehrken B, Mottola S, Hellmich S, Rommel FL, Fernández-Valenzuela E, Bagatin AC, Cikota S, Cikota A, Lecacheux J, Vieira-Martins R, Camargo JIB, Assafin M, Colas F, Behrend R, Desmars J, Meza E, Alvarez-Candal A, Beisker W, Gomes-Junior AR, Morgado BE, Roques F, Vachier F, Berthier J, Mueller TG, Madiedo JM, Unsalan O, Sonbas E, Karaman N, Erece O, Koseoglu DT, Ozisik T, Kalkan S, Guney Y, Niaei MS, Satir O, Yesilyaprak C, Puskullu C, Kabas A, Demircan O, Alikakos J, Charmandaris V, Leto G, Ohlert J, Christille JM, Szakáts R, Farkas AT, Varga-Verebélyi E, Marton G, Marciniak A, Bartczak P, Santana-Ros T, Butkiewicz-Bąk M, Dudziński G, Alí-Lagoa V, Gazeas K, Tzouganatos L, Paschalis N, Tsamis V, Sánchez-Lavega A, Pérez-Hoyos S, Hueso R, Guirado JC, Peris V, and Iglesias-Marzoa R
Abstract: Haumea-one of the four known trans-Neptunian dwarf planets-is a very elongated and rapidly rotating body. In contrast to other dwarf planets, its size, shape, albedo and density are not well constrained. The Centaur Chariklo was the first body other than a giant planet known to have a ring system, and the Centaur Chiron was later found to possess something similar to Chariklo's rings. Here we report observations from multiple Earth-based observatories of Haumea passing in front of a distant star (a multi-chord stellar occultation). Secondary events observed around the main body of Haumea are consistent with the presence of a ring with an opacity of 0.5, width of 70 kilometres and radius of about 2,287 kilometres. The ring is coplanar with both Haumea's equator and the orbit of its satellite Hi'iaka. The radius of the ring places it close to the 3:1 mean-motion resonance with Haumea's spin period-that is, Haumea rotates three times on its axis in the time that a ring particle completes one revolution. The occultation by the main body provides an instantaneous elliptical projected shape with axes of about 1,704 kilometres and 1,138 kilometres. Combined with rotational light curves, the occultation constrains the three-dimensional orientation of Haumea and its triaxial shape, which is inconsistent with a homogeneous body in hydrostatic equilibrium. Haumea's largest axis is at least 2,322 kilometres, larger than previously thought, implying an upper limit for its density of 1,885 kilograms per cubic metre and a geometric albedo of 0.51, both smaller than previous estimates. In addition, this estimate of the density of Haumea is closer to that of Pluto than are previous estimates, in line with expectations. No global nitrogen- or methane-dominated atmosphere was detected.
Published: 2017
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237. Berlin in Motion: Interprofessional teaching and learning for students in the fields of medicine, occupational therapy, physiotherapy and nursing (INTER-M-E-P-P).

Author: Bohrer A, Heinze C, Höppner H, Behrend R, Czakert J, Hitzblech T, Kaufmann I, Maaz A, Räbiger J, and Peters H
Subjects: Berlin, Humans, Physical Therapy Modalities, Students, Education, Nursing, Interprofessional Relations, Occupational Therapy education
Abstract: Aim: The Berlin project "Interprofessional teaching and learning in medicine, occupational therapy, physiotherapy and nursing" (INTER-M-E-P-P) pursues the goal of developing and testing interprofessional courses in an exemplary manner, and then implement these into their regular study programs., Method: Under the direction of a steering committee of the participating institutions, professions and status groups, interprofessional courses were designed, carried out and evaluated. Specific to this project are the participation of students in the steering committee, and the accompanying of external supervision. The evaluation integrates the perspectives of all project participants, and combines quantitative and qualitative methods., Results: INTER-M-E-P-P established cooperative structures between the participating universities and programs. Three courses were designed, taught and evaluated in an interprofessional manner. The various curricula, organizational patterns and locations of the study paths led to a great need for resources in regard to planning and implementation. This process can be made difficult by any stereotypes or preconceptions inherent to those doing the planning; however, under external supervision, the individual professional viewpoints can still be broadened and enriched., Conclusion: A sustainable implementation of interprofessional education into the curricula of health science study programs is currently complicated by barriers such as different geographical locations and differing university regulations concerning study and testing. Implementation will require long-term support at the university as well as at political levels.
Published: 2016
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238. Albedo and atmospheric constraints of dwarf planet Makemake from a stellar occultation.

