Academia Sinica Institute of Astronomy & Astrophysics
中央研究院天文及天文物理研究所
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Planetary Sciences

Planetary Sciences

Probability map of the fraction of symmetric island twotinos (fS) and asymmetric twotinos in the leading island (fL), constrained by the observed population fractions of the symmetric and leading asymmetric islands ( fS,OSSOS, fL,OSSOS; i.e., the number of detections in each island should be the same as the ratio in the OSSOS sample). The rejected regions for this probability distribution are indicated with solid (99% confidence level) and dashed (95% confidence) white curves. Note that the absolute probabilities (color map) are low only because the cells have very high resolution; the contours correctly enclose the normalized probabilities. The fS and fL from Chiang & Jordan (2002), Li et al. (2014), Pike & Lawler (2017), and Lawler et al. (2019) are overplotted with dots and labeled.
Constraining Migration Models with the 2:1 Resonance
Rotation period and spin rate vs diameter for the FOSSIL JTs (orange dots). The same is shown for previously measured JTs (green dots) and MBAs as well (the background gray dots). The green, orange, and blue dashed lines indicate rotation periods of 5, 4, and 3 hr, respectively. Note that only the objects with full and half derived rotation periods in our samples are used in this plot. All half periods are doubled for comparison to objects with full periods.
The spin-rate limit of Jupiter Trojans
Rotation period and spin rate vs diameter for the FOSSIL JTs (orange dots). The same is shown for previously measured JTs (green dots) and MBAs as well (the background gray dots). The green, orange, and blue dashed lines indicate rotation periods of 5, 4, and 3 hr, respectively. Note that only the objects with full and half derived rotation periods in our samples are used in this plot. All half periods are doubled for comparison to objects with full periods.
The spin-rate limit of Jupiter Trojans
Lightcurves of an occultation of a background star by Pluto observed on 15 Aug. 2018 at OAN, SPM in Baja California, México. The lightcurves were collected at a cadence of 20 Hz using two of the TAOS II telescopes, one with a commercial Andor Zyla CMOS camera (grey) and one with the TAOS II prototype CIS107 CMOS camera (blue). The spikes in the middle of occultation event, which are consistent in both light curves, are scintillation events stemming from density waves in the atmosphere of Pluto.
Pluto Occultation 2018
Spectral energy distribution (wavelength vs. flux density) of the debris disc host star HD 105. Data points are coloured by wavelength regime: green for optical/near-infrared, blue for mid-infrared (including the Spitzer/IRS spectrum), and red for far-infrared (Herschel/PACS). White data points are ancilliary data, including ALMA 1.3mm and ATCA 9mm observations. Grey lines denote a grid of dust models (grain size and distribution) fitted to the data to determine the best-fit dust properties for the system.
Spectral energy distribution
ALMA Band 6 (1.3mm) naturally weighted image of HD 105, a young pre-main sequence star with a bright debris disc. The disc is spatially resolved, with a radius of ~ 80 au.
A Young Solar System Analogue Imaged by ALMA
Plot of distance vs. disc radius for a sample of 97 spatially resolved debris discs. The colour of each data point denotes the photospheric temperature of the host star. The size of each data point denotes the fractional width (dR/R) of the disc, assuming it is a Gaussian annulus. The black line denotes the limit at which a disc could be resolved by the Herschel satellite observatory. The small black dots denote discs with fractional widths of 0.1, 0.3, 0.5, and 1.0, respectively.
Disc radius as a function of stellar distance
Plot of stellar luminosity vs. disc temperature for a sample of 97 spatially resolved debris discs, taken from Marshall et al. (2021a). The dust temperature is plotted as a ratio with the blackbody temperature (i.e. Tdust/Tbb) at the observed location of the dust disc around each star. A general trend can be seen that the disc temperature tends toward the blackbody temperature for more luminous stars. This indicates that the dust grains responsible for the observed emission are larger around more luminous stars, as expected from dust grain removal through radiation pressure.
Dust temperature vs. stellar luminosity
Plot of stellar luminosity vs. disc radius for a sample of 97 spatially resolved debris discs, taken from Marshall et al. (2021a). The vertical error bars denote the width of the debris disc. Light grey lines denote samples randomly drawn from the posterior probability distribution of a power law fit to the distribution. An increasing trend between disc radius and stellar luminosity is observed, suggesting that larger discs are (generally) found around more luminous stars. The slope of this trend is what would be expected if the CO ice line in primordial protoplanetary discs were responsible for setting the location for planetesimal formation around the host stars.
A Trend in Stellar Luminosity-Disc Radius
The number of new visible Jupiter Family Comets (JFCs) produced by each mean motion resonance (MMR) with Neptune, in our numerical simulations including the 34 largest dwarf planets (DPs, red line) or only the giant planets (black line).
Contribution of several MMRs populations to the production of JFCs
A figure representing the different possible combinations of the contributions of each of the three populations of the Kuiper belt (Classical, Resonant, and Scattering), to the total Jupiter Family Comet (JFC) production.
Number of cometary nuclei required to sustain a population of JFCs in steady state.
Diffusion is computed after a frequency analysis of thousands of test particles. Bluer colors are for stable orbits, redder colors indicate unstable ones.
Diffusion map around the small moon Aegaeon (Saturn LIII).
g-r and r-z photometry of TNOs, showing the 3 unique surface types revealed by these three bands.
TNO surface colors in g, r, and z bands
The three TAOS II enclosures at San Pedro Mártir Observatory.
TAOS II enclosures at San Pedro Mártir Observatory
TAOS II telescope at Site #2.
TAOS II Telescope.
Weather map of the transiting hot Jupiter HD 189733b, illustrated by air pressure (color) and wind velocity fields (arrows), as viewed by someone who descends through the planetary atmosphere. The patters are generated primarily by equatorial Rossby waves on the highly irradiated planet. These waves lead to the equatorial super-rotating circulation, which reduces the day-night temperature contrast of this tidally locked exoplanet. The circulation model also explains why the maximum thermal flux from the planet occurs several hours before secondary eclipse, an observational result revealed by the Spitzer Space Telescope (Tsai, Dobbs-Dixon, Gu, ApJ, 2014, 794, 141).
Weather on a Hot Jupiter
Orbit diagram of the planetary system surrounding the K-dwarf star HD 40307. The grey area indicates the star's habitable zone. Notice that the outermost planet is right in the habitable zone.
A super Earth in the habitable zone_animation gif
A back-scattered image of the E44 CAI from the CV3 Efremovka chondrite taken on a scanning electron microscope. This CAI is of particular interest because of the first demonstration of the former existence of short-lived 41Ca (t1/2 = 0.1 Myr). Reanalysis of potassium isotopes of this CAI (on the dark-gray minerals, named fassaite) resulted in a lower initial ratio of 41Ca/40Ca in the solar system from 1.4e-8 to 2.6e-9. A factor of 5 difference has an important implication for the origin of 41Ca and of the solar system.
A back-scattered image of the E44 CAI from the CV3 Efremovka chondrite taken on a scanning electron microscope
This isochron diagram shows the inferred 41Ca/40Ca ratio in the E44 CAI from the Efremovka meteorite. 20 years ago, the former existence of 41Ca (half-life = 0.1 Myr) was first demonstrated in this CAI, with the inferred 41Ca/40Ca ratio = 1.4e-8 (long dashed line). Reanalysis of K isotopes in the same CAI with an advanced secondary ion mass spectrometer revealed a 5-time lower 41Ca/40Ca ratio of 2.6e-9. This discovery has important implications for the origin of short-lived radionuclides in the early solar System.
A new initial abundance of 41Ca in the early solar system
Inferred 26Al/27Al ratios for spinel-hibonite spherules from Murchison and Paris and the probability density plot derived from the data. The overall 26Al/27Al range in the two groups of SHIBs is essentially identical, from ~1E−5 up to 6E−5. Three distinctive peaks can be identified in the probability plot at 26Al/27Al=4.9E−5, ~3.5E−5 and 6.5E−5, respectively. Two barely resolved components at 6E−5 and 2.5E−5 are also revealed.
The distribution of 26Al/27Al in spinel-hibonite spherules extracted from CM chondrites

We have a growing community of planetary scientists ASIAA who are involved in a wide range of research topics covering both theoretical modeling and observations of our own solar system and those of other stars.

For our own solar system, ASIAA is playing a leading role in two large surveys. The Transneptunian Automated Occultation Survey(TAOS II) aims to measure the size distribution of Trans-Neptunian Objects (TNOs) and objects in the Inner Oort Cloud. TAOS II will operate at the San Pedro Mártir Observatory in Baja California, Mexico. The survey will observe up to 10,000 stars simultaneously with three 1.3 m telescopes at a cadence of 20 Hz in order to resolve short duration (200 ms) occultation events by TNOs with diameters 300 m < D < 30 km. These objects are too faint to be observed directly, even with the largest telescopes. However, measuring the size distribution of these objects is critical to our understanding of the formation and evolution of the solar system. Furthermore, the target population of these observations is the source of the Jupiter Family Comets (JFCs), and a census of this reservoir is important to understand the dynamical processes by which these TNOs migrate into cometary orbits.

