CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars
G. Ottoni, S. Udry, D. S\'egransan, G. Buldgen, C. Lovis, P., Eggenberger, C. Pezzotti, V. Adibekyan, M. Marmier, M. Mayor, N.C. Santos,, S.G. Sousa, N. Lagarde, and C. Charbonnel

TL;DR
This paper reports the discovery of three new planets orbiting evolved giant stars through a radial-velocity survey, providing insights into planetary systems around intermediate-mass stars and contributing to statistical understanding.
Contribution
First detection of planets around evolved giant stars using the CORALIE spectrograph, expanding knowledge of planetary occurrence around intermediate-mass stars.
Findings
Discovered three new planets around giant stars.
Established a methodology for distinguishing stellar jitter from planetary signals.
Provided statistical data on planetary systems around evolved stars.
Abstract
Context. Following the first discovery of a planet orbiting a giant star in 2002, we started the CORALIE radial-velocity search for companions around evolved stars (CASCADES). We present the observations of three stars conducted at the 1.2 m Leonard Euler Swiss telescope at La Silla Observatory, Chile, using the CORALIE spectrograph. Aims. We aim to detect planetary companions to intermediate-mass G- and K- type evolved stars and perform a statistical analysis of this population. We searched for new planetary systems around the stars HD22532 (TIC 200851704), HD64121 (TIC 264770836), and HD69123 (TIC 146264536). Methods. We have followed a volume-limited sample of 641 red giants since 2006 to obtain high-precision radial-velocity measurements. We used the Data & Analysis Center for Exoplanets (DACE) platform to perform a radial-velocity analysis to search for periodic signals in the line…
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