papers

Publications (72)

astro-ph.SR2025

Search for Past Stellar Encounters and the Origin of 3I/ATLAS

Yiyang Guo, Luyao Zhang, Fabo Feng +3

3I/ATLAS, the third discovered interstellar object, has a heliocentric speed of 58 km/s and exhibits cometary activity. To constrain the origin of 3I/ATLAS and its past dynamical e…

astro-ph.EP2025

A Population Synthesis Study on the Formation of Cold Jupiters from Truncated Planetesimal Disks

Kangrou Guo, Masahiro Ogihara, Shigeru Ida +3

The occurrence rate of giant planets increases with orbital period and turns over at a location that roughly corresponds to the snow line of solar-type stars. Further, the density…

astro-ph.EP2017

Evidence for at least three planet candidates orbiting HD20794

Fabo Feng, Mikko Tuomi, Hugh R. A. Jones

We explore the feasibility of detecting Earth analogs around Sun-like stars using the radial velocity method by investigating one of the largest radial velocities datasets for the…

astro-ph.EP2015

Finding the imprints of stellar encounters in long period comets

Fabo Feng, C. A. L. Bailer-Jones

The solar system's Oort cloud can be perturbed by the Galactic tide and by individual passing stars. These perturbations can inject Oort cloud objects into the inner parts of the s…

astro-ph.EP2020

A collage of small planets from the Lick Carnegie Exoplanet Survey : Exploring the super-Earth and sub-Neptune mass regime

Jennifer A. Burt, Fabo Feng, Bradford Holden +12

Analysis of new precision radial velocity (RV) measurements from the Lick Automated Planet Finder (APF) and Keck HIRES have yielded the discovery of three new exoplanet candidates…

astro-ph.EP2019

Detection of the nearest Jupiter analog in radial velocity and astrometry data

Fabo Feng, Guillem Anglada-Escudé, Mikko Tuomi +4

The presence of Jupiter is crucial to the architecture of the Solar System and models underline this to be a generic feature of planetary systems. We find the detection of the diff…

astro-ph.EP2016

A Goldilocks principle for modeling radial velocity noise

Fabo Feng, M. Tuomi, H. R. A. Jones +2

The doppler measurements of stars are diluted and distorted by stellar activity noise. Different choices of noise models and statistical methods have led to much controversy in the…

astro-ph.EP2018

Detection of the closest Jovian exoplanet in the Epsilon Indi triple system

Fabo Feng, Mikko Tuomi, Hugh R. A. Jones

We confirm the trend in the radial velocity data for Epsilon Indi A suggesting a long-period planetary companion and find significant curvature is present, sufficient to quantify E…

astro-ph.EP2026

Detection of four cold Jupiters through combined analyses of radial velocity and astrometry data

Yiyun Wu, Guang-Yao Xiao, R. Paul Butler +19

Cold Jupiters play a crucial role in planet formation and dynamical evolution. Since their initial discovery around 47 UMa, they have attracted significant interest, yet their form…

astro-ph.SR2019

Activity and telluric contamination in HARPS observations of Alpha Centauri B

Maksym Lisogorskyi, Hugh Jones, Fabo Feng

The Alpha Centauri system is the primary target for planet search as it is the closest star system composed of a solar twin Alpha Centauri A, a K-dwarf Alpha Centauri B and an M-dw…

astro-ph.EP2023

Mitigating astrometric bias in barycentric correction with PEXO

Yicheng Rui, Fabo Feng

Extremely precise radial velocity is essential for the detection of sub-m/s radial velocity of stars induced by Earth-like planets. Although modeling of the barycentric correction…

astro-ph.EP2020

Exploring the robustness of Keplerian signals to the removal of active and telluric features

Maksym Lisogorskyi, Hugh R. A. Jones, Fabo Feng +2

We examine the influence of activity- and telluric-induced radial velocity signals on high resolution spectra taken with an iodine absorption cell. We exclude 2 Angstrom spectral c…

astro-ph.EP2023

Forming Giant Planets Around Late-M Dwarfs: Pebble Accretion and Planet-Planet Collision

