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Feuerbach, M.-J. Kim, M. K. Kami\\'nska, M. Poli\\'nska, M. \\.Zejmo, N. Parley, O. Thizy, P. Antonini, P. Kulczak, P. Trela, R. Behrend, R. Crippa, R. Ditteon, R. Duffard, R. Goncalves, R. Hirsch, R. Roy, R. Szak\\'ats, S. Fauvaud, S. Geier, S. Marks, S. Urakawa, T. G. M\\\"uller, T. Polakis, T. Santana-Ros, V. Al\\'i-Lagoa, V. Kudak, V. Perig, W. Og{\\l}oza","submitted_at":"2019-05-15T09:49:48Z","abstract_excerpt":"Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface. 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).\n  Aims. 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Marciniak, A. P\\'al, B. Skiff, D.-H. Kim, D. Oszkiewicz, E. Barbotin, E. Podlewska - Gaca, E. Sonbas, F. Manzini, F. Monteiro, F. Pilcher, I. Grze\\'skowiak, I. Konstanciak, J. Garlitz, J. Grice, J. Horbowicz, J. J. Sanabria, J. L. Maestre, J. Skrzypek, K. Kami\\'nski, K. Sobkowiak, K. \\.Zukowski, L. Bernasconi, L. Moln\\'ar, M. Butkiewicz - B\\k{a}k, M. Feuerbach, M.-J. Kim, M. K. Kami\\'nska, M. Poli\\'nska, M. \\.Zejmo, N. Parley, O. Thizy, P. Antonini, P. Kulczak, P. Trela, R. Behrend, R. Crippa, R. Ditteon, R. Duffard, R. Goncalves, R. Hirsch, R. Roy, R. Szak\\'ats, S. Fauvaud, S. Geier, S. Marks, S. Urakawa, T. G. M\\\"uller, T. Polakis, T. Santana-Ros, V. Al\\'i-Lagoa, V. Kudak, V. Perig, W. Og{\\l}oza","submitted_at":"2019-05-15T09:49:48Z","abstract_excerpt":"Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface. 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