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Integral-field Near-infrared Spectro-photometric Surveys from Dome C

Published online by Cambridge University Press:  13 November 2008

H. Zinnecker ,
N. Epchtein ,
H. Rauer ,
T. Le Bertre ,
N. Epchtein  and
I. Vauglin
T. Le Bertre
Affiliation:
LERMA, UMR 8112, Paris Observatory, France
N. Epchtein
Affiliation:
Fizeau, UMR 6525, Nice-Sophia-Antipolis University, France
I. Vauglin
Affiliation:
CRAL, UMR 5574, Lyon Observatory, France
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Abstract

Near-infrared spectro-photometry, at a spectral resolution of ~100, allows to characterize a great variety of stellar sources, from late-typegiants to emission line stars. Various components of the inter-stellar medium can also be traced. This technique can therefore be very fruitful, in addition, for studies of star forming regions, the Milky Way and external galaxies.The outstanding environmental conditions that are expected at Dome C should be favorable to carry out spectro-photometric surveys in the 1 to 2.5 μm region, that would usefully complement space-borne projects.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 33: 2nd ARENA Conference: The Astrophysical Science Cases at Dome C , 2008 , pp. 253 - 256
Copyright
© EAS, EDP Sciences, 2008

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