Mengrui Pan, Beibei Liu, Anders Johansen +6

We propose a pebble-driven core accretion scenario to explain the formation of giant planets around the late-M dwarfs of . In order to explore th…

astro-ph.EP2021

The Magellan-TESS Survey I: Survey Description and Mid-Survey Results

Johanna Teske, Sharon Xuesong Wang, Angie Wolfgang +66

revealed that roughly one-third of Sun-like stars host planets orbiting within 100 days and between the size of Earth and Neptune. How do these planets form, what are they…

astro-ph.EP2018

Minimizing the bias in exoplanet detection - application to radial velocities of LHS 1140

Fabo Feng, Mikko Tuomi, Hugh R. A. Jones

A rocky planet orbiting LHS 1140 with a period of 24.7d has been found based on the discovery of transits in its light and high precision radial velocity data (Dittmann et al. 2017…

astro-ph.EP2024

Astrometric detection of exoplanets

Fabo Feng

As the most ancient branch of astronomy, astrometry has been developed for thousands of years. However, it has only recently become possible to utilize astrometry for the detection…

astro-ph.EP2022

3-D selection of 167 sub-stellar companions to nearby stars

Fabo Feng, R. Paul Butler, Steven S. Vogt +20

We analyze 5108 AFGKM stars with at least five high precision radial velocity points as well as Gaia and Hipparcos astrometric data utilizing a novel pipeline developed in previous…

astro-ph.EP2024

HD 222237 b: a long period super-Jupiter around a nearby star revealed by radial-velocity and Hipparcos-Gaia astrometry

Guang-Yao Xiao, Fabo Feng, Stephen A. Shectman +16

Giant planets on long period orbits around the nearest stars are among the easiest to directly image. Unfortunately these planets are difficult to fully constrain by indirect metho…

astro-ph.IM2020

HiFLEx -- a highly flexible package to reduce cross-dispersed echelle spectra

Ronny Errmann, Neil Cook, Guillem Anglada-Escudé +8

We describe a flexible data reduction package for high resolution cross-dispersed echelle data. This open-source package is developed in Python and includes optional GUIs for most…

astro-ph.EP2025

Updated Mutual Inclination Measurement for 14 Her b and c

Guang-Yao Xiao, Fabo Feng

The mutual inclination between orbits within multi-planetary systems is difficult to measure directly. Through a joint analysis of RVs, Hipparcos-Gaia absolute astrometry and…

astro-ph.EP2026

HD 164604 c: a second giant planet on a 15-yr orbit and the constraint of the planet-planet mutual inclination

Guang-Yao Xiao, Fabo Feng, R. Paul Butler +4

We report the discovery of a new massive giant planet, HD 164604 c ( au, and or $7.6_{-1.0}…

astro-ph.IM2025

Architecture of Tianyu Software: Relative Photometry as a Case Study

Yicheng Rui, Yifan Xuan, Shuyue Zheng +8

Tianyu telescope, an one-meter robotic optical survey instrument to be constructed in Lenghu, Qinghai, China, is designed for detecting transiting exoplanets, variable stars and tr…

astro-ph.IM2024

The Jiao Tong University Spectroscopic Telescope Project

JUST Team, Chengze Liu, Ying Zu +28

The Jiao Tong University Spectroscopic Telescope (JUST) is a 4.4-meter f/6.0 segmentedmirror telescope dedicated to spectroscopic observations. The JUST primary mirror is composed…

astro-ph.EP2026

A universal brown dwarf desert formed between planets and stars

Kaiming Cui, Guang-Yao Xiao, Fabo Feng +10

Giant planets and brown dwarfs play a crucial role in star and planet formation, as they are situated at the boundary between planets and stars with uncertain formation mechanisms.…

astro-ph.SR2025

Detection of dark companions via the combination of eclipse timing variation, Hipparcos and/or Gaia astrometry: the cases of V Puppis and CY Ari