In addition to TAOS II, ASIAA is a major partner of the FOSSIL Survey (Formation of the Outer Solar System: An Icy Legacy). FOSSIL, an Intensive Program of the Subaru telescope using the Hyper Suprime-Cam (HSC) wide field camera, is a large international collaboration including Taiwan, Japan, South Korea, China, New Zealand, Canada, and the United States. The survey will cover 105 deg. 2 to as faint as r = 27 in order to detect and characterize small solar system bodies such as TNOs, Jupiter Trojans, Hildas, and Main Belt and Near Earth Asteroids. Phase I of the project, which aimed to measure the spin rates of JTs and Hildas, as well as measure the faint end size distributions of faint TNOs, JTs and Hildas, covered 30 deg. 2 of both the L4 and L5 JT clouds at a high cadence in order to measure the spin rates of JTs and Hildas in order to ascertain their internal structures (monolithic or gravitational aggregates), as well as detect very faint TNOs. Phase II of the proposal would concentrate on a three year survey of TNOs covering 75 deg. 2 to detect objects as faint as r = 26. By observing the objects over three years, the survey will be able to constrain their orbits sufficiently to classify them into their dynamical sub-populations. Color measurements will also be performed, which in conjunction with size distribution measurements and dynamical classifications, will allow the survey team to support or contravene the Planet 9 hypothesis, discover evidence of the formation histories of the different TNO dynamical classes, constrain models of the migration of Neptune and the collisional history of TNOs.

Several members of the planetary science group at ASIAA are performing large scale dynamical simulations of the outer solar system. In particular, investigation of the effect of the population of Dwarf Planets (DPs) in the Trans-Neptunian region has shown that they increase the migration rate of TNOs into cometary orbits relative to the rate found when only considering gravitational interactions with Neptune. In addition, DPs contribute to the long term instability of the orbits of many TNOs, leading to their eventual ejection from the solar system.

Similar simulations of the Centaur population have shown that some of these objects are in stable three-body resonances with Jupiter and Saturn. In addition, the orbits of the moons of Saturn, Pallene in particular, are being simulated to determine their resonant structures.

Outside of our solar system, the planetary science group at ASIAA is working on a wide range of topics, from protoplanetary and debris disks to evolved systems with exoplanets and exomoons. Observations of protoplanetary disks using the Atacama Large Millimeter/submillimeter Array (ALMA) are being used to discover and characterize various features in these structures such as gas rings, spiral inflow, pressure bumps, and disk eccentricities. Some of these features may be intimately related to planet formation processes, and it is thus important to learn as much as possible about these features.

Members of the ASIAA planetary science group are also involved in many aspects of debris disc studies, performing detailed multi-wavelength studies on the architectures of individual systems using ground- and space-based observing facilities such as ALMA, the Herschel space observatory, the Hubble Space Telescope (HST), and the Very Large Telescope (VLT) with the Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) facility, piecing together their evolution and searching for trends in the star/disc properties through systematic characterization of spatially resolved discs, modeling the composition of the constituent dust grains (and parent planetesimals) combining radiative transfer modeling and laboratory dust measurements, tracing the dynamical evolution of planetesimal belts under the influence of planetary companions, and searching for exocomets and their parent planetesimal belts around young stars in nearby open clusters.

Finally, significant research efforts are being made in the area of evolved planetary systems. Planet formation and evolution around FGKM dwarfs are being modeled to interpret Kepler/K2 data and to prepare for the science from the SPectropolarimètre InfraROUge (SPIRou) instrument on the Canada-France-Hawaii Telescope (CFHT). The theory of thermal tides is being investigated to examine whether this model can explain the anomalously large size of hot Jupiters. Simulations of the formation of short period exoplanets have led to the prediction of co-orbital planets, and subsequent work is now being done to examine the possibility of discovering such systems in data from the Kepler/K2 or the Transiting Exoplanet Survey Satellite (TESS) missions. Other research is focusing on exomoons, in particular, developing new approaches for identifying moon signals in Kepler/K2 and TESS data, as well as targeted observations using the HST or the James Webb Space Telescope (JWST). Recent work also includes modeling and interpreting the transit timing variations of planets hosting multiple moons.

Research Members (17)

Shang, Hsien 尚賢 cv Research Fellow
Research Interest: Origins of Solar Systems, Meteorites, Planetary material, CAIs, Chondrules, and Isotopes
Wang, Shiang-Yu 王祥宇 cv Research Fellow
Research Interest: Infrared sensor, Optical/Infrared Instrumentation, Semiconductor devices
Lin, Min-Kai 林明楷 cv Associate Research Fellow (Tenured)
Research Interest: planet formation, disk-planet interaction, planet migration, accretion disks
Gu, Pin-Gao 辜品高 cv Associate Research Fellow
Research Interest: exoplanets, protoplanetary disks, interstellar shocks
Wen, Chih-Yi 溫志懿 cv Senior Research Engineer
Research Interest: Instrument Software Engineering, High Energy Physics
Wang, Jen-Hung 汪仁鴻 cv EPO office manager, Assistant Research Scientist
Research Interest: Optical Astronomy, Solar System Minor Bodies, Occultation Prediction, Solar System Ephemeris
Kuan, Yi-Jehng 管一政 cv Joint Research Fellow; Dept. Earth Sciences, NTNU
Research Interest: Astrochemistry, Molecular Astrophysics, Molecular Clouds and Astrobiology
Chang, Rex Chan-Kao 章展誥 cv Visiting Scholar
Research Interest: Rotation period
Marshall, Jonathan 馬恩迪 cv NSTC Research Scholar
Research Interest: Exoplanets; dynamics, disc-planet interactions
Chen, Ying-Tung 陳英同 cv Support Scientist
Research Interest: Optical data pipeline, Solar System Astronomy
Granados Contreras, Agueda Paula 戈葆拉 cv Support Scientist
Research Interest: Exoplanets and orbital dynamics
