Modeling the Panchromatic Spectral Energy Distributions of Galaxies
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TLDR
An overview of the stellar population synthesis (SPS) technique and what can be reliably measured from galaxy spectral energy distributions can be found in this paper, including stellar masses, star-formation rates and histories, metallicities and abundance patterns, dust properties, and the stellar initial mass function.Abstract:
The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical property of the system, including the star-formation history, metal content, abundance pattern, dust mass, grain size distribution, star-dust geometry, and interstellar radiation field. The principal goal of stellar population synthesis (SPS) is to extract these variables from observed SEDs. In this review I provide an overview of the SPS technique and discuss what can be reliably measured from galaxy SEDs. Topics include stellar masses, star-formation rates and histories, metallicities and abundance patterns, dust properties, and the stellar initial mass function.read more
Citations
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Cosmic Star-Formation History
Piero Madau,Mark Dickinson +1 more
TL;DR: In this article, the authors review the range of complementary techniques and theoretical tools that allow astronomers to map the cosmic history of star formation, heavy element production, and reionization of the Universe from the cosmic "dark ages" to the present epoch.
Journal ArticleDOI
Cosmic Star Formation History
Piero Madau,Mark Dickinson +1 more
TL;DR: In this paper, the authors review the range of complementary techniques and theoretical tools that allow astronomers to map the cosmic history of star formation, heavy element production, and reionization of the Universe from the cosmic "dark ages" to the present epoch.
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A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
Joshua S. Speagle,Joshua S. Speagle,Charles L. Steinhardt,Charles L. Steinhardt,Peter Capak,John D. Silverman +5 more
TL;DR: In this article, the authors investigate the evolution of the star-forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out to z ~ 6.4 Gyr.
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Mesa isochrones and stellar tracks (mist). i. solar-scaled models
TL;DR: The Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project as discussed by the authors provides a set of stellar evolutionary tracks and isochrones computed using MESA, a state-of-the-art 1D stellar evolution package.
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MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
TL;DR: The Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project as mentioned in this paper provides a set of stellar evolutionary tracks and isochrones computed using MESA, a state-of-the-art 1D stellar evolution package.
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