Science Results Enabled by SDSS Astrometric Observations

Z. Ivezic; N. Bond; M. Juric; J. A. Munn; R. H. Lupton; J. R. Pier; G. S. Hennessy; G. R. Knapp; J. E. Gunn; C. M. Rockosi; T. Quinn

arXiv · astro-ph/0701502

Science Results Enabled by SDSS Astrometric Observations

Z. Ivezic·N. Bond·M. Juric·J. A. Munn·R. H. Lupton·J. R. Pier·G. S. Hennessy·G. R. Knapp·J. E. Gunn·C. M. Rockosi·T. Quinn

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Abstract

We discuss several results made possible by accurate SDSS astrometric measurements in a large sky area, with emphasis on asteroids and stellar proper motions obtained by comparing POSS and SDSS. SDSS has observed over 200,000 moving objects in five photometric bands, corresponding to about two orders of magnitude increase over previous multi--color surveys. These data were used to extend the measurement of asteroid size distribution to a smaller size limit, to demonstrate that asteroid dynamical families, defined as clusters in orbital parameter space, also strongly segregate in color space, and to discover a correlation between asteroid age and colors. A preliminary analysis of SDSS-POSS proper motions for about 1 million M dwarf stars demonstrates that, in the 0.1-1 kpc distance range, the rotational velocity and its dispersion for disk stars increase with the distance from the Galactic plane.

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Z. Ivezic, N. Bond, M. Juric, J. A. Munn, R. H. Lupton, J. R. Pier, G. S. Hennessy, G. R. Knapp, J. E. Gunn, C. M. Rockosi, T. Quinn. 2007-01-17. Science Results Enabled by SDSS Astrometric Observations. https://arxiv.org/abs/astro-ph/0701502

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