Quantifying the evolution of higher-order clustering

Quantifying the Faint Structure of Galaxies: The Late-type Spiral NGC 2403

Quantifying the fast outflow in the luminous Seyfert galaxy PG1211+143

Quantifying the Fragility of Galactic Disks in Minor Mergers

Quantifying the heart of darkness with GHALO - a multi-billion particle simulation of our galactic halo

Quantifying the Importance of Ram Pressure Stripping in a Galaxy Group at 100 Mpc

Quantifying the Imprecision of Accretion Theory and Implications for Multi-Epoch Observations of Protoplanetary Discs

Quantifying the Luminosity Evolution in Gamma-ray Bursts

Quantifying the measurement requirements needed to understand the origin of the Galilean satellite system

Quantifying the Morphologies and Dynamical Evolution of Galaxy Clusters. II. Application to a Sample of ROSAT Clusters

Quantifying the rareness of extreme galaxy clusters

Quantifying the Significance of the Magnetic Field from Large-Scale Cloud to Collapsing Core: Self-Similarity, Mass-to-Flux Ratio and Star Formation Efficiency

Quantifying the Topology of Large-Scale Structure

Quantifying the uncertainties of chemical evolution studies. I. Stellar lifetimes and initial mass function

Quantifying the uncertainties of chemical evolution studies. I. The stellar initial mass function and the stellar lifetimes

Quantifying the uncertainties of chemical evolution studies. II. Stellar yields

Quantifying the Uncertainty in the Orbits of Extrasolar Planets

Quantifying the Uncertainty in the Orbits of Extrasolar Planets with Markov Chain Monte Carlo

Quantifying the Universality of the Stellar Initial Mass Function in Old Star Clusters

Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations