Precision laboratory UV and IR wavelengths for cosmological and astrophysical applications

Details Precision laboratory UV and IR wavelengths for cosmological and astrophysical applications Precision laboratory UV and IR wavelengths for cosmological and astrophysical applications

2007-03-14

arxiv.org/abs/astro-ph/0703356v2

Astronomy and Astrophysics

Astrophysics

To appear in the proceedings of "Precision Spectroscopy in Astrophysics", Aveiro, Portugal, Sep. 2006, eds Pasquini et al., ES

Scientific paper

10.1007/978-3-540-75485-5_55

The quality of astronomical spectra is now so high that the accuracy of the laboratory data is getting more and more important for the analysis and interpretation. Both in astrophysics and cosmology the needs for accurate laboratory wavelengths have increased with the development of new ground-based and air-borne telescopes and spectrographs. The high resolution UV Fourier Transform spectrometer at Lund Observatory is being used for studying laboratory spectra of astrophysically important elements. Measurements of accurate laboratory UV and IR wavelengths have been made for cosmological and astrophysical applications.

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