Disentangling telluric lines in stellar spectra
arXiv:astro-ph/0602423 · doi:10.1051/0004-6361:20054209
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.
Accepted for publication in Astronomy and Astrophysics
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