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1. Effects from different grades of stickiness between icy and silicate particles on carbon depletion in protoplanetary disks

2. A search for water vapor plumes on Europa by spatially resolved spectroscopic observation using Subaru/IRCS

3. Forming planetary systems that contain only minor planets

4. Monte Carlo simulation of UV-driven synthesis of complex organic molecules on icy grain surfaces

5. Global N-body Simulation of Gap Edge Structures Created by Perturbations from a Small Satellite Embedded in Saturn's Rings

6. Large planets may not form fractionally large moons

7. Effective reaction temperatures of irreversible dust chemical reactions in a protoplanetary disk

8. Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

9. Planetesimals drifting through dusty and gaseous white dwarf debris discs: Types I, II and III-like migration

10. Spin of protoplanets generated by pebble accretion: Influences of protoplanet-induced gas flow

11. Modeling the Evolution of Silicate/Volatile Accretion Discs around White Dwarfs

12. A Trio of Giant Planets Orbiting Evolved Star HD 184010

13. Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks $\rm I$. Steady-state model

14. Monte Carlo Simulation of Sugar Synthesis on Icy Dust Particles Intermittently Irradiated by UV in a Protoplanetary Disk

15. A 'no-drift' runaway pile-up of pebbles in protoplanetary disks II. Characteristics of the resulting planetesimal belt

16. ALMA High-resolution Multiband Analysis for the Protoplanetary Disk around TW Hya

17. Monte Carlo Simulation of Dust Particles in a Protoplanetary Disk: Crystalline to Amorphous Silicate Ratio in Comets

18. High Spatial Resolution Observations of Molecular Lines towards the Protoplanetary Disk around TW Hya with ALMA

19. N-body simulations of planet formation via pebble accretion II. How various giant planets form

20. Photoevaporative Dispersal of Protoplanetary Disks around Evolving Intermediate-mass Stars

21. A 'no-drift' runaway pile-up of pebbles in protoplanetary disks in which midplane turbulence increases with radius

22. Keys of a Mission to Uranus or Neptune, the Closest Ice Giants

23. Planetesimal formation around the snow line. II. Dust or pebbles?

24. Planetesimal formation around the snow line: I. Monte Carlo simulations of silicate dust pile-up in a turbulent disk

25. The impact of pre-main sequence stellar evolution on midplane snowline locations and C/O in planet forming discs

26. Orbital evolution of Saturn's satellites due to the interaction between the moons and massive Saturn's rings

27. A new and simple prescription for planet orbital migration and eccentricity damping by planet-disc interactions based on dynamical friction

28. Uranian Satellite Formation by Evolution of a Water Vapor Disk Generated by a Giant Impact

29. The Galilean Satellites Formed Slowly from Pebbles

30. Formation of rocky and icy planetesimals inside and outside the snow line: Effects of diffusion, sublimation and back-reaction

31. Effects of a Binary Companion Star on Habitability of Tidally Locked Planets around an M-type Host Star

32. Discovery of an au-scale excess in millimeter emission from the protoplanetary disk around TW Hya

33. Speeding past planets? Asteroids radiatively propelled by giant branch Yarkovsky effects

34. Gas flow around a planet embedded in a protoplanetary disc: the dependence on the planetary mass

35. Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks

36. Microlensing Results Challenge the Core Accretion Runaway Growth Scenario for Gas Giants

37. How planetary growth outperforms migration

38. Orbital evolution of Saturn's mid-sized moons and the tidal heating of Enceladus

39. Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition

40. Slowing Down Type II Migration of Gas Giants to Match Observational Data

41. The curious case of Mars formation

42. Planets around the evolved stars 24 Booties and $\gamma$ Libra: A 30d-period planet and a double giant-planet system in possible 7:3 MMR

43. TESS Discovery of a Transiting Super-Earth in the pi Mensae System

45. Satellitesimal Formation via Collisional Dust Growth in Steady Circumplanetary Disks

46. Formation of wide-orbit gas giants near the stability limit in multi-stellar systems

47. N-body simulations of planet formation via pebble accretion I: First Results

48. Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance

49. Temporary Capture of Asteroids by an Eccentric Planet

50. Formation of dust-rich planetesimals from sublimated pebbles inside of the snow line

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