Towards accurate wave functions and oscillator strengths

Towards an open-source tool dedicated to the representation of gravitational interaction with neighbouring celestial bodies in planetary sciences

Towards Complete Microphysical Modeling of Warm Interstellar Molecules: H2 Collisional Dissociation for Spitzer IR Observations

Towards consistency in simple prescriptions for stellar convection

Towards development of a consistent orbit series for TOPEX, Jason-1, and Jason-2

Towards Forming a Primordial Protostar in a Cosmological AMR Simulation

Towards H.265 video coding standard

Towards high-resolution mantle convection simulations

Towards INPOP07, adjustments to LLR data

Towards making shift-and-add a versatile imaging technique

Towards Measuring Secular Velocity Changes in Circumstellar Shells

Towards Nonstationary, Nonparametric Independent Process Analysis with Unknown Source Component Dimensions

Towards Optimal Learning of Chain Graphs

Towards PPP-RTK: Ambiguity resolution in real-time precise point positioning

Towards self-consistent modelling of the Martian dichotomy: Coupled models of simultaneous core and crust formation

Towards self-consistent modelling of the Martian dichotomy: The influence of one-ridge convection on crustal thickness distribution

Towards Simulating a Realistic Planetary Seismic Wavefield: The Contribution of the Megaregolith and Low-Velocity Waveguides

Towards Simulating Binary Neutron Star Coalescence

Towards solution of the pulsar problem

Towards stable evolutions of excised black hole spacetimes via the ADM equations: A spherically symmetric test