Huang, Chung-Kai 黃鍾凱 cv Support Scientist
Research Interest: Solar System, Trans-Neptunian Objects, Stellar Occultations, Astronomy Data Modeling, Time Domain Astronomy, Light Curves
King, Sun-Kun 金升光 cv Program Facilitator
Research Interest: Kuiper belt objects; Diffraction due to occultation
Otten, Gilles Peter Paul Louis 歐碁爾 cv Support Scientist
Research Interest: optical and infrared instrumentation, exoplanets
Zhang, Zhi-Wei Kiwi 張智威 cv TAOS Support Engineer/Scientist
Research Interest: Trans-Neptunian Objects in outer Solar System
Teachey, Alexander 齊孝嵐 cv Distinguished Postdoc Fellow
Research Interest: exoplanets, exomoons, machine learning, big data, detection methods
Lehner, Matthew 連馬修 cv RCUH Research Fellow / Chief Scientist TAOS-2
Research Interest: Optical Astronomy,Trans-Neptunian Objects

Journal Papers (160)

  1. Narang M; Manoj P; Chandra CHI; Banerjee B; Tyagi H; Tamura M; Henning T; Mathew B; Lazio J; Surya A; Nayak PK, "A uGMRT search for radio emission from planets around evolved stars" , MNRAS: 529(2), 1161-1168, Apr, 2024 [SCI] ( ADS | Fulltext )
  2. Teachey A; Agarwal G, "On the impact and utility of single-exomoon modelling for multimoon systems" , MNRAS: 529(2), 1232-1249, Apr, 2024 [SCI] ( ADS | Fulltext )
  3. Smallwood JL; Yang C-C; Zhu Z; Martin RG; Dong R; Cuello N; Isella A, "Exciting spiral arms in protoplanetary discs from flybys" , MNRAS: 521(3), 3500-3516, May, 2023 [SCI] ( ADS | Fulltext )
  4. Kuo IHG; Yen H-W; Gu P-G; Chang T-E, "Kinematical Constraint on Eccentricity in the Protoplanetary Disk MWC 758 with ALMA" , ApJ: 938(1), id.50 (13pp), Oct, 2022 [SCI] ( ADS | Fulltext )
  5. Chang C-K; Chen Y-T; Fraser WC; Yoshida F; Lehner MJ; Wang S-Y; Kavelaars J; Pike RE; Alexandersen M; Ito T; Choi Y-J; Granados Contreras AP; Jeongahn Y; Ji J; Kim M-J; Lawler SM; Li J; Lin Z-Y; Lykawka PS; Moon H-K; More S; Munoz-Gutierrez M; Ohtsuki K; Terai T; Urakawa S; Zhang H; Zhao H-B; The FOSSIL Collaboration, "FOSSIL. I. The Spin Rate Limit of Jupiter Trojans" , The Planetary Science Journal: 2(5), id.191 (11pp), Oct, 2021 [SCI] ( ADS | Fulltext )
  6. Dharmawardena TE; Barlow MJ; Drew JE; Seales A; Sale SE; Jones D; Mampaso A; Parker QA; Sabin L; Wesson R, "H α fluxes and extinction distances for planetary nebulae in the IPHAS survey of the northern galactic plane" , MNRAS: 501(4), 6156-6167, Mar, 2021 [SCI] ( ADS | Fulltext )
  7. Hsieh HH; Chandler CO; Denneau L; Fitzsimmons A; Erasmus N; Kelley MSP; Knight MM; Lister TA; Pittichová J; Sheppard SS; Thirouin A; Trujillo CA; Usher H; Gomez E; Chatelain J; Greenstreet S; Angel T; Miles R; Roche P; Wooding B, "Physical Characterization of Main-belt Comet (248370) 2005 QN173" , ApJL: 922 (1), id.L9 (10pp), Nov, 2021 [SCI] ( ADS | Fulltext )
  8. Huang C-K; Lehner MJ; Granados Contreras AP; Castro-Chacón JH; Chen W-P; Alcock C; Alvarez-Santana FI; Cook KH; Geary JC; Guerrero Peña CA; Hernández-Ñguila JB; Hernández-Valencia B; Karr J; Kavelaars JJ; Norton T; Nuñez JM; Ochoa D; Reyes-Ruiz M; Sánchez E; Silva JS; Szentgyorgyi A; Wang S-Y; Yen W-L; Zhang Z-W, "The TAOS II Survey: Real-time Detection and Characterization of Occultation Events" , PASP: 133(1021), id.34503 (17pp), Mar, 2021 [SCI] ( ADS | Fulltext )
  9. Lin Y-C; Matsumoto Y; Gu P-G, "Formation of multiple-planet systems in resonant chains around M dwarfs" , ApJ: 907(2), id.81 (11pp), Feb, 2021 [SCI] ( ADS | Fulltext )
  10. Lin Z-YD; Lee C-F; Li Z-Y; Tobin JJ; Turner NJ, "Inferring (sub)millimetre dust opacities and temperature structure in edge-on protostellar discs from resolved multiwavelength continuum observations: the case of the HH 212 disc" , MNRAS: 501(1), 1316-1335, Feb, 2021 [SCI] ( ADS | Fulltext )
  11. Matsumoto Y; Kokubo E; Gu P-G; Kurosaki K, "Size evolution of close-in super-Earths through giant impacts and photoevaporation" , ApJ: 923(1), id.81 (17pp), Dec, 2021 [SCI] ( ADS | Fulltext )
  12. Muñoz-Gutiérrez MA; Peimbert A; Lehner MJ; Wang S-Y, "Long-term Dynamical Stability in the Outer Solar System I: The Regular and Chaotic Evolution of the 34 Largest Trans-Neptunian Objects" , AJ: 162(4), id.164 (13pp), Oct, 2021 [SCI] ( ADS | Fulltext )
  13. Auddy S; Lin M-K, "A Machine Learning Model to Infer Planet Masses from Gaps Observed in Protoplanetary Disks" , ApJ: 900(1), id.62 (12pp.), Sep, 2020 [SCI] ( ADS | Fulltext )
  14. Marshall JP; Horner J; Wittenmyer RA; Clark JT; Mengel MW, "Stability analysis of three exoplanet systems" , MNRAS: 494(2), 2280-2288, Apr, 2020 [SCI] ( ADS | Fulltext )
  15. Matsumoto Y; Gu P-G; Kokubo E; et al., "Ejection of close-in super-Earths around low-mass stars in the giant impact stage" , A&A: 642, id.A23 (10pp.), Oct, 2020 [SCI] ( ADS | Fulltext )
  16. Matsumoto Y; Ogihara M, "Breaking Resonant Chains: Destabilization of Resonant Planets Due to Long-term Mass Evolution" , ApJ: 893(1), id.43 (12pp.), Apr, 2020 [SCI] ( ADS | Fulltext )
  17. Pike RE; Proudfoot BCN; Ragozzine D; Alexandersen M; ...; Chen Y-T; et al., "A dearth of small members in the Haumea family revealed by OSSOS" , Nature Astronomy: 4(1), 89-96, Jan, 2020 [SCI] ( ADS | Fulltext )
  18. Yen H-W; Gu P-G, "Kinematical signs of dust trapping and feedback in a local pressure bump in the protoplanetary disk around HD 142527 revealed with ALMA" , ApJ: 905(2), id.89 (16 pp.), Dec, 2020 [SCI] ( ADS | Fulltext )
  19. Chen Y-T; Gladman B; Volk K; ...; Lehner MJ; ...; Wang S-Y; ...; Alexandersen M; et al., "OSSOS. XVIII. Constraining Migration Models with the 2:1 Resonance Using the Outer Solar System Origins Survey" , ApJ: 158(5), id. 214 (17 pp.), Nov, 2019 [SCI] ( ADS | Fulltext )
  20. Gu P-G; Peng D-K; Yen C-C, "Modeling the Thermal Bulge of a Hot Jupiter with the Two-stream Approximation" , ApJ: 887(2), id. 228 (15 pp.), Dec, 2019 [SCI] ( ADS | Fulltext )
  21. Marshall JP; Wittenmyer RA; Horner J; et al., "Re-analyzing the Dynamical Stability of the HD 47366 Planetary System" , AJ: 157(1), id. 1 (11 pp.), Jan, 2019 [SCI] ( ADS | Fulltext )
  22. Matsumoto Y; Wakita S; Hasegawa Y; Oshino S, "Aggregate Growth and Internal Structures of Chondrite Parent Bodies Forming from Dense Clumps" , ApJ: 887(2), id. 248 (22 pp.), Dec, 2019 [SCI] ( ADS | Fulltext )
  23. Muñoz-Gutiérrez MA; Peimbert A; Pichardo B; Lehner MJ;Wang S-Y, "The Contribution of Dwarf Planets to the Origin of Jupiter Family Comets" , AJ: 158(5), id. 184 (14 pp.), Nov, 2019 [SCI] ( ADS | Fulltext )
  24. Schwamb ME; Fraser WC; Bannister MT; ...; Pike RE; ...; Lehner MJ; Wang S-Y; ...; Alexandersen M; Chen Y-T ;et al., "Col-OSSOS: The Colors of the Outer Solar System Origins Survey" , ApJS: 43(1), id. 12 (24 pp.), Jul, 2019 [SCI] ( ADS | Fulltext )
