The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years

@article{Zavala2021TheEO,
  title={The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years},
  author={Jorge A. Zavala and Caitlin M. Casey and Sinclaire M. Manning and Manuel Aravena and Matthieu B{\'e}thermin and Karina I. Caputi and David L. Clements and E. da Cunha and Patrick M. Drew and Steven L. Finkelstein and Seiji Fujimoto and Christopher C. Hayward and Jacqueline A. Hodge and Jeyhan S. Kartaltepe and K. K. Knudsen and Anton M. Koekemoer and Arianna S. Long and Georgios E. Magdis and Allison W. S. Man and Gerg{\"o} Popping and David B. Sanders and N. Z. Scoville and Kartik Sheth and Johannes G. Staguhn and Sune Toft and Ezequiel Treister and Joaquin D. Vieira and Min Su Yun},
  journal={The Astrophysical Journal},
  year={2021},
  volume={909}
}
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References

SHOWING 1-10 OF 100 REFERENCES
Galactic stellar and substellar initial mass function
We review recent determinations of the present‐day mass function (PDMF) and initial mass function (IMF) in various components of the Galaxy—disk, spheroid, young, and globular clusters—and in
The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History
We make use of sensitive (9.3 μJy beam−1 rms) 1.2 mm continuum observations from the Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble Ultra-Deep Field (ASPECS)
Physical properties and evolution of (sub-)millimetre-selected galaxies in the galaxy formation simulation shark
We thoroughly explore the properties of (sub)-millimetre (mm) selected galaxies (SMGs) in the shark semi-analytic model of galaxy formation. Compared to observations, the predicted number counts at
The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼ 5
We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR)–stellar mass (M*) relation, called the main sequence (MS) of star-forming galaxies , for
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies
We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the
The ALMA Spectroscopic Survey in the HUDF: A Model to Explain Observed 1.1 and 0.85 mm Dust Continuum Number Counts
We present a new semiempirical model for the dust continuum number counts of galaxies at 1.1 mm and 850 μm. Our approach couples an observationally motivated model for the stellar mass and star
The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts
We present the results from the 1.2 mm continuum image obtained as part of the Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field. The 1.2 mm continuum
SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies
We construct a SCUBA-2 450 μm map in the COSMOS field that covers an area of 300 arcmin2 and reaches a 1σ noise level of 0.65 mJy in the deepest region. We extract 256 sources detected at 450 μm with
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ∼1 deg2 field,
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