Author: Ortiz JL, Sicardy B, Braga-Ribas F, Alvarez-Candal A, Lellouch E, Duffard R, Pinilla-Alonso N, Ivanov VD, Littlefair SP, Camargo JI, Assafin M, Unda-Sanzana E, Jehin E, Morales N, Tancredi G, Gil-Hutton R, de la Cueva I, Colque JP, Da Silva Neto DN, Manfroid J, Thirouin A, Gutiérrez PJ, Lecacheux J, Gillon M, Maury A, Colas F, Licandro J, Mueller T, Jacques C, Weaver D, Milone A, Salvo R, Bruzzone S, Organero F, Behrend R, Roland S, Vieira-Martins R, Widemann T, Roques F, Santos-Sanz P, Hestroffer D, Dhillon VS, Marsh TR, Harlingten C, Bagatin AC, Alonso ML, Ortiz M, Colazo C, Lima HJ, Oliveira AS, Kerber LO, Smiljanic R, Pimentel E, Giacchini B, Cacella P, and Emilio M
Abstract: Pluto and Eris are icy dwarf planets with nearly identical sizes, comparable densities and similar surface compositions as revealed by spectroscopic studies. Pluto possesses an atmosphere whereas Eris does not; the difference probably arises from their differing distances from the Sun, and explains their different albedos. Makemake is another icy dwarf planet with a spectrum similar to Eris and Pluto, and is currently at a distance to the Sun intermediate between the two. Although Makemake's size (1,420 ± 60 km) and albedo are roughly known, there has been no constraint on its density and there were expectations that it could have a Pluto-like atmosphere. Here we report the results from a stellar occultation by Makemake on 2011 April 23. Our preferred solution that fits the occultation chords corresponds to a body with projected axes of 1,430 ± 9 km (1σ) and 1,502 ± 45 km, implying a V-band geometric albedo p(V) = 0.77 ± 0.03. This albedo is larger than that of Pluto, but smaller than that of Eris. The disappearances and reappearances of the star were abrupt, showing that Makemake has no global Pluto-like atmosphere at an upper limit of 4-12 nanobar (1σ) for the surface pressure, although a localized atmosphere is possible. A density of 1.7 ± 0.3 g cm(-3) is inferred from the data.
Published: 2012
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239. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation.