Guang-Yao Xiao, Fabo Feng, Song Wang +3

The third body is expected to shape the formation and evolution of close binary systems. In this work, we develop a method to detect and characterize the tertiary companion around…

astro-ph.IM2026

LenghuSky-8: An 8-Year All-Sky Cloud Dataset with Star-Aware Masks and Alt-Az Calibration for Segmentation and Nowcasting

Yicheng Rui, Xiao-Wei Duan, Licai Deng +9

Ground-based time-domain observatories require minute-by-minute, site-scale awareness of cloud cover, yet existing all-sky datasets are short, daylight-biased, or lack astrometric…

astro-ph.GA2018

Probabilistic galactic dynamics I - the Sun and GJ 710 with Monte Carlo, linearised and unscented treatments

Fabo Feng, Hugh R. A. Jones

Deterministic galactic dynamics is impossible due to the space-time randomness caused by gravitational waves. Instead of treating stellar orbits deterministically, we integrate not…

astro-ph.EP2018

The test case of HD26965: difficulties disentangling weak Doppler signals from stellar activity

Matías R. Díaz, James S. Jenkins, Mikko Tuomi +9

We report the discovery of a radial velocity signal that can be interpreted as a planetary-mass candidate orbiting the K dwarf HD26965, with an orbital period of 42.3640.015 d…

astro-ph.EP2019

PEXO: a global modeling framework for nanosecond timing, microsecond astrometry, and m/s radial velocities

Fabo Feng, Maksym Lisogorskyi, Hugh R. A. Jones +4

The ability to make independent detections of the signatures of exoplanets with complementary telescopes and instruments brings a new potential for robust identification of exoplan…

astro-ph.EP2025

Predicting the detection yields of giant planets and brown dwarfs with CSST astrometry

Yifan Xuan, Fabo Feng, Zhensen Fu +3

Chinese Space Station Telescope (CSST), which will begin its scientific operations around 2027, is going to survey the sky area of the median-to-high Galactic latitude and median-t…

astro-ph.EP2020

The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary

Ilaria Carleo, Davide Gandolfi, Oscar Barragán +110

We report the discovery of a warm Neptune and a hot sub-Neptune transiting TOI-421 (BD-14 1137, TIC 94986319), a bright (V=9.9) G9 dwarf star in a visual binary system observed by…

astro-ph.EP2020

Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs

Fabo Feng, Stephen A. Shectman, Matthew S. Clement +10

Earth-sized planets in the habitable zones of M dwarfs are good candidates for the study of habitability and detection of biosignatures. To search for these planets, we analyze all…

astro-ph.EP2024

Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581

Michelle Kunimoto, Zifan Lin, Sarah Millholland +43

We report the validation of multiple planets transiting the nearby ( pc) K5V dwarf HD 101581 (GJ 435, TOI-6276, TIC 397362481). The system consists of at least two Earth-…

astro-ph.IM2024

Tianyu: search for the second solar system and explore the dynamic universe

Fabo Feng, Yicheng Rui, Zhimao Du +32

Giant planets like Jupiter and Saturn, play important roles in the formation and habitability of Earth-like planets. The detection of solar system analogs that have multiple cold g…

astro-ph.EP2021

Identify Light-Curve Signals with Deep Learning Based Object Detection Algorithm. I. Transit Detection

Kaiming Cui, Junjie Liu, Fabo Feng +1

Deep learning techniques have been well explored in the transiting exoplanet field; however, previous work mainly focuses on classification and inspection. In this work, we develop…

astro-ph.EP2019

Search for nearby Earth analogs I. 15 planet candidates found in PFS data

Fabo Feng, Jeffrey D. Crane, Sharon Xuesong Wang +6

The radial velocity method plays a major role in the discovery of nearby exoplanets. To efficiently find planet candidates from the data obtained in high precision radial velocity…

astro-ph.EP2025

Breaking the Mass Inclination Degeneracy of Radial Velocity Measurements via Monitoring von Zeipel-Lidov-Kozai Cycles: Implications in the HD 41004 System

