collaborators

6 papers

astro-ph.EP2026

Closeby Habitable Exoplanet Survey (CHES). V. Planetary Parameters Derived from Angular Separation Variations

Dongjie Tan, Jianghui Ji, Chunhui Bao +11

The Closeby Habitable Exoplanet Survey (CHES) aims to achieve microarcsecond-level astrometry of about one hundred nearby FGK-type stars within 10 parsecs to detect Earth-like plan…

astro-ph.EP2025

The Formation of Ultra-short-period Planets under the Influence of the Nearby Planetary Companions

Jia Jun Zhu, Su Wang, Jianghui Ji +1

Ultra-short-period (USP) planets, defined as those with orbital periods shorter than 1 day, provide valuable insights into planetary evolution under strong stellar tidal interactio…

astro-ph.EP2025

Direct Imaging for the Debris Disk around Eridani with the Cool-Planet Imaging Coronagraph

Chunhui Bao, Jianghui Ji, Gang Zhao +4

We analyze the inner debris disk around Eridani using simulated observations with the Cool-Planet Imaging Coronagraph (CPI-C). Using the radiative transfer code MCFOST, we gen…

astro-ph.EP2025

A high mutual inclination system around KOI-134 revealed by transit timing variations

Emma Nabbie, Chelsea X. Huang, Judith Korth +9

Few planetary systems have measured mutual inclinations, and even less are found to be non-coplanar. Observing the gravitational interactions between exoplanets is an effective too…

astro-ph.EP2025

Closeby Habitable Exoplanet Survey (CHES). IV. Synergy between astrometry and direct imaging missions of the Habitable World Observatory for detecting Earth-like planets

Chunhui Bao, Jianghui Ji, Dongjie Tan +4

The detection and characterization of habitable planets around nearby stars persist as one of the foremost objectives in contemporary astrophysics. This work investigates the syner…

astro-ph.EP2025

Closeby Habitable Exoplanet Survey (CHES). III. Retrieval of Planetary Masses in Binaries Using the N-body Model with RV and Astrometry Synergy

Xiumin Huang, Jianghui Ji, Chunhui Bao +4

Given that secular perturbations in a binary system not only excite high orbital eccentricities but also alter the planetary orbital inclination, the classical Keplerian orbital mo…