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

Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

We present results on the dust attenuation curve of z∼ 2 galaxies using early observations
from the MOSFIRE Deep Evolution Field survey. Our sample consists of 224 star-forming …

Two main modes of star formation are know to control the growth of galaxies: a relatively
steady one in disk-like galaxies, defining a tight star formation rate (SFR)–stellar mass …

We use the first systematic data sets of CO molecular line emission in z∼ 1–3 normal star-
forming galaxies (SFGs) for a comparison of the dependence of galaxy-averaged star …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …

We present a new, publicly available library of dust spectral energy distributions (SEDs).
These SEDs are characterized by only three parameters: the dust mass (M dust), the dust …

Aims. We study the relationship between the local environment of galaxies and their star
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …

Examining a sample of massive galaxies at 1.4< z< 2.5 with K Vega< 22 from GOODS, we
compare photometry from Spitzer at mid-and far-IR to submillimeter, radio, and rest-frame …