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SpS1-The Spitzer atlas of stellar spectra

Published online by Cambridge University Press:  21 October 2010

David R. Ardila ,
W. Makowiecki ,
S. van Dyk ,
I. Song ,
J. Stauffer ,
J. Rho ,
S. Fajardo-Acosta ,
D. W. Hoard  and
S. Wachter
David R. Ardila
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
W. Makowiecki
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
S. van Dyk
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
I. Song
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
J. Stauffer
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
J. Rho
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
S. Fajardo-Acosta
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
D. W. Hoard
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
S. Wachter
Affiliation:
Spitzer Science Center, California Institute of Technology, M/C 220-6, Pasadena, California 91214, USA email: dlp@ipac.caltech.edu
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We present Spitzer Space Telescope spectra of 147 stars (R~64 - 128, λλ = 5 - 35 μm, S/N~100) covering most spectral and luminosity classes within the HR diagram. The spectra are available from the NASA/IPAC Infrared Science Archive (IRSA) and from the first author's webpage (http://web.ipac.caltech.edu/staff/ardila/Atlas/). The Atlas contains spectra of ‘typical’ stars, which may serve to refine galactic synthesis models, study stellar atmospheres, and establish a legacy for future IR missions, such as JWST.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 512
Copyright
Copyright © International Astronomical Union 2010

References

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