Rotational properties of asteroids from Gaia disk-integrated photometry: A “genetic” algorithm

Author:

Cellino A.,Delbò M.,Zappalà V.,Dell’Oro A.,Tanga P.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference8 articles.

1. Bus, S.J., 1999. Compositional Structure in the Asteroid Belt: Results of a Spectroscopic Survey, Ph.D. Thesis, Massachusetts Institute of Technology, Boston.

2. Ivezić, Z. and other 31 authors. Solar system objects observed in the Sloan digital sky survey commissioning data. Astron. J. 122, 2749–2784, 2001.

3. Kaasalainen, K., Mottola, S., Fulchignoni, M. Asteroid models from disk-integrated data, in: Bottke, W.F., Cellino, A., Paolicchi, P., Binzel, R.P. (Eds.), Asteroids III, Tucson, pp. 139–150, 2002.

4. Physical models of large number of asteroids from calibrated photometry sparse in time;Kaasalainen;Astron. Astrophys.,2004

5. Magnusson, P., Barucci, M.A., Drummond, J.D., Lumme, K., Ostro, S.J., Surdej, J., Taylor, R.C., Zappalá, V. Determination of pole orientations and shapes of asteroids, in: Binzel, R.P., Gehrels, T., Matthews, M.S. (Eds.), Asteroids II, Tucson, pp. 66–97, 1989.

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