HARPSN_spectral_line_profile_indicators

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A computer code (procedure) written in Interactive Data Language (IDL, version 8.4) to compute the spectral line profile indicators used by Lanza et al. (2018, A&A in press) to study the radial velocity variations of planet-hosting sun-like stars.

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Created on

April 18, 2018

Copy SSH clone URLgit@git.ia2.inaf.it:antonino.lanza/HARPSN_spectral_line_profile_indicators.git
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