Author: Sicardy B, Ortiz JL, Assafin M, Jehin E, Maury A, Lellouch E, Hutton RG, Braga-Ribas F, Colas F, Hestroffer D, Lecacheux J, Roques F, Santos-Sanz P, Widemann T, Morales N, Duffard R, Thirouin A, Castro-Tirado AJ, Jelínek M, Kubánek P, Sota A, Sánchez-Ramírez R, Andrei AH, Camargo JI, da Silva Neto DN, Gomes AR Jr, Martins RV, Gillon M, Manfroid J, Tozzi GP, Harlingten C, Saravia S, Behrend R, Mottola S, Melendo EG, Peris V, Fabregat J, Madiedo JM, Cuesta L, Eibe MT, Ullán A, Organero F, Pastor S, de Los Reyes JA, Pedraz S, Castro A, de la Cueva I, Muler G, Steele IA, Cebrián M, Montañés-Rodríguez P, Oscoz A, Weaver D, Jacques C, Corradi WJ, Santos FP, Reis W, Milone A, Emilio M, Gutiérrez L, Vázquez R, and Hernández-Toledo H
Abstract: The dwarf planet Eris is a trans-Neptunian object with an orbital eccentricity of 0.44, an inclination of 44 degrees and a surface composition very similar to that of Pluto. It resides at present at 95.7 astronomical units (1 AU is the Earth-Sun distance) from Earth, near its aphelion and more than three times farther than Pluto. Owing to this great distance, measuring its size or detecting a putative atmosphere is difficult. Here we report the observation of a multi-chord stellar occultation by Eris on 6 November 2010 UT. The event is consistent with a spherical shape for Eris, with radius 1,163 ± 6 kilometres, density 2.52 ± 0.05 grams per cm(3) and a high visible geometric albedo, Pv = 0.96(+0.09)(-0.04). No nitrogen, argon or methane atmospheres are detected with surface pressure larger than ∼1 nanobar, about 10,000 times more tenuous than Pluto's present atmosphere. As Pluto's radius is estimated to be between 1,150 and 1,200 kilometres, Eris appears as a Pluto twin, with a bright surface possibly caused by a collapsed atmosphere, owing to its cold environment. We anticipate that this atmosphere may periodically sublimate as Eris approaches its perihelion, at 37.8 astronomical units from the Sun.
Published: 2011
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240. Charon's size and an upper limit on its atmosphere from a stellar occultation.

Author: Sicardy B, Bellucci A, Gendron E, Lacombe F, Lacour S, Lecacheux J, Lellouch E, Renner S, Pau S, Roques F, Widemann T, Colas F, Vachier F, Martins RV, Ageorges N, Hainaut O, Marco O, Beisker W, Hummel E, Feinstein C, Levato H, Maury A, Frappa E, Gaillard B, Lavayssière M, Di Sora M, Mallia F, Masi G, Behrend R, Carrier F, Mousis O, Rousselot P, Alvarez-Candal A, Lazzaro D, Veiga C, Andrei AH, Assafin M, da Silva Neto DN, Jacques C, Pimentel E, Weaver D, Lecampion JF, Doncel F, Momiyama T, and Tancredi G
Abstract: Pluto and its satellite, Charon (discovered in 1978; ref. 1), appear to form a double planet, rather than a hierarchical planet/satellite couple. Charon is about half Pluto's size and about one-eighth its mass. The precise radii of Pluto and Charon have remained uncertain, leading to large uncertainties on their densities. Although stellar occultations by Charon are in principle a powerful way of measuring its size, they are rare, as the satellite subtends less than 0.3 microradians (0.06 arcsec) on the sky. One occultation (in 1980) yielded a lower limit of 600 km for the satellite's radius, which was later refined to 601.5 km (ref. 4). Here we report observations from a multi-station stellar occultation by Charon, which we use to derive a radius, R(C) = 603.6 +/- 1.4 km (1sigma), and a density of rho = 1.71 +/- 0.08 g cm(-3). This occultation also provides upper limits of 110 and 15 (3sigma) nanobar for an atmosphere around Charon, assuming respectively a pure nitrogen or pure methane atmosphere.
Published: 2006
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241. Intraarticular hip treatment with triamcinolonehexacetonide in juvenile chronic arthritis.

