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1. Scaling slowly rotating asteroids with stellar occultations

Author

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

Published
2023
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2. Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Author

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

Published
2021
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3. Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

Author

Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Marciniak, Anna, Ďurech, Josef, Alí-Lagoa, Víctor, Ogłoza, W., Szakáts, Róbert, Müller, Thomas G., Molnár, László, Pál, András, Monteiro, F., Arcoverde, P., Behrend, Raoul, Benkhaldoun, Zouhair, Bernasconi, Laurent, Bosch, J., Brincat, S., Brunetto, L., Butkiewicz-Bąk, Magdalena, Del Freo, F., Duffard, René, Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, Marin, Geier, Stefan, Golonka, J., Grice, Jonny, Hirsch, R., Horbowicz, J., Jehin, Emmanuel, Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M.K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, Myung-Jin, Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, Nicolás, Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, Edyta, Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, René, Sanabria, J.J., Santana-Ros, Toni, Skiff, B., Skrzypek, J., Sobkowiak, Krzysztof, Sonbas, E., Stachowski, G., Strajnic, J., Trela, P., Tychoniec, Ł., Urakawa, S., Verebelyi, E., Wagrez, K., Żejmo, M., Żukowski, K., Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Marciniak, Anna, Ďurech, Josef, Alí-Lagoa, Víctor, Ogłoza, W., Szakáts, Róbert, Müller, Thomas G., Molnár, László, Pál, András, Monteiro, F., Arcoverde, P., Behrend, Raoul, Benkhaldoun, Zouhair, Bernasconi, Laurent, Bosch, J., Brincat, S., Brunetto, L., Butkiewicz-Bąk, Magdalena, Del Freo, F., Duffard, René, Evangelista-Santana, M., Farroni, G., Fauvaud, S., Fauvaud, M., Ferrais, Marin, Geier, Stefan, Golonka, J., Grice, Jonny, Hirsch, R., Horbowicz, J., Jehin, Emmanuel, Julien, P., Kalup, Cs., Kamiński, K., Kamińska, M.K., Kankiewicz, P., Kecskeméthy, V., Kim, D.-H., Kim, Myung-Jin, Konstanciak, I., Krajewski, J., Kudak, V., Kulczak, P., Kundera, T., Lazzaro, D., Manzini, F., Medeiros, H., Michimani-Garcia, J., Morales, Nicolás, Nadolny, J., Oszkiewicz, D., Pakštienė, E., Pawłowski, M., Perig, V., Pilcher, F., Pinel, P., Podlewska-Gaca, Edyta, Polakis, T., Richard, F., Rodrigues, T., Rondón, E., Roy, René, Sanabria, J.J., Santana-Ros, Toni, Skiff, B., Skrzypek, J., Sobkowiak, Krzysztof, 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 work we increase the sample of slow rotators with reliable spin and shape models and known thermal inertia by 40%. The thermal inertia values of our sample d

Published
2021

4. Thermal properties of slowly rotating asteroids: results from a targeted survey

Author

National Science Centre (Poland), European Commission, Ministry of Education (Slovak Republic), Ministerio de Ciencia, Innovación y Universidades (España), Hungarian Academy of Sciences, Marciniak, A., Ali-Lagoa, Victor, Mueller, T.G., Szakáts, R., Molnár, L., Pal, A., Podlewska-Gaca, E., Parley, N., Antonini, P., Barbotin, E., Behrend, R., Bernasconi, L., Butkiewicz-Bąk, M., Crippa, R., Duffard, René D., Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S., Goncalves, R, Grice, J., Grzeskowiak, I, Hirsch, R., Horbowicz, J, Kaminski, K., Kamińska, M. K., Kim, D. H., Kim, M. J., Konstanciak, I., Kudak, V., Kulczak, P, Maestre, J.L., Manzini, F., Marks, S, Monteiro, F, Ogloza, W, Oszkiewicz, D., Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R., Sanabria, JJ, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Zejmo, M, Zukowski, K, National Science Centre (Poland), European Commission, Ministry of Education (Slovak Republic), Ministerio de Ciencia, Innovación y Universidades (España), Hungarian Academy of Sciences, Marciniak, A., Ali-Lagoa, Victor, Mueller, T.G., Szakáts, R., Molnár, L., Pal, A., Podlewska-Gaca, E., Parley, N., Antonini, P., Barbotin, E., Behrend, R., Bernasconi, L., Butkiewicz-Bąk, M., Crippa, R., Duffard, René D., Ditteon, R, Feuerbach, M, Fauvaud, S, Garlitz, J, Geier, S., Goncalves, R, Grice, J., Grzeskowiak, I, Hirsch, R., Horbowicz, J, Kaminski, K., Kamińska, M. K., Kim, D. H., Kim, M. J., Konstanciak, I., Kudak, V., Kulczak, P, Maestre, J.L., Manzini, F., Marks, S, Monteiro, F, Ogloza, W, Oszkiewicz, D., Pilcher, F, Perig, V, Polakis, T, Polinska, M, Roy, R., Sanabria, JJ, Santana-Ros, T, Skiff, B, Skrzypek, J, Sobkowiak, K, Sonbas, E, Thizy, O, Trela, P, Urakawa, S, Zejmo, M, and Zukowski, K

Abstract

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the subsurface. However, thermal inertias have been determined mainly for fast rotators due to selection effects in the available photometry used to obtain shape models required for thermophysical modelling (TPM). Aims. Our aims are to mitigate these selection effects by producing shape models of slow rotators, to scale them and compute their thermal inertia with TPM, and to verify whether thermal inertia increases with the rotation period. Methods. To decrease the bias against slow rotators, we conducted a photometric observing campaign of main-belt asteroids with periods longer than 12 h, from multiple stations worldwide, adding in some cases data from WISE and Kepler space telescopes. For spin and shape reconstruction we used the lightcurve inversion method, and to derive thermal inertias we applied a thermophysical model to fit available infrared data from IRAS, AKARI, and WISE. Results. We present new models of 11 slow rotators that provide a good fit to the thermal data. In two cases, the TPM analysis showed a clear preference for one of the two possible mirror solutions. We derived the diameters and albedos of our targets in addition to their thermal inertias, which ranged between 3(-3)(+33) and 45(-30)(+60) Jm(-2) s(-1/2) K-1. Conclusions. Together with our previous work, we have analysed 16 slow rotators from our dense survey with sizes between 30 and 150 km. The current sample thermal inertias vary widely, which does not confirm the earlier suggestion that slower rotators have higher thermal inertias.© ESO 2019

Published
2019

5. Thermal properties of slowly rotating asteroids: results from a targeted survey

Author

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

Published
2019
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