Abstract
The use of a method of spectra disentangling for telluric lines is explained in detail, with a particular emphasis on high-precision radial-velocity measurements for the search for extrasolar planets. New improvements to the method are introduced. © ESO 2006.
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APA
Hadrava, P. (2006). Disentangling telluric lines in stellar spectra. Astronomy and Astrophysics, 448(3), 1149–1152. https://doi.org/10.1051/0004-6361:20054209
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