(Q58217161)

Guilaine Lagache

4

0 references

Emanuele Daddi

Emanuele Daddi

6

0 references

Olivier Doré

3

Olivier Doré

0 references

Mark Sargent

5

Mark Sargent

0 references

Hervé Aussel

8

Hervé Aussel

0 references

author name string

Lingyu Wang

2

0 references

Morgane Cousin

Astronomy and Astrophysics

7

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language of work or name

English

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publication date

September 2013

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published in

1 reference

SIMBAD

volume

557

1 reference

SIMBAD

page(s)

66–66

1 reference

Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar masses

SIMBAD

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1 reference

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A unified empirical model for infrared galaxy counts based on the observed physical evolution of distant galaxies

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Where stars form and live at high redshift: clues from the infrared

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A median redshift of 2.4 for galaxies bright at submillimetre wavelengths

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HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements

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Far‐infrared Source Counts at 70 and 160 Microns inSpitzerDeep Surveys

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Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA

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The Global Schmidt Law in Star‐forming Galaxies

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The evolving interstellar medium of star-forming galaxies since z = 2 as probed by their infrared spectral energy distributions

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BLAST: resolving the cosmic submillimeter background

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A Universal Density Profile from Hierarchical Clustering

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The Luminosity Function and Stellar Evolution.

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A new prescription for protogalactic feedback and outflows: where have all the baryons gone?

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Phibss: molecular gas content and scaling relations in z ~ 1-3 massive, main-sequence star-forming galaxies

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Very high gas fractions and extended gas reservoirs in z = 1.5 disk galaxies

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Correlations in the (Sub)millimeter background from ACTxBLAST

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Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies

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The lesser role of starbursts in star formation at z = 2

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The contribution of starbursts and normal galaxies to infrared luminosity functions at z < 2

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BLAST: correlations in the cosmic far-infrared background at 250, 350, and 500 {mu}m reveal clustering of star-forming galaxies

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