  25. Yen H-W; Gu P-G; Hirano N; Koch PM; Lee C-F; Liu HB; Takakuwa S, "HL Tau Disk in HCO+ (3-2) and (1-0) with ALMA: Gas Density, Temperature, Gap, and One-arm Spiral" , ApJ: 880(2), id. 69 (18 pp.), Aug, 2019 [SCI] ( ADS | Fulltext )
  26. Yen H-W; Takakuwa S; Gu P-G; Hirano N; Lee CF; Liu HB; Liu SY; Wu CJ, "Signs of outflow feedback from a nearby young stellar object on the protostellar envelope around HL Tauri" , A&A: 623, id. A96 (20 pp.), Mar, 2019 [SCI] ( ADS | Fulltext )
  27. Chen J-W; Lin M-K, "Dusty disc-planet interaction with dust-free simulations" , MNRAS: 478(2), 2737-2752, Aug, 2018 [SCI] ( ADS | Fulltext )
  28. Chen Y-T; Lin H-W; Alexandersen M; Lehner MJ; Wang S-Y; Wang J-H; et al., "Searching for moving objects in HSC-SSP: Pipeline and preliminary results" , PASJ: 70(SP1), S38 (17 pp.), Jan, 2018 [SCI] ( ADS | Fulltext )
  29. Hsieh HH; Kim Y; Fitzsimmons A; Sykes MV, "Search for Dust Emission from (24) Themis Using the Gemini-North Observatory" , PASP: 130 (990), 084402 (9 pp.), Aug, 2018 [SCI] ( ADS | Fulltext )
  30. Hsieh HH; Novaković B; Kim Y; Brasser R, "Asteroid Family Associations of Active Asteroids" , AJ: 155(2), 96, Feb, 2018 [SCI] ( ADS | Fulltext )
  31. Lin M-K; Pierens A, "Vortex survival in 3D self-gravitating accretion discs" , MNRAS: 478(1), 575-591, July, 2018 [SCI] ( ADS | Fulltext )
  32. Muñoz-Gutiérrez MA; Peimbert A; Pichardo B, "The Contribution of Dwarf Planets to the Origin of Low-inclination Comets by the Replenishment of Mean Motion Resonances in Debris Disks" , AJ: 156(3), id. 108 (12 pp.), Sep, 2018 [SCI] ( ADS | Fulltext )
  33. Schwamb ME; Aye K-M; Portyankina G; et al., "Planet Four: Terrains - Discovery of araneiforms outside of the South Polar layered deposits" , Icarus: 308, 148-187, July, 2018 [SCI] ( ADS | Fulltext )
  34. Hsieh HH, "Asteroid-comet continuum objects in the solar system" , Philosophical Transactions of the Royal Society A: 375(2097), 20160259, May, 2017 [SCI] ( ADS | Fulltext )
  35. Lin M-K; Youdin AN, "A Thermodynamic View of Dusty Protoplanetary Disks" , ApJ: 849(2), 129, Nov 10, 2017 [SCI] ( ADS | Fulltext )
  36. Pike RE; Fraser WC; Schwamb ME;...; Lehner MJ; Wang S-Y; Alexandersen M; Chen Y-T; et al., "Col-OSSOS: z-Band Photometry Reveals Three Distinct TNO Surface Types" , AJ: 154(3), 101, Sept, 2017 [SCI] ( ADS | Fulltext )
  37. Pike RE; Lawler,S; Brasser R; Shankman CJ; Alexandersen M; Kavelaars JJ, "The Structure of the Distant Kuiper Belt in a Nice Model Scenario" , AJ: 153(3), 127, March, 2017 [SCI] ( ADS | Fulltext )
  38. Alexandersen M; Gladman B; Kavelaars JJ; ...; Pike RE, "A Carefully Characterized and Tracked Trans-Neptunian Survey: The Size distribution of the Plutinos and the Number of Neptunian Trojans" , ApJ: 152(5), 111, Nov, 2016 [SCI] ( ADS | Fulltext )
  39. Chen Y-T; Lin HW; Holman MJ; ...; Wang SY; Lehner MJ, "Discovery of a New Retrograde Trans-Neptunian Object: Hint of a Common Orbital Plane for Low Semimajor Axis, High-inclination TNOs and Centaurs" , ApJL: 827(2), 24, Aug 20, 2016 [SCI] ( ADS | Fulltext )
  40. Hirashita H; Koch PM; Matsushita S; Takakuwa S; Nakamura M; Asada K; Liu HB; Urata U; Wang M-J; Wang W-H; Takahashi S; Tang Y-W; Chang H-H; Huang K; Morata O; Otsuka M; Lin K-Y; Tsai A-L; Lin Y-T; Srinivasan S; Martin-Cocher P; Pu J-Y; Kemper F; Patel N; Grimes P; Huang Y-D; Han C-C; Huang Y-R; Nishioka H; Lin C-CL; Zhang Q; Keto E; Burgos R; Chen M-T; Inoue M; Ho PTP, "First-generation Science Cases for Ground-based Terahertz Telescopes" , PASJ: 68(1), R1, Feb, 2016 [SCI] ( ADS | Fulltext )
  41. Yen H-W; Liu HB; Gu P-G; Hirano N; Lee C-F ; Puspitaningrum E; Takakuwa S, "Gas Gaps in the Protoplanetary Disk around the Young Protostar HL Tau" , ApJL: 820(2), L25, April 1, 2016 [SCI] ( ADS | Fulltext )
  42. Hsieh HH; Denneau L; Wainscoat RJ; et al., "The main-belt comets: The Pan-STARRS1 perspective" , Icarus: 248, 289-312, Mar 1, 2015 [SCI] ( ADS | Fulltext )
  43. Hsieh HH; Hainaut O; Novaković B; et al., "Sublimation-Driven Activity in Main-Belt Comet 313p/Gibbs" , ApJL: 800(1), L16, Feb 10, 2015 [SCI] ( ADS | Fulltext )
  44. Lee W-K; Gu P-G, "The Effect of Vertical Temperature Gradient on the Propagation of Three-dimensional Waves in a Protoplanetary Disk" , ApJ: 814(1), 72, Nov 20, 2015 [SCI] ( ADS | Fulltext )
  45. Brasser R; Ida S; Kokubo E, "A dynamical study on the habitability of terrestrial exoplanets II: The super Earth HD 40307 g" , MNRAS: 440(4), 3685-3700, June, 2014 [SCI] ( ADS | Fulltext )
  46. Hasegawa Y; Hirashita H, "Planet Traps and First Planets: the Critical Metallicity for Gas Giant Formation" , ApJ: 788(1), 62, June 10, 2014 [SCI] ( ADS | Fulltext )
  47. Hasegawa Y; Pudritz RE, "Planet Traps and Planetary Cores: Origins of the Planet-Metallicity Correlation" , ApJ: 794(1), 25, Oct 10, 2014 [SCI] ( ADS | Fulltext )
  48. Hsieh HH, "The nucleus of main-belt Comet P/2010 R2 (La Sagra)" , Icarus: 243, 16-26, Nov, 2014 [SCI] ( ADS | Fulltext )
  49. Hsieh HH; et al., "Search for the return of activity in active asteroid 176P/LINEAR" , AJ: 147(4), 89, April, 2014 [SCI] ( ADS | Fulltext )
  50. Liu M-C, "On the Injection of Short-lived Radionuclides from a Supernova into the Solar Nebula: Constraints from the Oxygen Isotopes" , ApJL: 781(2), L28, Feb, 2014 [SCI] ( ADS | Fulltext )
  51. Schwamb ME, "Solar System: Stranded in no-man's-land" , Nature: 507(7493), 435-436, March, 2014 [SCI] ( ADS | Fulltext )
  52. Schwamb ME; Brown ME; Fraser WC, "The Small Numbers of Large Kuiper Belt Objects" , AJ: 147(1), 2, Jan, 2014 [SCI] ( ADS | Fulltext )
  53. Takami M; Hasegawa Y; Muto T; ...; Gu P-G; Dong R; Karr JL; ...; Chapillon E; Tang Y-W; et al., "Surface Geometry of Protoplanetary Disks Inferred From Near-Infrared Imaging Polarimetry" , ApJ: 795(1), 71, Nov, 2014 [SCI] ( ADS | Fulltext )
  54. Tang Y-W; Dutrey A; Guilloteau S; ...; Ho PTP; et al., "Circumbinary Ring, Circumstellar Disks, and Accretion in the Binary System UY Aurigae" , ApJ: 793(1), 10, Sept 20, 2014 [SCI] ( ADS | Fulltext )
  55. Tsai S-M; Dobbs-Dixon I; Gu P-G, "Three-dimensional Structures of Equatorial Waves and the Resulting Super-rotation in the Atmosphere of a Tidally Locked Hot Jupiter" , ApJ: 793(2), 141, Oct, 2014 [SCI] ( ADS | Fulltext )
  56. Wang J-H; Brasser R, "An Oort cloud origin of the Halley-type comets" , A&A: 563, A122, Mar, 2014 [SCI] ( ADS | Fulltext )
