Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …

Abstract Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation
observed at frequencies in the range≈ 10–60 GHz. AME was first detected in 1996 and …

Abstract We describe the Dark Energy Survey (DES) photometric data set assembled from
the first three years of science operations to support DES Year 3 cosmologic analyses, and …

Correcting for interstellar dust extinction is a critical step in many analyses of astrophysical
data. Indeed, a standard dust reddening map, Schlegel, Finkbeiner, and Davis (1998), is …

We use luminous red galaxies selected from the imaging surveys that are being used for
targeting by the Dark Energy Spectroscopic Instrument (DESI) in combination with CMB …

We present a new model of interstellar dust in which large grains are a single composite
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …

We present the NPIPE processing pipeline, which produces calibrated frequency maps in
temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and …

ABSTRACT We present the Emission Line Galaxy (ELG) sample of the extended Baryon
Oscillation Spectroscopic Survey from the Sloan Digital Sky Survey IV Data Release 16. We …

We present a synthesis of the astronomical observations constraining the wavelength-
dependent extinction, emission, and polarization from interstellar dust from UV to microwave …

We present a formalism for jointly fitting pre-and post-reconstruction redshift-space
clustering (RSD) and baryon acoustic oscillations (BAO) plus gravitational lensing (of the …