The accelerating expansion of the universe is the most surprising cosmological discovery in
many decades, implying that the universe is dominated by some form of “dark energy” with …

We present angular diameter measurements obtained by measuring the position of baryon
acoustic oscillations (BAO) in an optimized sample of galaxies from the first three years of …

We present a one per cent measurement of the cosmic distance scale from the detections of
the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon …

We present the angular diameter distance measurement obtained with the baryonic acoustic
oscillation (BAO) feature from galaxy clustering in the completed Dark Energy Survey …

We present angular diameter distance measurements obtained by locating the baryon
acoustic oscillations (BAO) scale in the distribution of galaxies selected from the first year of …

The simplest theory describing large-scale redshift-space distortions (RSD), based on linear
theory and distant galaxies, depends on the growth of cosmological structure, suggesting …

We present a new N-body simulation from the Marenostrum Institut de Ciències de l'Espai
(MICE) collaboration, the MICE Grand Challenge (MICE-GC), containing about 70 billion …

Cosmic voids are usually identified in spectroscopic galaxy surveys, where 3D information
about the large-scale structure of the Universe is available. Although an increasing amount …

Accurate statistical measurement with large imaging surveys has traditionally required
throwing away a sizable fraction of the data. This is because most measurements have …

We study the clustering of galaxies detected at i< 22.5 in the Science Verification
observations of the Dark Energy Survey (DES). Two-point correlation functions are …