Zhizhen Qin, Shang-Fei Liu, Bo Ma +1

We investigate the dynamical stability of the S-type planet in the compact binary HD 41004. Using -body simulations, we find that the planet could be dynamically stable at a mut…

astro-ph.GA2025

A Cartesian catalog of 30 million Gaia sources based on second-order and Monte Carlo error propagation

Luyao Zhang, Fabo Feng, Yicheng Rui +2

Accurate measurements of stellar positions and velocities are crucial for studying galactic and stellar dynamics. We aim to create a Cartesian catalog from Gaia DR3 to serve as a h…

astro-ph.EP2020

Search for Nearby Earth Analogs. II. detection of five new planets, eight planet candidates, and confirmation of three planets around nine nearby M dwarfs

Fabo Feng, R. Paul Butler, Stephen A. Shectman +9

Zechmeister et al. (2009) surveyed 38 nearby M dwarfs from March 2000 to March 2007 with VLT2 and the UVES spectrometer. This data has recently been reanalyzed (Butler et al. 2019)…

astro-ph.GA2023

Binary Star Evolution in Different Environments: Filamentary, Fractal, Halo and Tidal-tail Clusters

Xiaoying Pang, Yifan Wang, Shih-Yun Tang +7

Using membership of 85 open clusters from previous studies (Pang et al. 2021a,b, 2022b; Li et al. 2021) based on Gaia DR3 data, we identify binary candidates in the color-magnitude…

astro-ph.SR2017

A catalogue of close encounter pairs

Fabo Feng, Hugh R. A. Jones, Tabassum S. Tanvir

We provide a catalogue of pairs of stars whose periapses are less than 1pc within the past or future 100 Myr. We use astrometric data from TGAS, Hipparcos and radial velocity data…

astro-ph.IM2024

Identifying Light-curve Signals with a Deep Learning Based Object Detection Algorithm. II. A General Light Curve Classification Framework

Kaiming Cui, D. J. Armstrong, Fabo Feng

Vast amounts of astronomical photometric data are generated from various projects, requiring significant effort to identify variable stars and other object classes. In light of thi…

astro-ph.SR2017

Was Proxima captured by alpha Centauri A and B?

Fabo Feng, Hugh R. A. Jones

The nearest stellar system consists of the stars Proxima, alpha Centauri A and B and at least one planet Proxima b. The habitability of Proxima b and any other planets are likely t…

astro-ph.GA2023

Unraveling the Complexity of Dwarf Galaxy Dynamics: A study of Binary Orbital Motions

Wenting Wang, Ling Zhu, Yipeng Jing +8

We investigate the impact of binary orbital motions on the dynamical modeling of dwarf galaxies with intrinsic line-of-sight velocity dispersions () of 1 to 9 km/s. Using…

astro-ph.EP2021

Optimized modeling of Gaia-Hipparcos astrometry for the detection of the smallest cold Jupiter and confirmation of seven low mass companions

Fabo Feng, R. Paul Butler, Hugh R. A. Jones +6

To fully constrain the orbits of low mass circumstellar companions, we conduct combined analyses of the radial velocity data as well as the Gaia and Hipparcos astrometric data for…

astro-ph.EP2015

Obliquity and precession as pacemakers of Pleistocene deglaciations

Fabo Feng, C. A. L. Bailer-Jones

The Milankovitch theory states that the orbital eccentricity, precession, and obliquity of the Earth influence our climate by modulating the summer insolation at high latitudes in…

astro-ph.EP2025

The NCORES Program: Precise planetary masses, null results, and insight into the planet mass distribution near the radius gap