  57. Chang Y-L; Bodenheimer PH; Gu P-G, "Coupled Evolutions of the Stellar Obliquity, Orbital Distance, and Planet's Radius due to the Ohmic Dissipation Induced in a Diamagnetic Hot Jupiter around a Magnetic T Tauri Star" , ApJ: 757(2), 118, Oct 1, 2012 [SCI] ( ADS | Fulltext )
  58. Hsieh H-F; Gu P-G, "On the Secular Behavior of Dust Particles in an Eccentric Protoplanetary Disk with an Embedded Massive Gas Giant Planet" , ApJ: 760(2), 119, Dec 1, 2012 [SCI] ( ADS | Fulltext )
  59. Chang SH; Gu PG; Bodenheimer PH, "Tidal and Magnetic Interactions Between a Hot Jupiter and its Host Star in the Magnetospheric Cavity of a Protoplanetary Disk" , ApJ: 708(2), 1692-1702, Jan 10, 2010 [SCI] ( ADS | Fulltext )
  60. Gu PG, "[News & Views] Extrasolar planets: Larger than they ought to be" , Nature: 465(7296), 300-301, May 20, 2010 [SCI] ( ADS | Fulltext )
  61. Liu MC; Nittler LR; Alexander CMO; Lee T, "Protosolar Irradiation in the Early Solar System: A Hibonite Perspective" , Meteorit Planet Sci: 45, A120, Jul, 2010 [SCI] ( ADS | Fulltext )
  62. Gu PG; Ogilvie GI, "Diurnal thermal tides in a non-synchronized hot Jupiter" , MNRAS: 395(1), 422-435, May 1, 2009 [SCI] ( ADS | Fulltext )
  63. Gu PG; Suzuki TK, "Thermal Response of a Solar-like Atmosphere to an Electron Beam from a Hot Jupiter: A Numerical Experiment" , ApJ: 705(2), 1189-1195, Nov 10, 2009 [SCI] ( ADS | Fulltext )
  64. Gu PG; Shkolnik E; Li SL; et al., "Interactions between hot Jupiters and their host stars" , AN: 326(10), 909-912, Dec, 2005 [SCI] ( ADS | Fulltext )
  65. Gu PG; Bodenheimer PH; Lin DNC, "The Internal Structural Adjustment Due to Tidal Heating of Short-Period Inflated Giant Planets" , ApJ: 608(2), 1076-1094, Jun 20, 2004 [SCI] ( ADS | Fulltext )
  66. Gu PG; Lin DNC; Bodenheimer PH, "The effect of tidal inflation instability on the mass and dynamical evolution of extrasolar planets with ultrashort periods" , ApJ: 588(1), 509-534, May 1, 2003 [SCI] ( ADS | Fulltext )
  67. Shu FH; Shang H; Gounelle M; Glassgold AE; Lee T, "Making calcium-aluminum-rich inclusions and chondrules near the young sun by flares" , Meteorit Planet Sci: 35 Supplement, A145-A146, Sep, 2000 [SCI] ( ADS | Fulltext )
  68. Dalba PA; Kane SR; Isaacson H; Fulton B; Howard AW; Schwieterman EW; Thorngren DP; Fortney J; Vowell N; Beard C; Blunt S; Brinkman CL; Chontos A; Dai F; Giacalone S; Hill ML; Kosiarek M; Lubin J; Mayo AW; Močnik T; Akana Murphy JM; Petigura EA; Rice M; Rubenzahl RA; Van Zandt J; Weiss LM; Dragomir D; Kipping D; Payne MJ; Roy A; Teachey A; Villanueva S, "Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets" , ApJS: 271(1), 16 (25pp), Mar, 2024 [SCI] ( ADS | Fulltext )
  69. Fraser WC; Pike RE; Marsset M; Schwamb ME; Bannister MT; Buchanan L; Kavelaars JJ; Benecchi SD; Tan NJ; Peixinho N; Gwyn SDJ; Alexandersen M; Chen Y-T; Gladman B; Volk K, "Col-OSSOS: The Two Types of Kuiper Belt Surfaces" , The Planetary Science Journal: 4(5), id.80 (15pp), May, 2023 [SCI] ( ADS | Fulltext )
  70. Kiefer F; Hébrard G; Martioli E; Artigau E; Doyon R; Donati J-F; Cadieux C; Carmona A; Ciardi DR; Cristofari PI; de Almeida L; Figueira P; Gaidos E; Gonzales E; Lecavelier Des Etangs A; Stassun KG; Arnold L; Benneke B; Boisse I; Bonfils X; Cook NJ; Cortés-Zuleta P; Delfosse X; do Nascimento JD; Fausnaugh M; Fong W; Fouqué P; Forveille T; Gomes da Silva J; Hesse K; Kóspál Á; Lewis H; Liu C-F; Martins JHC; Paegert M; Seager S; Shang H; Twicken JD; Vandal T; Vinatier S; Widemann T; Winn JN, "A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS" , A&A: 670, id.A136 (28 pp), Feb, 2023 [SCI] ( ADS | Fulltext )
  71. Long JD; Males JR; Haffert SY; Pearce L; Marley MS; Morzinski KM; Close LM; Otten GPPL; Snik F; Kenworthy MA; Keller CU; Hinz P; Monnier JD; Weinberger A; Tolls V, "Improved Companion Mass Limits for Sirius A with Thermal Infrared Coronagraphy Using a Vector-apodizing Phase Plate and Time-domain Starlight-subtraction Techniques" , AJ: 165(5), id.216 (14pp), May, 2023 [SCI] ( ADS | Fulltext )
  72. Orihara R; Momose M; Muto T; Hashimoto J; Liu HB; Tsukagoshi T; Kudo T; Takahashi S; Yang Y; Hasegawa Y; Dong R; Konishi M; Akiyama E, "ALMA Band 6 high-resolution observations of the transitional disk around SY Chamaeleontis" , MNRAS: 75(2), 424-445, April, 2023 [SCI] ( ADS | Fulltext )
  73. Pereira CL; Sicardy B; Morgado BE; Braga-Ribas F; Fernández-Valenzuela E; Souami D; Holler BJ; Boufleur RC; Margoti G; Assafin M; Ortiz JL; Santos-Sanz P; Epinat B; Kervella P; Desmars J; Vieira-Martins R; Kilic Y; Gomes Júnior AR; Camargo JIB; Emilio M; Vara-Lubiano M; Kretlow M; Albert L; Alcock C; Ball JG; Bender K; Buie MW; Butterfield K; Camarca M; Castro-Chacón JH; Dunford R; Fisher RS; Gamble D; Geary JC; Gnilka CL; Green KD; Hartman ZD; Huang C-K; Januszewski H; Johnston J; Kagitani M; Kamin R; Kavelaars JJ; Keller JM; de Kleer KR; Lehner MJ; Luken A; Marchis F; Marlin T; McGregor K; Nikitin V; Nolthenius R; Patrick C; Redfield S; Rengstorf AW; Reyes-Ruiz M; Seccull T; Skrutskie MF; Smith AB; Sproul M; Stephens AW; Szentgyorgyi A; Sánchez-Sanjuán S; Tatsumi E; Verbiscer A; Wang S-Y; Yoshida F; Young R; Zhang Z-W, "The two rings of (50000) Quaoar" , A&A: 673, id.L4 (14 pp), May, 2023 [SCI] ( ADS | Fulltext )
  74. Petit J-M; Gladman B; Kavelaars JJ; Bannister MT; Alexandersen M; Volk K; Chen Y-T, "The Hot Main Kuiper Belt Size Distribution from OSSOS" , ApJL: 947(1), id.L4 (9pp), April, 2023 [SCI] ( ADS | Fulltext )
  75. Christian S; Vanderburg A; Becker J; Yahalomi DA; Pearce L; Zhou G; Collins KA; Kraus AL; Stassun KG; De Beurs Z; Ricker GR; Vanderspek RK; Latham DW; Winn JN; Seager S; Jenkins JM; Abe L; Agabi K; Amado PJ; Baker D; Barkaoui K; Benkhaldoun Z; Benni P; Berberian J; Berlind P; Bieryla A; Esparza-Borges E; Bowen M; Brown P; Buchhave LA; Burke CJ; Buttu M; Cadieux C; Caldwell DA; Charbonneau D; Chazov N; Chimaladinne S; Collins KI; Combs D; Conti DM; Crouzet N; De Leon JP; Deljookorani S; Diamond B; Doyon R; Dragomir D; Dransfield G; Essack Z; Evans P; Fukui A; Gan T; Esquerdo GA; Gillon M; Girardin E; Guerra P; Guillot T; K. Habich EK; Henriksen A; Hoch N; Isogai KI; Jehin E; Jensen ELN; Johnson MC; Livingston JH; Kielkopf JF; Kim K; Kawauchi K; Krushinsky V; Kunzle V; Laloum D; Leger D; Lewin P; Mallia F; Massey B; Mori M; Mcleod KK; Mékarnia D; Mireles I; Mishevskiy N; Tamura M; Murgas F; Narita N; Naves R; Nelson P; Osborn HP; Palle E; Parviainen H; Plavchan P; Pozuelos FJ; Rabus M; Relles HM; Rodríguez López C; Quinn SN; Schmider F-X; Schlieder JE; Schwarz RP; Shporer A; Sibbald L; Srdoc G; Stibbards C; Stickler H; Suarez O; Stockdale C; Tan T-G; Terada Y; Triaud A; Tronsgaard R; Waalkes WC; Wang G; Watanabe N; Wenceslas M-S; Wingham G; Wittrock J; Ziegler C, "A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions" , AJ: 163(5), id.207 (26pp), May, 2022 [SCI] ( ADS | Fulltext )