Author: Boehnke M, Behrend R, Dietz G, and Küster RM
Subjects: Adolescent, Child, Female, Hip Joint, Humans, Injections, Intra-Articular, Male, Triamcinolone Acetonide administration & dosage, Anti-Inflammatory Agents administration & dosage, Arthritis, Juvenile drug therapy, Triamcinolone Acetonide analogs & derivatives
Abstract: To evaluate the effect and tolerance of intraarticular Triamcinolonehexacetonide (TCH) in the course of chronic coxitis in juvenile chronic arthritis (JCA) in an open uncontrolled study. Since 1990 we treated patients < 16 years of age suffering from chronic coxitis with 1 mg/TCH/KG body weight. The patients were checked again 4-8 weeks after the treatment. Clinical and ultrasound courses were recorded with the help of ultrasound and joint scores. The evaluation took place 6, 12, 24 and 36 months after the treatment. At that time we give a report on the 12 months follow-up of 37 hip joints and the 24 months follow-up of 20 hip joints. The immediate effect of TCH influencing mobility, pain sensitivity and joint effusions of the patients is impressing. The long term effect of TCH has to be evaluated by regular check ups for at least 2 years. An individual comparison with the not treated contralateral joint would be desired if ethically justifiable. Most patients suffering from polyarticular diseases with a long course of coxitis needed more than one injection of TCH (mean reinjection time 5.8 months). Any avascular necrosis of the femoral heads or other complications were not observed.
Published: 1994

242. [Ultrasonographic diagnosis in inflammatory-rheumatic changes of the shoulder joint].

Author: Behrend R
Subjects: Acromioclavicular Joint diagnostic imaging, Arthritis, Rheumatoid diagnostic imaging, Bursa, Synovial diagnostic imaging, Humans, Humerus diagnostic imaging, Joint Capsule diagnostic imaging, Osteoarthritis diagnostic imaging, Rotator Cuff diagnostic imaging, Synovial Membrane diagnostic imaging, Tendons diagnostic imaging, Ultrasonography, Rheumatic Diseases diagnostic imaging, Shoulder Joint diagnostic imaging
Abstract: Inflammatory rheumatoid changes of the shoulder joint are often diagnosed rather late, so therapy is largely directed towards pain reduction and less towards maintenance of full joint function. When considering the mutilating type of chronic polyarthritis, it becomes evident how important the role of the shoulder joint is in the patients performance of basic everyday activities. In this paper the important structures of the shoulder joint that can be visualized by ultrasound are described as to their rheumatological significance, and pathological findings are discussed along with the appropriate therapy.
Published: 1993

243. [Early experiences with the total mini hip-joint endoprosthesis (St. George Mini model) in dysplasia coxarthrosis].

Author: Buchholz HW, Baars GW, Dahmen G, and Behrend R
Subjects: Adult, Aged, Female, Follow-Up Studies, Hip Dislocation, Congenital surgery, Humans, Male, Middle Aged, Postoperative Complications etiology, Prosthesis Design, Prosthesis Failure, Wound Healing, Hip Dislocation surgery, Hip Joint surgery, Hip Prosthesis, Osteoarthritis surgery
Abstract: The results of 106 patients with osteoarthritis secondary to severe congenital hip dysplasia and dislocations of the hip operated at the Endo-Klinik were evaluated after an average follow up of 21 months. 142 "St. Georg-Mini" total hips were implanted employing Refobacin-Palacos R. The clinical results were graded as "combined performance" which considered hip pain, walking distance, hip mobility and walking aids. In 93% of the cases "combined performance" was improved at follow up and 91.7% of the patients were satisfied with the result. The early (during hospitalization) and late (after discharge from hospital) complication rate which had an influence on the result at follow up was 2.1% (n = 3) and 3.5% (n = 4) respectively. There were no deep infections. An extended indication for total hip arthroplasty also for younger patients with severe osteoarthritis secondary to hip dysplasia is discussed and can be advocated.
Published: 1985

244. [Methods of surface measurements in idiopathic scoliosis].