David J. Armstrong, Ares Osborn, Remo Burn +39

NCORES was a large observing program on the ESO HARPS spectrograph, dedicated to measuring the masses of Neptune-like and smaller transiting planets discovered by the TESS satellit…

astro-ph.EP2020

Revisiting the HD 21749 Planetary System with Stellar Activity Modeling

Tianjun Gan, Sharon Xuesong Wang, Johanna K. Teske +26

HD 21749 is a bright ( mag) K dwarf at 16 pc known to host an inner terrestrial planet HD 21749c as well as an outer sub-Neptune HD 21749b, both delivered by TESS. Follow-up…

astro-ph.IM2025

Observatory Science with eXTP

Ping Zhou, Jirong Mao, Liang Zhang +97

Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in ast…

astro-ph.EP2023

Revised orbits of the two nearest Jupiters

Fabo Feng, R. Paul Butler, Steven S. Vogt +2

With its near-to-mid-infrared high contrast imaging capabilities, JWST is ushering us into a golden age of directly imaging Jupiter-like planets. As the two closest cold Jupiters,…

astro-ph.EP2026

A second visit to Eps Ind Ab with JWST: new photometry confirms ammonia and suggests thick clouds in the exoplanet atmosphere of the closest super-Jupiter

Elisabeth C. Matthews, James Mang, Aarynn L. Carter +9

With JWST, we are directly imaging cold (~200-300K), solar-age giant exoplanets for the first time. At these temperatures many molecular features appear and water-ice clouds may co…

astro-ph.EP2025

Segmented-Polynomial-fitting Least Squares (SPLS): An optimized algorithm to find Earth twins

Shuyue Zheng, Fabo Feng, Yicheng Rui

Detecting Earth twins remains challenging because their shallow, long-period transits are difficult to distinguish from background noise. Motivated by the challenge, we developed S…

astro-ph.EP2018

An improved quantification of HD 147379 b

Fabo Feng, Hugh R. A. Jones, Mikko Tuomi

We reanalyze the CARMENES and HIRES/KECK radial velocity data for HD 147379, and also analyze the SOPHIE data using the Agatha software in combination with MCMC posterior sampling.…

astro-ph.EP2023

Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions

Katherine Laliotis, Jennifer A. Burt, Eric E. Mamajek +22

Directly imaging temperate rocky planets orbiting nearby, Sun-like stars with a 6-m-class IR/O/UV space telescope, recently dubbed the Habitable Worlds Observatory, is a high prior…

astro-ph.EP2020

The Magellan/PFS Exoplanet Search: A 55-day period dense Neptune transiting the bright () star HD 95338

Matías R. Díaz, James S. Jenkins, Fabo Feng +14

We report the detection of a transiting, dense Neptune planet candidate orbiting the bright () K0.5V star HD 95338. Detection of the 55-day periodic signal comes from the an…

astro-ph.EP2026

The 3D Architecture of a pair of 6:1 Resonant Brown Dwarfs around the Naked-eye star Ophiuchi

Tianshenhong Sang, Guang-Yao Xiao, Ying-Yi Cao +8

We present a revisiting study of the brown dwarf pair orbiting the naked-eye () K-giant ~Ophiuchi, located only 44\,pc from our Solar system. By jointly analysing archiv…

astro-ph.SR2024

Modeling and Calibration of Gaia, Hipparcos, and Tycho-2 astrometric data for the detection of dark companions

Fabo Feng, Yicheng Rui, Yifan Xuan +1

Hidden within the Gaia satellite's multiple data releases lies a valuable cache of dark companions. To facilitate the efficient and reliable detection of these companions via combi…

astro-ph.EP2026

Cold giant discoveries from a joint radial-velocity and astrometry framework

Pablo A. Peña, James S. Jenkins, Fabo Feng +11

The population of long-period giant planets shapes planetary system architectures and formation pathways, but these cold Jupiters remain relatively unexplored. Radial velocity (RV)…

astro-ph.EP2020

TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert

Jennifer A. Burt, Louise D. Nielsen, Samuel N. Quinn +54

We report the detection of a transiting hot Neptune exoplanet orbiting TOI-824 (SCR J1448-5735), a nearby (d = 64 pc) K4V star, using data from the \textit{Transiting Exoplanet Sur…

astro-ph.EP2017

Color difference makes a difference: four planet candidates around tau Ceti

Fabo Feng, Mikko Tuomi, Hugh R. A. Jones +4

The removal of noise typically correlated in time and wavelength is one of the main challenges for using the radial velocity method to detect Earth analogues. We analyze radial vel…

astro-ph.EP2021

Constraints on the nearby exoplanet Ind Ab from deep near/mid-infrared imaging limits