  76. Kipping D; Bryson S; Burke C; Christiansen J; Hardegree-Ullman K; Quarles B; Hansen B; Szulágyi J; Teachey A, "An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i" , Nature Astronomy: 6, 367-380, Jan, 2022 [SCI] ( ADS | Fulltext )
  77. Martioli E; Hébrard G; Fouqué P; Artigau Ù; Donati JF; Cadieux C; Bellotti S; Lecavelier Des Etangs A; Doyon R; Do Nascimento JD; Arnold L; Carmona A; Cook NJ; Cortes-Zuleta P; De Almeida L; Delfosse X; Folsom CP; König PC; Moutou C; Ould-Elhkim M; Petit P; Stassun KG; Vidotto AA; Vandal T; Benneke B; Boisse I; Bonfils X; Boyd P; Brasseur C; Charbonneau D; Cloutier R; Collins K; Cristofari P; Crossfield I; Díaz RF; Fausnaugh M; Figueira P; Forveille T; Furlan E; Girardin E; Gnilka CL; Gomes Da Silva J; Gu PG; Guerra P; Howell SB; Hussain GaJ; Jenkins JM; Kiefer F; Latham DW; Matson RA; Matthews EC; Morin J; Naves R; Ricker G; Seager S; Takami M; Twicken JD; Vanderburg A; Vanderspek R; Winn J, "TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS" , A&A: 660, id.A86 (39 pp), Apr, 2022 [SCI] ( ADS | Fulltext )
  78. Sanghani MN; Lajaunie L; Marhas KK; Rickard WDA; Hsiao SS-Y; Peeters Z; Shang H; Lee D-C; Calvino JJ; Bizzarro M, "Microstructural and Chemical Investigations of Presolar Silicates from Diverse Stellar Environments" , ApJ: 925(2), id.110 (28pp), Feb, 2022 [SCI] ( ADS | Fulltext )
  79. Chandler CO; Trujillo CA; Hsieh HH, "Recurrent Activity from Active Asteroid (248370) 2005 QN173: A Main-belt Comet" , ApJL: 922(1), id.L8 (10pp), Nov, 2021 [SCI] ( ADS | Fulltext )
  80. Fraser WC; Benecchi SD; Kavelaars JJ; Marsset M; Pike RE; Bannister MT; Schwamb ME; Volk K; Nesvorny D; Alexandersen M; Chen Y-T; Gwyn S; Lehner MJ; Wang S-Y, "Col-OSSOS: The Distinct Color Distribution of Single and Binary Cold Classical KBOs" , The Planetary Science Journal: 2(3), id.90 (6pp), Jun, 2021 [SCI] ( ADS | Fulltext )
  81. Hoang T; Lazarian A; Lee H; Cho K; Gu P-G ; Ng C-H, "Effect of Dust Rotational Disruption by Radiative Torques and Implications for the F-corona Decrease Revealed by the Parker Solar Probe" , ApJ: 919(2), id.91 (14pp), Sep, 2021 [SCI] ( ADS | Fulltext )
  82. Kamp I; Honda M; Nomura H; Audard M; Fedele D; Waters LBFM; Aikawa Y; Banzatti A; Bowey JE; Bradford M; Dominik C; Furuya K; Habart E; Ishihara D; Johnstone D; Kennedy G; Kim M; Kral Q; Lai SP; Larsson B; Mcclure M; Miotello A; Momose M; Nakagawa T; Naylor D; Nisini B; Notsu S; Onaka T; Pantin E; Podio L; Riviere Marichalar P; Rocha WRM; Roelfsema P; Santos F; Shimonishi T; Tang YW; Takami M; Tazaki R; Wolf S; Wyatt M; Ysard N, "The formation of planetary systems with SPICA" , PASA: 38, id. e055, Nov, 2021 [SCI] ( ADS | Fulltext )
  83. Roberts AC; Muñoz-Gutiérrez MA, "Dynamics of Small Bodies in Orbits Between Jupiter and Saturn" , Icarus: 358, id.114201 (11pp), Apr, 2021 [SCI] ( ADS | Fulltext )
  84. Boley AC; Van Laerhoven C; Granados Contreras AP, "Transit Duration Variations in Multiplanet Systems" , AJ: 159(5), id.207 (12pp.), May, 2020 [SCI] ( ADS | Fulltext )
  85. Cotton DV; Bailey J; Pringle JE; ...; Marshall JP, "Polarization measurements of the polluted white dwarf G29-38" , MNRAS: 494(4), 4591-4605, Apr, 2020 [SCI] ( ADS | Fulltext )
  86. Gaslac Gallardo DM; Giuliatti Winter SM; Madeira G; Muñoz-Gutiérrez MA, "Analysing the region of the rings and small satellites of Neptune" , Ap&SS: 365(1), id. 5 (10 pp.), Jan, 2020 [SCI] ( ADS | Fulltext )
  87. Horner J; Kane SR; Marshall JP; et al., "Solar System Physics for Exoplanet Research" , PASP: 132 (1016), id.102001 (15pp.), Oct, 2020 [SCI] ( ADS | Fulltext )
  88. Lee C-H; Lin H-W; Chen Y-T; Yen S-F, "Infrared Observations of 2I/Borisov near Perihelion" , AJ: 160(3), id.132 (6pp.), Sep, 2020 [SCI] ( ADS | Fulltext )
  89. Marsset M; Fraser WC; Bannister MT; Schwamb ME; Pike RE; ...; Alexandersen M; Chen Y-T; et al., "Col-OSSOS: Compositional Homogeneity of Three Kuiper Belt Binaries" , The Planetary Science Journal: 1(1), id.16 (10pp.), June, 2020 ( ADS | Fulltext )
  90. Toalá JA; Guerrero MA; Bianchi L; Chu YH; et al., "Chandra observations of the planetary nebula IC 4593" , MNRAS: 494(3), 3784-3789, Apr, 2020 [SCI] ( ADS | Fulltext )
  91. Dong R; Liu S-Y; Fung J, "Observational Signatures of Planets in Protoplanetary Disks: Planet-Induced Line Broadening in Gaps" , ApJ: 870(2), id. 72 (15 pp.), Jan, 2019 [SCI] ( ADS | Fulltext )
  92. Horner J; Wittenmyer RA; Wright DJ; ...; Marshall JP; et al., "The HD 181433 Planetary System: Dynamics and a New Orbital Solution" , AJ: 158(3), id. 100 (12 pp.), Sep, 2019 [SCI] ( ADS | Fulltext )
  93. Lee C-H; Lin H-W; Chen Y-T; Yen S-F, "FLAMINGOS-2 Infrared Photometry of 2I/Borisov" , RNAAS: 3(12), id. 184 (3 pp.), Dec, 2019 ( ADS | Fulltext )
  94. Marsset M; Fraser WeC; Pike RE; …; Alexandersen M; Chen Y-T; ...; Lehner MJ; …; Wang S-Y; et al., "Col-OSSOS: Color and Inclination Are Correlated throughout the Kuiper Belt" , AJ: 157(3), id. 94 (17 pp.), Mar, 2019 [SCI] ( ADS | Fulltext )
  95. Nesvorný D; Vokrouhlický D; Stern AS; ...; Chen Y-T; ...; Alexandersen M, "OSSOS. XIX. Testing Early Solar System Dynamical Models Using OSSOS Centaur Detections" , AJ: 158(3), id. 132 (6 pp.), Sep, 2019 [SCI] ( ADS | Fulltext )
  96. Oshino S; Hasegawa Y; Wakita S; Matsumoto Y, "The Properties of Planetesimal Collisions under Jupiter’s Perturbation and the Application to Chondrule Formation via Impact Jetting" , AJ: 884(1), id. 37 (19 pp.), Oct, 2019 [SCI] ( ADS | Fulltext )
  97. Van Laerhoven C; Gladman B; Volk K; ...; Alexandersen M; Chen Y-T; et al., "OSSOS. XIV. The Plane of the Kuiper Belt" , AJ: 158(1), id. 49 (13 pp.), Jul, 2019 [SCI] ( ADS | Fulltext )
  98. Bannister MT; Gladman BJ; Kavelaars JJ; ...; Chen Y-T; Alexandersen M; ...; Schwamb ME; ...; Lehner M; ...; Pike RE; ...; Wang SY, "OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release" , ApJS: 236(1), 18, May, 2018 [SCI] ( ADS | Fulltext )
  99. Benecchi SD; Lisse CM; Ryan EL; ...; Schwamb ME; et al., "K2 precision lightcurve: Twelve days in the Pluto-Charon system" , Icarus: 314, 265-273, Nov, 2018 [SCI] ( ADS | Fulltext )
  100. Bott K; Bailey J; Cotton DV; ...; Marshall JP; et al., "The Polarization of the Planet-Hosting WASP-18 System" , AJ: 156(6), id. 293 (16 pp.)., Dec, 2018 [SCI] ( ADS | Fulltext )
