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About me

keywords: cool stars · binaries · exoplanets · radial velocity

I am a postdoctoral researcher at the Centro de Astrobiología (CAB) based at the European Space Astronomy Centre (ESAC) in Madrid. I investigate stellar multiplicity and planetary architectures, with a current emphasis on hierarchical triple systems. I contribute to the KOBE and CARMENES projects and lead observing proposals focused on stellar multiplicity, exoplanet detection, and stellar parameter determination from high-resolution spectroscopy.

ADS GitHub CV

Projects

In course

Triple Trouble: Exoplanets in hierarchical triple systems

Triple star systems are more common than often assumed, yet planets in them remain understudied. Their orbital architectures offer valuable clues about planet and star formation in complex gravitational settings. Stable planets in these systems reflect the delicate balance required for long-term dynamical survival.

Exoplanets Binaries Dynamics
In course

One is the Loneliest Number: Triple stars are everywhere

Gaia astrometry reveals subtle anomalies in stars that appear single, hinting at unresolved companions. This project follows up such cases to identify spectroscopic binaries, essential to avoid false planet detections, refine stellar parameters, and complete the census of close stellar multiplicity.

Binaries Spectroscopy Gaia
Project collaboration

K-dwarfs Orbited By habitable Exoplanets (KOBE)

PI: J. Lillo Box

The KOBE experiment is a legacy radial-velocity survey using CARMENES at Calar Alto. By targeting the overlooked K dwarfs, KOBE bridges the gap between G- and M‑dwarf studies. The project has already confirmed a planet near the habitable zone of a K dwarf.

Exoplanets Spectroscopy CARMENES
Project collaboration

Calar Alto search for exoearths in M dwarfs (CARMENES)

PIs: P.J. Amado, A. Quirrenbach

CARMENES is a dual-channel high-resolution spectrograph operating at the 3.5m Calar Alto telescope, dedicated to the detection of terrestrial-mass exoplanets around M dwarfs. The survey has led to the discovery and characterisation of dozens of exoplanets, and is a cornerstone of low-mass star research in Europe.

Exoplanets Spectroscopy CARMENES

Selected publications

For a complete list of my publications, visit my profile on ADS.

2025

KOBE-1: The first planetary system from the KOBE survey

Balsalobre-Ruza et al.

The first discovery of the KOBE project: two super-Earth- or sub-Neptune-mass planets orbiting a quiet K7 star.

New! KOBE K dwarfs Habitability

2025

Multiplicity of M dwarfs from close spectroscopic binaries to ultra‑wide systems

Cifuentes et al.

Complete multiplicity study ranging from close spectroscopic binaries to ultra-wide companions.

New! M dwarfs Binaries

2024

Multiplicity of stars with planets in the solar neighbourhood

González-Payo et al.

Detailed study of 212 exoplanet host stars in multiple systems, revealing how stellar multiplicity influences planet formation, orbital properties, and habitability.

Exoplanets Binaries Multiplicity

2024

Kinematics of M dwarfs in the solar neighbourhood

Cortés-Contreras et al.

Exhaustive kinematic analysis of 2187 M dwarfs, identifying 191 young star candidates and improving our understanding of stellar ages.

M dwarfs Kinematics Young stars

2023

C. Cifuentes | PhD thesis

2022

A detailed analysis of the Gl 486 planetary system

Caballero et al.

An improved characterization of the nearby warm rocky planet Gl 486 b achieving 4.7% precision in radius and 4.2% in mass.

Exoplanets Rocky planets Characterization

2021

Stellar atmospheric parameters of CARMENES target stars with SteParSyn

Marfil et al.

Bayesian determination of effective temperatures, surface gravities, and metallicities for 343 M dwarfs using spectral synthesis.

Top cited Stellar parameters Spectroscopy

2020

Luminosities, colours, and spectral energy distributions of M dwarfs

Cifuentes et al.

Benchmark study for colours and stellar parameters of M dwarfs in the CARMENES input catalogue.

Top cited M dwarfs Stellar parameters

2019

Different roads to radii and masses of the CARMENES target stars

Schweitzer et al.

Precise radii and masses for 293 nearby M dwarfs, achieving 2-5% precision and consistency across techniques.

Top cited M dwarfs Stellar parameters

2019

Exomoons in the habitable zones of M dwarfs

Martínez-Rodríguez et al.

Among 33 exoplanets in habitable zones around M dwarfs, four are capable of hosting stable Moon- to Titan-mass exomoons for timescales exceeding the age of the Universe.

Exomoons Habitability M dwarfs

Search the associated catalogues

Now

Past, present and future scientific events of 2025.

February 2026

Workshop on Planets Around M-Dwarfs

Invited talk: "M dwarfs in multiple star systems"

Lund University, Sweden

December 2025

Exploring Tattoine and beyond: Circumbinary planets with ESAC missions

Local Organising Committee

European Space Astronomy Centre, Spain

Now

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October 2025

ESA's Madrid-Area Exoplanet Science Meeting (MAESM)

Talk: "Exoplanets in triple star systems"

European Space Astronomy Centre, Spain

July 2025

Detection and Dynamics of Exoplanets (DDE): Interplay between theory and observations

Talk: "Exoplanets in triple star systems"

University of Coimbra, Portugal

May 2025

KOBE Hackathon Week #3

Genève Observatory, Switzerland

Contact

ccifuentes@cab.inta-csic.es
Schedule a meeting

Centro de Astrobiología (CSIC-INTA)
Camino Bajo del Castillo s/n
Campus European Space Astronomy Centre
28692 Villanueva de la Cañada, Madrid, Spain