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The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys

The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys

http://www.wikidata.org/entity/Q58035539

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The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z = 2.23 from HiZELS The evolving far-IR galaxy luminosity function and dust-obscured star formation rate density out to ≃Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation Which galaxies dominate the neutral gas content of the Universe?MASSIV: Mass Assembly Survey with SINFONI in VVDS MASSIV: Mass Assembly Survey with SINFONI in VVDS MASSIV: Mass Assemby Survey with SINFONI in VVDS The evolving star formation rate: M⋆relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6 Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)Evidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveys The zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8 He II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions The evolution of the [O ii], H β and [O iii] emission line luminosity functions over the last nine billions years The WIRCam Deep Survey II. Mass selected clustering The WIRCam Deep Survey I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fields The ALHAMBRA survey:B-band luminosity function of quiescent and star-forming galaxies at 0.2 ≤ z < 1 by PDF analysis Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph On the evolution of the cosmic ionizing background Galactic winds in cosmological simulations of the circumgalactic medium The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5 The Lyman continuum escape fraction of galaxies at z = 3.3 in the VUDS-LBC/COSMOS field VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 <z< 5.5 and the colour selection of high-redshift galaxies A high definition view of the COSMOS Wall atz ~ 0.73 Hidden starbursts and active galactic nuclei at 0 < z < 4 from theHerschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback Dust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxies HerMES: unveiling obscured star formation – the far-infrared luminosity function of ultraviolet-selected galaxies at z ∼ 1.5 The VIMOS Public Extragalactic Redshift Survey (VIPERS)The extended epoch of galaxy formation: Age dating of ~3600 galaxies with 2 < z < 6.5 in the VIMOS Ultra-Deep Survey The evolution of the star formation rate function in the EAGLE simulations: a comparison with UV, IR and Hα observations from z ∼ 8 to z ∼ 0 Constraints on galaxy formation models from the galaxy stellar mass function and its evolution HSTHα grism spectroscopy of ROLES: a flatter low-mass slope for thez ∼ 1 SSFR–mass relation The eagle simulations of galaxy formation: the importance of the hydrodynamics scheme Efficient satellite quenching at z∼1 from the GEEC2 spectroscopic survey of galaxy groups Dust attenuation up to z ≃ 2 in the AKARI North Ecliptic Pole Deep Field Lyman continuum escape fraction of faint galaxies at z ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC

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The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys

http://www.wikidata.org/entity/Q58035539

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im Februar 2012 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в лютому 2012

@uk

name

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@en

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@nl

type

label

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@en

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@nl

prefLabel

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@en

The star formation rate densit ...... r 12 Gyr with the VVDS surveys

@nl

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Astronomy and Astrophysics

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The star formation rate densit ...... r 12 Gyr with the VVDS surveys

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D. Maccagni

http://www.w3.org/2001/XMLSchema#string

M. Bolzonella

http://www.w3.org/2001/XMLSchema#string

O. Cucciati

http://www.w3.org/2001/XMLSchema#string

R. M. Bielby

http://www.w3.org/2001/XMLSchema#string

V. Le Brun

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Galactic Stellar and Substellar Initial Mass Function

The Luminosity Function and Stellar Evolution.

Energy input from quasars regulates the growth and activity of black holes and their host galaxies.

The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field

Cosmic Variance in the Great Observatories Origins Deep Survey

The Cosmic Evolution Survey (COSMOS): Overview

Production of dust by massive stars at high redshift

The Star Formation History of Field Galaxies

The Galaxy Luminosity Function atz≃ 1 in the HUDF: Probing the Dwarf Population

The VIMOS VLT Deep Survey: star formation rate density of Lyαemitters from a sample of 217 galaxies with spectroscopic redshifts 2 ≤ z ≤ 6.6

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31–31

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scholarly article

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10.1051/0004-6361/201118010

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539

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Marco Scodeggio

Paolo Franzetti

Giovanni Zamorani

Alessandra Zanichelli

Daniela Vergani

Sandro Bardelli

Henry Joy McCracken

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2012-02-23T00:00:00Z

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1109.1005

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2012A&A...539A..31C

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