  101. Hasegawa S; Kuroda D; Kitazato K; ...; Ohyama Y; et al., "Physical properties of near-Earth asteroids with a low delta-v: Survey of target candidates for the Hayabusa2 mission" , PASJ: 70, 114, Dec, 2018 [SCI] ( ADS | Fulltext )
  102. Holman MJ; Payne MJ; Fraser W; ...; Chen Y-T; et al., "A Dwarf Planet Class Object in the 21:5 Resonance with Neptune" , ApJL: 855(1), L6, March, 2018 [SCI] ( ADS | Fulltext )
  103. Kennedy GM; Bryden G; Ardila D; ...; Marshall JP; et al., "Kuiper Belt Analogues in Nearby M-type Planet-host Systems" , MNRAS: 476(4), 4584-4591, June, 2018 [SCI] ( ADS | Fulltext )
  104. Lawler SM; Shankman C; Kavelaars JJ; ...; Chen Y-T; et al., "OSSOS. VIII. The Transition between Two Size Distribution Slopes in the Scattering Disk" , AJ: 155(5), 197, May, 2018 [SCI] ( ADS | Fulltext )
  105. Lin H-W; Chen Y-T; Wang J-H; Wang S-Y; et al., "Machine-Learning-Based Real-Bogus System for HSC-SSP Moving Object Detecting Pipeline" , PASJ: 70(SP1), S39, Jan, 2018 [SCI] ( ADS | Fulltext )
  106. Pierens A; Lin M-K, "On the evolution of vortices in massive protoplanetary discs" , MNRAS: 479(4), 4878-4890, Oct, 2018 [SCI] ( ADS | Fulltext )
  107. Roelfsema PR; Shibai H; Armus L; ...; Kemper F; et al., "SPICA-A Large Cryogenic Infrared Space Telescope: Unveiling the Obscured Universe" , PASA: 35, id.e030 (17 pp.), Aug, 2018 [SCI] ( ADS | Fulltext )
  108. van Kooten EMME; Cavalcante LL; Nagashima K; ...; Peeters Z; Hsiao SSY; Shang H; Lee DC; Lee T; et al., "Isotope record of mineralogical changes in a spectrum of aqueously altered CM chondrites" , GCA: 237, 79-102, Sep, 2018 [SCI] ( ADS | Fulltext )
  109. Volk K; Murray-Clay RA; Gladman BJ; ...; Chen Y-T; et al., "OSSOS. IX. Two Objects in Neptune's 9:1 Resonance—Implications for Resonance Sticking in the Scattering Population" , AJ: 155(6), 260, June, 2018 [SCI] ( ADS | Fulltext )
  110. Wittenmyer RA; Sharma S; Stello D; ...; Marshall JP; et al., "The K2-HERMES Survey. I. Planet-candidate Properties from K2 Campaigns 1–3" , AJ: 155(2), 84, Feb, 2018 [SCI] ( ADS | Fulltext )
  111. Bannister MT; Schwamb ME; Fraser WC; …; Pike RE; …; Wang S-Y; Lehner M, "Col-OSSOS: Colors of the Interstellar Planetesimal 1I/`Oumuamua" , ApJL: 851(2), L38, Dec 20, 2017 [SCI] ( ADS | Fulltext )
  112. Bannister MT; Shankman C; Volk K; Chen Y-T; ...; Schwamb ME; ...; Wang S-Y; ...; Alexandersen M; Pike RE, "OSSOS. V. Diffusion in the Orbit of a High-perihelion Distant Solar System Object" , AJ: 153(6), 262, June, 2017 [SCI] ( ADS | Fulltext )
  113. Donati J-F; Yu L; Moutou C; ...; Takami M; et al., "The hot Jupiter of the magnetically active weak-line T Tauri star V830 Tau" , MNRAS: 465(3), 3343-3360, March, 2017 [SCI] ( ADS | Fulltext )
  114. Fraser WC; Bannister MT; Pike RE;…; Schwamb ME; …; Lehner MJ; …; Chen Y-T; Wang S-Y; Alexandersen M; et al., "All planetesimals born near the Kuiper belt formed as binaries" , Nature Astronomy: 1, 0088, April, 2017 [SCI] ( ADS | Fulltext )
  115. Garcia EV; Currie T; Guyon O; ...; Takami M; Takato N; et al., "SCExAO and GPI Y JHBand Photometry and Integral Field Spectroscopy of the Young Brown Dwarf Companion to HD 1160" , ApJ: 834(2), 162, Jan, 2017 [SCI] ( ADS | Fulltext )
  116. Hammer M; Kratter KM; Lin M-K, "Slowly-growing gap-opening planets trigger weaker vortices" , MNRAS: 466(3), 3533-3543, April, 2017 [SCI] ( ADS | Fulltext )
  117. Rich EA; Wisniewski JP; McElwain MW; ...; Takami M; et al., "The fundamental stellar parameters of FGK stars in the SEEDS survey Norman, OK 73071, USA" , MNRAS: 472(2), 1736-1752, Dec, 2017 [SCI] ( ADS | Fulltext )
  118. Shankman C; Kavelaars JJ; Bannister MT; ...; Chen Y-T; ...; Alexandersen M; et al., "OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects" , AJ: 154(2), 50, Aug, 2017 [SCI] ( ADS | Fulltext )
  119. Wittenmyer RA; Jones MI; Horner J; Kane SR; Marshall JP; et al., "The Pan-Pacific Planet Search. VII. The Most Eccentric Planet Orbiting a Giant Star" , AJ: 154(6), 274, Dec, 2017 [SCI] ( ADS | Fulltext )
  120. Yen H-W; Takakuwa S; Chu Y-H; Hirano N; Ho PTP; Kanagawa, KD; Lee C-F; Liu HB; Liu S-Y; Matsumoto T; Matsushita S; ...; Tang Y-W; Trejo A; Wu C-J, "1000 AU Exterior Arcs Connected to the Protoplanetary Disk around HL Tau" , A&A: 608, A134, Dec, 2017 [SCI] ( ADS | Fulltext )
  121. Yu L; Donati J-F; Hébrard EM; ...; Takami M; et al., "A hot Jupiter around the very active weak-line T Tauri star TAP 26" , MNRAS: 467(2), 1342-1359, May, 2017 [SCI] ( ADS | Fulltext )
  122. Asensio-Torres R; Janson M; Hashimoto J; ...; Takami M; et al., "Polarimetry and flux distribution in the debris disk around HD 32297" , A&A: 593, A73, Sept, 2016 [SCI] ( ADS | Fulltext )
  123. Bannister MT; Alexandersen M; Benecchi SD; Chen Y-T; ...; Lehner MJ; ...; Schwamb ME; ...; Wang S-Y; et al., "OSSOS: IV. Discovery of a dwarf planet candidate in the 9:2 resonance with Neptune" , AJ: 152(6), 212, Dec, 2016 [SCI] ( ADS | Fulltext )
  124. Bannister MT; Kavelaars JJ; Petit J-M; ...; Chen Y-T; ...; Alexandersen M; ...; ...; Lehner MJ; ...; Schwamb ME; ...; Wang S-Y, "The Outer Solar System Origins Survey. I. Design and First-quarter Discoveries" , AJ: 152(3), 70, Sept, 2016 [SCI] ( ADS | Fulltext )
  125. Barr AC; Schwamb ME, "Interpreting the Densities of the Kuiper Belt's Dwarf Planets" , MNRAS: 460(2), 1542-1548, Aug 1, 2016 [SCI] ( ADS | Fulltext )
  126. Donati JF; Moutou C; Malo L; ...; Takami M; et al., "A hot Jupiter orbiting a 2-million-year-old solar-mass T Tauri star" , Nature: 534(7609), 662, June, 2016 [SCI] ( ADS | Fulltext )
  127. Fraser WC; Alexandersen M; Schwamb ME; et al., "TRIPPy: Trailed Image Photometry in Python" , AJ: 151(6), 158, June, 2016 [SCI] ( ADS | Fulltext )
  128. Kimura M; Isogai K; Kato T; ...; Chen Y-T; King S-K; Wen C-Y; Wang SY; Lehner MJ; Schwamb ME; Wang J-H; Zhang Z-W; ...;Cook KH; Kim D-W; Lee T;et al. (the TAOS collaboration), "Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni" , Nature: 529(7584), 54-58, Jan, 2016 [SCI] ( ADS | Fulltext )
  129. Lin HW; Chen Y-T; et al., "The Pan-STARRS 1 Discoveries of Five New Neptune Trojans" , AJ: 152(5), 147, Nov, 2016 [SCI] ( ADS | Fulltext )
  130. Ryu T; Sato B; Kuzuhara M; ...; Takami M; et al., "High-contrast Imaging of Intermediate-mass Giants with Long-term Radial Velocity Trends" , ApJ: 825(2), 127, July 10, 2016 [SCI] ( ADS | Fulltext )
  131. Schmitt JR; Tokovinin A; Wang J; ...; Schwamb ME; et al., "Planet Hunters. X. Searching for Nearby Neighbors of 75 Planet and Eclipsing Binary Candidates from the K2 Kepler extended mission" , AJ: 151(6), 159, June, 2016 [SCI] ( ADS | Fulltext )
