The TROY project 

Publications
  Refereed articles of the project and previous works on co-orbital bodies from the team members
TROY papers

• Balsalobre-Ruza et al., 2024, A&A, in press: The TROY project. III. Exploring co-orbitals around low-mass stars
• Balsalobre-Ruza et al., 2023, A&A, 675, 172: Tentative co-orbital submillimeter emission within the Lagrangian region L5 of the protoplanet PDS 70 b
• Lillo-Box et al., 2020, A&A, 642, 121: Planetary system LHS 1140 revisited with ESPRESSO and TESS
• Leleu et al., 2019, A&A, 624, 46: Co-orbital exoplanets from close period candidates: The TOI-178 case
• Lillo-Box et al., 2018, A&A 618, A42 : The TROY project: II. Multi-technique constraints on exotrojans in nine planetary systems.
• Lillo-Box et al., 2018, A&A, 609, 96 : The TROY project: searching for co-orbital bodies to known planets.
• Leleu et al., 2017, A&A, 599, 7 : Detection of co-orbital planets by combining transit and radial-velocity measurements

TROY non-refereed works

• Lillo-Box et al., 2018 , White paper submitted in response to the solicitation of feedback for the "Exoplanet Science Strategy" by the National Academy of Sciences, Engineering, and Medicine) : Towards completing Planetary Systems: The role of minor bodies on life growth and survival.

Papers on co-orbitals including team members

Observations

• Maire et al. (incl. Lillo-Box), 2023, PASP, 135, 1052, 17: Workshop Summary: Exoplanet Orbits and Dynamics
• Damasso et al. (incl. Lillo-Box), 2020, A&A, 642, 31 : A precise architecture characterization of the π Mensae planetary system
• Mortier et al. (incl. Lillo-Box), 2020, MNRAS, 499, 5004: K2-111: an old system with two planets in near-resonance
• Toledo-Padrón et al. (incl. Lillo-Box), 2020, A&A, 641, 92 : Characterization of the K2-38 planetary system.
• Armstrong et al. (incl. Lillo-Box), 2020, Nature, 583, 39: A remnant planetary core in the hot-Neptune desert

Theory

• Leleu et al. (2019) : On the stability of the co-orbital resonance under dissipation
• Leleu et al. (2015) : Detectability of quasi-circular co-orbital planets. Application to the radial velocity technique
• Leleu et al. (2015) : On the rotation of co-orbital bodies in eccentric orbits
• Robutel et al. (2015) : Rigorous treatment of the averaging process for co-orbital motions in the planetary problem
• Robutel et al. (2014) : Spin-orbit resonances and rotation of coorbital bodies in quasi-circular orbits
• Correia et al. (2013) : Analytical description of physical librations of saturnian coorbital satellites Janus and Epimetheus
• Robutel et al. (2011) : Analytical description of physical librations of saturnian coorbital satellites Janus and Epimetheus
• Robutel et al. (2006) : The resonant structure of Jupiter's Trojan asteroids - I. Long-term stability and diffusion
  

Master Thesis

• José Atienza (2017-2018):  "Exploring the transit timing variations technique to search for co-orbital planets" (Valencia International University)
• Ángel Fernández Lois (2019): "Search for co-orbital pairs in long-period exoplanets " (Valencia International University)
• Raúl de Frutos (2019): "Detection of co-orbital planets with TESS" (Valencia International University
• David Barba González (2020): "A Transit Search for Exotrojans in Planetary Systems with Mean Motion Resonances" (Universidad Autónoma de Madrid)
• Eva Herrero (2020): "Búsqueda de cuerpos troyanos en estrellas de tipo M por el método de tránsitos "
• Amadeo Castro (2020): "Ground-based photometric search for transiting co-orbital planets: A proof-of-concept
  " (Valencia International University)
• Laura López Ibáñez (2022): Implications of co-orbital planets destabilization in the architecture of planetary systems
• Jimmy Alexander Muela Pillajo (2023-2024.): "The astrometric signature of co-orbital bodies"