Author: Heise U, Behrend R, and Hinzmann J
Subjects: Adolescent, Adult, Child, Child, Preschool, Female, Humans, Male, Middle Aged, Prognosis, Scoliosis therapy, Anthropometry methods, Scoliosis diagnosis
Abstract: The radiologic evaluation of scoliotic spines is a well established, exact method. In long follow-up histories these patients aquire a remarcable radiation exposure. Measurement of additional clinical parameters intends since decades to minimize this exposure. Documentation of surface deformities follows the presumption of a correlation between these and the radiologic angles. The analysis of 714 completely documented untreated idiopathic scoliotic curves showed a good overall correlation between surface deformity and Cobb angle, but single measurements varied too widely to make the used surface documentation a real alternative to x-rays. Treated scoliosis patients pose additional problems in the evaluation, a any treatment - brace and operation - further diminish the correlation. Obviously the usual clinical surface evaluation can only document the cosmetic appearance. Regular radiologic follow-up stays inevitable especially in treated scoliotic patients.
Published: 1989
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245. [Spontaneous liver rupture in eclampsia].

Author: Seeler M, Behrend R, Mörl FK, and Körner J
Subjects: Adult, Cesarean Section, Eclampsia surgery, Female, Follow-Up Studies, Hematoma pathology, Humans, Infant, Newborn, Liver pathology, Liver Diseases surgery, Male, Pregnancy, Rupture, Spontaneous, Tomography, X-Ray Computed, Ultrasonography, Eclampsia pathology, Liver Diseases pathology
Abstract: We report on a case of a 34-year old nullipara who suffered from rupture of the liver during eclampsia and survived despite most serious complications. Most cases of rupture of a non-traumatic subcapsular haematoma of the liver during pregnancy are associated with symptoms of pre-eclampsia. The pathogenesis of this severe complication as well as diagnostic imaging and surgical treatment are discussed. The classical trias of pre-eclampsia, epigastric pain and sudden circulary collapse may vary considerably. Since early diagnosis is crucial for maternal and foetal outcome, a subcapsular haematoma of the liver should be considered in women during pregnancy and childbed presenting with pre-eclampsia and upper abdominal pain. Here ultrasonographic imaging is a valuable and readily available diagnostic tool for the obstetrician.
Published: 1987
Full Text: View/download PDF

246. [Sonographic assessment of typical lesions in shoulder dislocation].

Author: Hinzmann J, Behrend R, and Heise U
Subjects: Adult, Humans, Joint Instability diagnosis, Male, Recurrence, Shoulder Joint pathology, Shoulder Dislocation diagnosis, Ultrasonography instrumentation
Abstract: The traumatic dislocation of the shoulder joint is the most often joint luxation. The involved patients are often sporting and between the age of 20 to 40 years. The therapeutic and prognostic point of interest is to recognize and reconstruct injured structures. Among the soft tissue injuries the Bankart lesions, among the osseous injuries the Hill-Sachs defect are numeric well to the fore. Hitherto existing diagnostic methods for these injuries are either invasive or with X-rays. Its is demonstrated, that dynamic ultrasonography examination of the shoulder joint can visualize besides the rotator cuff abnormalities of the labrum glenoidale and the caput humeri outline.
Published: 1988
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247. Gentamicin-polymethylmethacrylate chains in the treatment of infected cardiac pacemaker pouches--two case reports.

Author: Behrend R
Subjects: Aged, Aged, 80 and over, Humans, Male, Gentamicins therapeutic use, Methylmethacrylates therapeutic use, Pacemaker, Artificial, Surgical Wound Infection drug therapy
Published: 1988

248. [On the pathogenesis and clinical aspects of anoxic and ischemic cerebral accidents].

Author: ZUELCH KJ and BEHREND RC
Subjects: Humans, Accidents, Brain blood supply, Cardiovascular System, Hypoxia
Published: 1961

249. [Induced abortion and marriage counseling in multiple sclerosis].

Author: Behrend RC
Subjects: Family Planning Services, Female, Germany, West, Humans, Pregnancy, Abortion, Therapeutic, Counseling, Eugenics, Multiple Sclerosis prevention & control
Published: 1972

250. [Vertigo].

Author: Behrend RC
Subjects: Brain Injuries, Cerebrovascular Disorders, Humans, Intracranial Arteriosclerosis, Male, Middle Aged, Vertigo physiopathology, Vertigo therapy, Vertigo etiology
Published: 1966

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