Quantifying the geometry of large-scale structure

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

Quantifying the Impact of the Sloan Digital Sky Survey: Evolving Patterns of Research Topics and Collaboration

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 Information or Relevance of Astronomical Image Data

Quantifying the inhomogeneities of matter with Supernovae and Gamma-Ray Bursts

Quantifying the ionising flux escaping from the ultra-luminous HII regions in four spiral galaxies

Quantifying the Local Environment of Low Redshift Quasars

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 Morphologies Of Galaxies At Z 1 To 4: A Multiwavelength Survey On The Progenitors Of Local Galaxies

Quantifying the Performance of Force-free Extrapolation Methods Using Known Solutions

Quantifying the rareness of extreme galaxy clusters

Quantifying the Redistribution of Mass in Galactic Disks due to Bars

Quantifying The Relationship Between Reconnection Rate And Energy Release In A Survey Of Coronal Bright Points

Quantifying The Self-helicity Of A Flux Tubes

Quantifying the Short-Period Brown Dwarf Deserts

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