A review of spectroscopic methods for observations of stars in searching and studying exoplanets is presented. Instrumental errors in measuring ray velocities and ways to decrease (or fundamentally eliminate) them are considered. The role of astrometric and photometric methods is pointed out. The results of the study of the chemical composition of parent stars and the spectroscopy of transit phenomena are discussed. Some promising directions are evaluated. The development of ground-based and orbital domestic equipment for spectroscopy and spectropolarimetry of stars is reported.

Keywords: extrasolar planets, stars, spectroscopy PACS: 95.75.Fg, 97.10.−q, 97.82.−j (all) DOI: 10.3367/UFNe.2019.07.038597 URL: https://ufn.ru/en/articles/2020/6/c/ 000563842900003 2-s2.0-85092061603 2020PhyU...63..562P Citation: Panchuk V E, Balega Yu Yu, Klochkova V G, Sachkov M E "Study of exoplanets by spectroscopic methods" Phys. Usp. 63 562–582 (2020) BibTexBibNote ® (generic)BibNote ® (RIS)Medline RefWorks RT Journal T1 Study of exoplanets by spectroscopic methods A1 Panchuk,V.E. A1 Balega,Yu.Yu. A1 Klochkova,V.G. A1 Sachkov,M.E. PB Physics-Uspekhi PY 2020 FD 10 Jun, 2020 JF Physics-Uspekhi JO Phys. Usp. VO 63 IS 6 SP 562-582 DO 10.3367/UFNe.2019.07.038597 LK https://ufn.ru/en/articles/2020/6/c/ Received: 4th, April 2019, revised: 2nd, July 2019, accepted: 2nd, July 2019 Оригинал: Панчук В Е, Балега Ю Ю, Клочкова В Г, Сачков М Е «Исследование экзопланет спектроскопическими методами» УФН 190 605–626 (2020); DOI: 10.3367/UFNr.2019.07.038597