Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-23T10:42:34.401Z Has data issue: false hasContentIssue false
  • English
  • Français

Hubble's Next Generation Spectral Library

Published online by Cambridge University Press:  01 December 2006

Sara R. Heap  and
Don Lindler
Sara R. Heap
Affiliation:
NASA's Goddard Space Flight Center, Greenbelt MD 20771, USA
Don Lindler
Affiliation:
NASA's Goddard Space Flight Center, Greenbelt MD 20771, USA Sigma Space Corp., 9801 Greenbelt Rd., Lanham MD 20706, USA
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.

We give a progress report on our work to reduce and calibrate spectra obtained for Hubble's Next Generation Spectral Library (NGSL). We will shortly be working with Bruzual and Charlot to incorporate these spectra into their stellar population synthesis code.

Keywords

stars: fundamental parametersultraviolet: starsspace vehicle: instrumentstechniques: spectroscopicatlases
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 95 - 96
Copyright
Copyright © International Astronomical Union 2007

References

Bruzual, A.G. & Charlot, S. 2003, MNRAS, 344, 1000CrossRefGoogle Scholar
Heap, S.R. & Lanz, T.M. 2005, in Multiwavelength Mapping of Galaxy Formation and Evolution, Springer-Verlag: Berlin, p. 210CrossRefGoogle Scholar
Kauffmann, G., Heckman, T., White, S. et al. , 2003, MNRAS, 341, 54CrossRefGoogle Scholar
Munari, U. et al. 2005, A&A, 442, 1127Google Scholar