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Dusty Star Forming Galaxies at High Redshift

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TLDR
In this paper, the authors summarized the current status of star-forming galaxies (DSFGs) studies, focusing especially on the detailed characterization of the best-understood subset (submillimeter galaxies), and also the selection and characterization of more recently discovered DSFG populations.
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This article is published in Physics Reports.The article was published on 2014-02-06 and is currently open access. It has received 583 citations till now. The article focuses on the topics: Luminous infrared galaxy & Galaxy.

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An alma survey of sub-millimeter galaxies in the extended chandra deep field south: physical properties derived from ultraviolet-to-radio modeling

TL;DR: In this article, the spectral energy distributions (SEDs) of star-forming galaxies were derived using an energy balance technique to connect the emission from stellar populations, dust attenuation, and dust emission in a physically consistent way.
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Cosmic X-ray surveys of distant active galaxies

TL;DR: In this paper, the authors review results from cosmic X-ray surveys of active galactic nuclei (AGNs) over the past 15 years that have dramatically improved our understanding of growing supermassive black holes in the distant universe.
References
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Journal ArticleDOI

Stellar population synthesis at the resolution of 2003

TL;DR: In this article, the spectral evolution of stellar populations at ages between 100,000 yr and 20 Gyr at a resolution of 3 A across the whole wavelength range from 3200 to 9500 A for a wide range of metallicities.
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The Luminosity function and stellar evolution

TL;DR: In this paper, the evolutionary significance of the observed luminosity function for main-sequence stars in the solar neighborhood is discussed and it is shown that stars move off the main sequence after burning about 10 per cent of their hydrogen mass and that stars have been created at a uniform rate in a solar neighborhood for the last five billion years.
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Star formation in galaxies along the hubble sequence

TL;DR: In this article, the authors focus on the broad patterns in the star formation properties of galaxies along the Hubble sequence and their implications for understanding galaxy evolution and the physical processes that drive the evolution.
Journal ArticleDOI

The Cosmological simulation code GADGET-2

TL;DR: GADGET-2 as mentioned in this paper is a massively parallel tree-SPH code, capable of following a collisionless fluid with the N-body method, and an ideal gas by means of smoothed particle hydrodynamics.
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