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2017MNRAS.472.3467S - Mon. Not. R. Astron. Soc., 472, 3467-3473 (2017/December-2)
A differential least-squares deconvolution method for high precision spectroscopy of stars and exoplanets - I. Application to obliquity measurements of HARPS observations of HD189733b.
STRACHAN J.B.P. and ANGLADA-ESCUDE G.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): techniques: spectroscopic - planet-star interactions - stars: rotation - stars: rotation
Simbad objects: 5
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