Gayathri Viswanath, Markus Janson, Carl-Henrik Dahlqvist +16

The past decade has seen increasing efforts in detecting and characterising exoplanets by high contrast imaging in the near/mid-infrared, which is the optimal wavelength domain for…

astro-ph.EP2014

Exploring the role of the Sun's motion in terrestrial comet impacts

Fabo Feng, C. A. L. Bailer-Jones

The cratering record on the Earth and Moon shows that our planet has been exposed to high velocity impacts for much or all of its existence. Some of these craters were produced by…

astro-ph.EP2015

Investigations into the impact of astronomical phenomena on the terrestrial biosphere and climate

Fabo Feng

This thesis assesses the influence of astronomical phenomena on the Earth's biosphere and climate. I examine in particular the relevance of both the path of the Sun through the Gal…

astro-ph.IM2022

ET White Paper: To Find the First Earth 2.0

Jian Ge, Hui Zhang, Weicheng Zang +163

We propose to develop a wide-field and ultra-high-precision photometric survey mission, temporarily named "Earth 2.0 (ET)". This mission is designed to measure, for the first time,…

astro-ph.IM2026

AstroSkyFlow: an astronomical sky image flow simulator for time domain survey validation and machine learning

Kexin Li, Yicheng Rui, Fabo Feng +5

Modern time-domain optical surveys produce massive data volumes that require robust, high-fidelity simulated datasets for developing and validating automated pipelines and machine-…

astro-ph.EP2026

RVTESS I: Modeling Asteroseismic Signals with Simultaneous Photometry and RVs

Jiaxin Tang, Sharon X. Wang, Yaguang Li +22

Detecting small planets via the radial velocity method remains challenged by signals induced by stellar variability, versus the effects of the planet(s). Here, we explore using Gau…

astro-ph.EP2025

Lessons learned from the detection of wide companions by radial velocity and astrometry

Fabo Feng, Guang-Yao Xiao, Hugh R. A. Jones +3

The detection and constraint of the orbits of long-period giant planets is essential for enabling their further study through direct imaging. Recently, it has been highlighted that…

astro-ph.EP2021

TOI-1231 b: A Temperate, Neptune-Sized Planet Transiting the Nearby M3 Dwarf NLTT 24399

Jennifer A. Burt, Diana Dragomir, Paul Mollière +59

We report the discovery of a transiting, temperate, Neptune-sized exoplanet orbiting the nearby ( = 27.5 pc), M3V star TOI-1231 (NLTT 24399, L 248-27, 2MASS J10265947-5228099).…

astro-ph.EP2017

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

Fabo Feng, Mikko Tuomi, Hugh R. A. Jones

Periodograms are used as a key significance assessment and visualisation tool to display the significant periodicities in unevenly sampled time series. We introduce a framework of…

astro-ph.EP2020

TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet

Johanna Teske, Matías R. Díaz, Rafael Luque +44

The Transiting Exoplanet Survey Satellite mission was designed to find transiting planets around bright, nearby stars. Here we present the detection and mass measurement of a small…

astro-ph.EP2017

`Oumuamua as a messenger from the Local Association

Fabo Feng, Hugh R. A. Jones

With a hyperbolic trajectory around the Sun, `Oumuamua is the first confirmed interstellar object. However, its origin is poorly known. By simulating the orbits of 0.23 million loc…

astro-ph.SR2017

Understanding Fomalhaut as a Cooper pair

Fabo Feng, Hugh R. A. Jones

Fomalhaut is a nearby stellar system and has been found to be a triple based on astrometric observations. With new radial velocity and astrometric data, we study the association be…