We study the large-scale anisotropy of the universe by measuring the dipole in the angular
distribution of a flux-limited, all-sky sample of 1.36 million quasars observed by the Wide …

We measure a value for the cosmic expansion of H (z)= 89±23 (stat)±44 (syst) km s− 1 Mpc−
1 at a redshift of z≃ 0.47 based on the differential age technique. This technique, also known …

We present the discovery of nine quasars at $ z\sim 6$ identified in the Sloan Digital Sky
Survey (SDSS) imaging data. This completes our survey of $ z\sim 6$ quasars in the SDSS …

This paper presents cosmological results based on full-mission Planck observations of
temperature and polarization anisotropies of the cosmic microwave background (CMB) …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …

ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …

This paper presents a study of the local radio source population, by cross-comparing the
data from the first data release (DR1) of the LOFAR Two-Metre Sky Survey (LoTSS) with the …

Cosmological models with Galileon gravity are an alternative to the standard ΛCDM
paradigm with testable predictions at the level of its self-accelerating solutions for the …

In this paper, we present the GALEX–SDSS–WISE Legacy Catalog (GSWLC), a catalog of
physical properties (stellar masses, dust attenuations, and star formation rates [SFRs]) for∼ …

ABSTRACT The Galaxy And Mass Assembly (GAMA) survey furnishes a deep redshift
catalog that, when combined with the Wide-field Infrared Survey Explorer (WISE), allows us …