The R_h = ct Universe
The S4G perspective on circumstellar dust extinction of AGB stars in M100
The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
The Satellite Luminosity Functions of Galaxies in SDSS
The SAURON Project - XIX. Optical and near-infrared scaling relations of nearby elliptical, lenticular and Sa galaxies
The SAURON project - XV. Modes of star formation in early-type galaxies and the evolution of the red sequence
The SAURON project - XVIII. The integrated UV-linestrength relations of early-type galaxies
The SAURON Project - XX. The Spitzer [3.6] - [4.5] colour in early-type galaxies: colours, colour gradients and inverted scaling relations
The SAURON project XVI: On the Sources of Ionisation for the Gas in Elliptical and Lenticular Galaxies
The SAURON project-XXI. The spatially-resolved UV-line strength relations of early-type galaxies
The scalar bi-spectrum in the Starobinsky model: The equilateral case
The Scale Dependence of the Molecular Gas Depletion Time in M33
The Scale Factor in the Universe with Dark Energy
The scale of homogeneity of the galaxy distribution in SDSS DR6
The scaling of X-ray variability with luminosity in Ultra-luminous X-ray sources
The scaling relation between richness and mass of galaxy clusters: a Bayesian approach
The scatter about the "Universal" dwarf spheroidal mass profile: A kinematic study of the M31 satellites, And V and And VI
The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM
The Science Case for PILOT II: the Distant Universe
The SDSS Coadd: 275 deg^2 of Deep SDSS Imaging on Stripe 82