  132. Shankman C.; Kavelaars JJ.; Gladman BJ; Alexandersen M; ...; Chen Y-T; et al., "OSSOS. II. A Sharp Transition in the Absolute Magnitude Distribution of the Kuiper Belt’s Scattering Population" , AJ: 151(2), 31, Feb, 2016 [SCI] ( ADS | Fulltext )
  133. Thompson MA*; Scicluna P; Kemper F; …; Morata O; …; Ho PTP; et al., "Constraints on the circumstellar dust around KIC 8462852" , MNRAS: 458(1), L39-L43, May, 2016 [SCI] ( ADS | Fulltext )
  134. Volk K; Murray-Clay R; Gladman B; ...; Alexandersen M; Chen Y-T; et al., "OSSOS III—Resonant Trans-Neptunian Populations: Constraints from the first quarter of the Outer Solar System Origins Survey" , AJ: 152(1), 23, July, 2016 [SCI] ( ADS | Fulltext )
  135. ALMA Partnership; Brogan CL; Pérez LM; ...; Matsushita S; ...; Takahashi S; Lee C-F; ...; Takakuwa S; ...; Liu H-Y; et al., "The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL Tau Region" , ApJL: 808(1), L3, July 20, 2015 [SCI] ( ADS | Fulltext )
  136. ALMA Partnership; Hunter TR; Kneissl R; Matsushita S; et al., "The 2014 ALMA Long Baseline Campaign: Observations of Asteroid 3 Juno at 60 Kilometer Resolution" , ApJL: 808(1), L2, July 20, 2015 [SCI] ( ADS | Fulltext )
  137. Denneau L; Jedicke R; Fitzsimmons A; Hsieh H; et al., "Observational constraints on the catastrophic disruption rate of small main belt asteroids" , Icarus: 245, 1-15, Jan 1, 2015 [SCI] ( ADS | Fulltext )
  138. Donati JF; Hebrard E; Hussain GAJ;...; Takami M; et al., "Magnetic activity and hot Jupiters of young Suns: the weak-line T Tauri stars V819 Tau and V830 Tau" , MNRAS: 453(4), 3706-3719, Nov 11, 2015 [SCI] ( ADS | Fulltext )
  139. Jewitt D; Hsieh H; Agarwal J, "The active asteroids" , Asteroids IV, 221–241, 2015 ( ADS | Fulltext )
  140. Lin HW; Yoshida F; Chen YT; Ip WH; Chang CK, "A search for subkilometer-sized ordinary chondrite like asteroids in the main-belt" , Icarus: 254, 202-212, July 1, 2015 [SCI] ( ADS | Fulltext )
  141. Bonnefoy M; Currie T; Marleau G-D; ...; Takami M; et al., "Characterization of the gaseous companion κ Andromedae b. New Keck and LBTI high-contrast observations" , A&A: 562, A111, Feb, 2014 [SCI] ( ADS | Fulltext )
  142. Boxe CS; Francisco JS; Shia R-L; Yung YL; Nair H; Liang M-C; Saiz-Lopez A, "New insights into martian atmospheric chemistry" , Icarus: 242, 97-104., Nov 1, 2014 [SCI] ( ADS | Fulltext )
  143. Brandt TD; Kuzuhara M; McElwain MW; ...; Takami M; et al., "The Moving Group Targets of the SEEDS High-contrast Imaging Survey of Exoplanets and Disks: Results and Observations from the First Three Years" , ApJ: 786(1), 1, May, 2014 [SCI] ( ADS | Fulltext )
  144. Brandt TD; McElwain MW; Turner EL; ...; Takami M; et al., "A Statistical Analysis of SEEDS and Other High-contrast Exoplanet Surveys: Massive Planets or Low-mass Brown Dwarfs?" , ApJ: 794(2), 159, Oct 20, 2014 [SCI] ( ADS | Fulltext )
  145. Cordiner MA; Nixon CA; Teanby NA; ...; Kuan Y-J; Remijan AJ, "ALMA Measurements of the HNC and HC3N Distributions in Titan's Atmosphere" , ApJL: 795(2), L30, Nov, 2014 [SCI] ( ADS | Fulltext )
  146. Dutrey A; Di Folco E; Guilloteau S; ...; Tang YW, "Possible planet formation in the young, low-mass, multiple stellar system GG Tau A" , Nature: 514(7524), 600-602, Oct 30, 2014 [SCI] ( ADS | Fulltext )
  147. Gicquel A; Milam SN; Villanueva GL; ...; Kuan YJ, "Ground-based Multiwavelength Observations of Comet 103P/Hartley 2" , ApJ: 794(1), 10, Oct 10, 2014 [SCI] ( ADS | Fulltext )
  148. Ishiguro M; Kuroda D; Hasegawa S; ...; Hsieh HH; et al., "Optical Properties of (162173) 1999 JU3: In Preparation for the JAXA Hayabusa 2 Sample Return Mission" , ApJ: 792(1), 74, Sept 1, 2014 [SCI] ( ADS | Fulltext )
  149. Lin HW; Chen YT; Lacerda P; et al., "Pan-STARRS 1 Observations of the Unusual Active Centaur P/2011 S1(Gibbs)" , AJ: 147(5), 114, May, 2014 [SCI] ( ADS | Fulltext )
  150. Lin YC; Huh CA; Hsu SC; Lin CY; Liang MC; Lin PH, "Stratospheric influence on the concentration and seasonal cycle of lower tropospheric ozone: Observation at Mount Hehuan, Taiwan" , J Geophys Res Space Atmo: 119(6), 3527-3536, Mar 27, 2014 [SCI] ( ADS | Fulltext )
  151. Mohn J; Wolf B; Toyoda S; Lin CT; Liang MC; et al., "Interlaboratory assessment of nitrous oxide isotopomer analysis by isotope ratio mass spectrometry and laser spectroscopy: current status and perspectives" , Rapid Commun. Mass Spectrom.: 28(18), 1995-2007, Sept 30, 2014 [SCI] ( ADS | Fulltext )
  152. Schmitt JR; Agol E; Deck KM; ...; Schwamb ME; et al., "Planet Hunters. VII. Discovery of a New Low-mass, Low-density Planet (PH3 C) Orbiting Kepler-289 with Mass Measurements of Two Additional Planets (PH3 B and D)" , ApJ: 795(2), 167-180, Nov, 2014 [SCI] ( ADS | Fulltext )
  153. Schmitt JR; Wang J; Fischer DA; ...; Schwamb ME; et al., "Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates from the Kepler Archival Data" , AJ: 148(2), 28, Aug, 2014 [SCI] ( ADS | Fulltext )
  154. Bu D; Shang H; Yuan F, "The effects of viscosity on circumplanetary disks" , RAA: 13(1), 71-86, Jan, 2013 [SCI] ( ADS | Fulltext )
  155. Janson M; Brandt TD; Kuzuhara M; ...; Takami M; et al., "Direct Imaging Detection of Methane in the Atmosphere of GJ 504 b" , ApJL: 778(1), L4, Nov, 2013 [SCI] ( ADS | Fulltext )
  156. Jenkins JS; Tuomi M; Brasser R; et al., "Two Super-Earths Orbiting the Solar Analog HD 41248 on the Edge of a 7:5 Mean Motion Resonance" , ApJ: 771(1), 41, July, 2013 [SCI] ( ADS | Fulltext )
  157. Yamamoto K; Matsuo T; Shibai H; ...; Takami M; et al., "Direct Imaging Search for Extrasolar Planets in the Pleiades" , PASJ: 65(4), 90, Aug, 2013 [SCI] ( ADS | Fulltext )
  158. Kim D-W; ...; King S-K; Lee T; Lehner MJ; ...; Wang J-H; Wang SY; Wen C-Y; Zhang Z-W, "The Taiwan-American Occultation Survey Project Stellar Variability. I. Detection of Low-Amplitude δ Scuti Stars" , AJ: 139(2), 757-764, Feb, 2010 [SCI] ( ADS | Fulltext )
  159. Ootsubo T; Usui F; Kawakita H; Ishiguro M; Furusho R; Hasegawa S; Ueno M; Watanabe J; Sekiguchi T; Wada T; Ohyama Y; Oyabu S; Matsuhara H; Onaka T; Nakagawa T; Murakami H, "Detection of Parent H2O and CO2 Molecules in the 2.5–5 μm Spectrum of Comet C/2007 N3 (Lulin) Observed with AKARI" , ApJ: 717(1), L66-L70, Jul 1, 2010 [SCI] ( ADS | Fulltext )
  160. Shkolnik E; Walker GAH; ...; Gu PG; et al, "Hot Jupiters and hot spots: The short- and long-term chromospheric activity on stars with giant planets" , ApJ: 622(2), 1075-1090, Apr 1, 2005 [SCI] ( ADS | Fulltext )
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