We review progress over the past decade in observations of large-scale star formation, with
a focus on the interface between extragalactic and Galactic studies. Methods of measuring …

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 …

Major advances in our understanding of the universe have historically arisen from dramatic
improvements in our ability to “see.” We have developed progressively larger telescopes …

An all sky map of the apparent temperature and optical depth of thermal dust emission is
constructed using the Planck-HFI (350μm to 2 mm) andIRAS (100μm) data. The optical …

We determine the magnetic field strength in the OMC 1 region of the Orion A filament via a
new implementation of the Chandrasekhar–Fermi method using observations performed as …

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite
through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ …

Planck allows unbiased mapping of Galactic sub-millimetre and millimetre emission from the
most diffuse regions to the densest parts of molecular clouds. We present an early analysis …

Anomalous microwave emission (AME) has been observed by numerous experiments in the
frequency range~ 10–60 GHz. Using Planck maps and multi-frequency ancillary data, we …

We present an analysis of the dust and gas in Andromeda, using Herschel images sampling
the entire far-infrared peak. We fit a modified-blackbody model to∼ 4000 quasi-independent …

This paper presents the first results from a comparison of Planck dust maps at 353, 545 and
857 GHz, along with IRAS data at 3000 9100 mu m) and 5000 GHz 960 mu m), with Green …