We measure cosmic weak lensing shear power spectra with the Subaru Hyper Suprime-
Cam (HSC) survey first-year shear catalog covering 137 deg2 of the sky. Thanks to the high …

We measure the luminosity and color dependence of galaxy clustering in the largest-ever
galaxy redshift survey, the main galaxy sample of the Sloan Digital Sky Survey Seventh Data …

We present a finely binned tomographic weak lensing analysis of the Canada–France–
Hawaii Telescope Lensing Survey (CFHTLenS) mitigating contamination to the signal from …

We present a detection of correlated clustering between MeerKAT radio intensity maps and
galaxies from the WiggleZ Dark Energy Survey. We find a 7.7 σ detection of the cross …

We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation
Spectroscopic Survey Final Data Release (BOSS DR11&DR12) with high fidelity on all …

Aims. Understanding the link between the galaxy properties and the dark matter halos they
reside in and their coevolution is a powerful tool for constraining the processes related to …

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 explore the abundance, spatial distribution, and physical properties of the O vi, O vii, and
O viii ions of oxygen in circumgalactic and intergalactic media (the CGM, IGM, and WHIM) …

Observational astrophysics consists of making inferences about the Universe by comparing
data and models. The credible intervals placed on model parameters are often as important …

We present a fast method for producing mock galaxy catalogues that can be used to
compute the covariance of large-scale clustering measurements and test analysis …