Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-26T07:53:04.010Z Has data issue: false hasContentIssue false
  • English
  • Français

Getting ready for the micro-arcsecond era

Published online by Cambridge University Press:  01 October 2007

A. G. A. Brown
A. G. A. Brown*
Affiliation:
Sterrewacht Leiden, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

As the title of this symposium implies, one of the aims is to examine the future of astrometry as we move from an era in which thanks to the Hipparcos Catalogue everyone has become familiar with milliarcsecond astrometry to an era in which microarcsecond astrometry will become the norm. I will take this look into the future by first providing an overview of present astrometric programmes and how they fit together and then I will attempt to identify the most promising future directions. In addition I discuss the important conditions for the maximization of the scientific return of future large and highly accurate astrometric catalogues; catalogue access and analysis tools, the availability of sufficient auxiliary data and theoretical knowledge, and the education of the future generation of astrometrists.

Keywords

astrometrycatalogssurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S248: A Giant Step: from Milli- to Micro-arcsecond Astrometry , October 2007 , pp. 567 - 576
Copyright
Copyright © International Astronomical Union 2008

References

Beichman, Ch. 2008, this volume, p.238Google Scholar
Boden, A. F. 2008, this volume, p.36Google Scholar
Borsenberger, J., et al. 2006, in Visions for Infrared Astronomy, eds. Coudé du Foresto, V., Rouan, D., & Rousset, G., Paris, RS série I2M vol. 6, LavoisierGoogle Scholar
Bucciarelli, B. 2008, this volume, p.316Google Scholar
Dravins, D., Lindegren, L., & Madsen, S. 1999, A&A, 348, 1040Google Scholar
ESA 1997, The Hipparcos and Tycho Catalogues, ESA SP-1200Google Scholar
Ghez, A. M. 2008, this volume, p.52Google Scholar
Gouda, N. 2008, this volume, p.248Google Scholar
Hekker, S., Reffert, S., Quirrenbach, A., Mitchell, D. S., Fischer, D. A., Marcy, G. W., Butler, R. P. 2006, A&A, 454, 943Google Scholar
Høg, E., Fabricius, C., Makarov, V. V., et al. 2000, A&A, 355, L27Google Scholar
Ivezić, Ž. 2008, this volume, p.537Google Scholar
Jao, W. 2008, this volume, p.421Google Scholar
Lestrade, J.-F. 2008, this volume, p.170Google Scholar
Lindegren, L. 2005, in The Three-Dimensional Universe with Gaia, eds. Turon, C., O'Flaherty, K. S. & Perryman, M. A. C., ESA SP-576, p.29Google Scholar
Lindegren, L. 2008, this volume, p.217Google Scholar
Ma, C. 2008, this volume, p.337Google Scholar
Madsen, S., Dravins, D., & Lindegren, L. 2002, A&A, 381, 446Google Scholar
Magnier, E. A. 2008, this volume, p.552Google Scholar
Monet, D. G., Levine, S. E., Canzian, B., et al. 2003, AJ, 125, 984CrossRefGoogle Scholar
Morrison, J. E., Röser, S., McLean, B., et al. 2001, AJ, 121, 1752Google Scholar
Reid, M. 2008, this volume, p.141CrossRefGoogle Scholar
Richichi, A. 2008, this volume, p.44CrossRefGoogle Scholar
Röll, T., Seifahrt, T., Neuhauser, R. 2008, this volume, p.48CrossRefGoogle Scholar
Skrutskie, M. F., Cutri, R. M., Stiening, M. D., et al. 2006, AJ, 131, 1163Google Scholar
Shao, M. 2008, this volume, p.231Google Scholar
Smart, R. 2008, this volume, p. 429Google Scholar
Steinmetz, M., Zwitter, T., Siebert, A., et al. 2006, AJ, 132, 1645CrossRefGoogle Scholar
van Leeuwen, F. 2007, Hipparcos, the New Reduction of the Raw Data, SpringerCrossRefGoogle Scholar
Zacharias, N., Urban, S. E., Zacharias, M. I., et al. 2004, AJ, 127, 3043CrossRefGoogle Scholar